Astronomy Picture of the Day |
APOD: 2024 January 8 – The Phases of Venus
Explanation:
Venus goes through
phases.
Just like our Moon,
Venus
can appear as a full circular disk, a thin
crescent, or anything in between.
Venus, frequently the brightest object in the
post-sunset or
pre-sunrise sky, appears so small,
however, that it usually requires binoculars or a small telescope to clearly see its current phase.
The featured time-lapse sequence was taken over the course of six months in 2015 from Surgères,
Charente-Maritime,
France,
and shows not only how Venus changes phase, but changes angular size as well.
When
Venus is on the far side of the Sun from the Earth,
it appears angularly smallest and nearest to full phase, while when
Venus and Earth are on the same side of the Sun,
Venus appears larger, but as a crescent.
This month Venus rises before dawn in
waxing
gibbous
phases.
APOD: 2023 November 16 - Daytime Moon Meets Morning Star
Explanation:
Venus now
appears as Earth's brilliant morning star, shining
above the southeastern horizon before dawn.
For early morning risers, the silvery celestial
beacon rose predawn in a close pairing
with a waning crescent Moon on Thursday, November 9.
But from some
northern locations,
the Moon was seen to occult or pass in front of Venus.
From much of Europe,
the lunar occultation could be
viewed in daylight skies.
This time series composite
follows the daytime approach of Moon and morning star
in blue skies from Warsaw, Poland.
The progression of eight
sharp telescopic snapshots,
made between 10:56am and 10:58am local time,
runs from left to right, when Venus
winked out behind the bright lunar limb.
APOD: 2023 November 14 – Three Planets Rock
Explanation:
In the fading darkness before dawn,
a tilted triangle appeared to balance atop a
rock formation
off the southern tip of
Sicily.
Making up the points of the triangle are three of the four
brightest objects visible in Earth’s sky:
Jupiter,
Venus and the
Moon.
Though a thin
waning crescent,
most of the moon’s disk is visible due to
earthshine.
Captured in this image on 2022 April 27,
Venus (center) and Jupiter (left) are roughly three degrees apart --
and were headed toward a
close conjunction.
Conjunctions of
Venus and Jupiter
occur about once a year and are visible either
in the east before sunrise or in the west after sunset.
The featured image was taken
about an hour before the
arrival of the
brightest object in Earth’s sky –
the Sun.
APOD: 2023 September 15 - Venus, Moon, and the Smoking Mountain
Explanation:
Venus has returned,
now appearing in planet Earth's predawn skies
as a brilliant morning star.
From a window seat on a flight to Mexico City,
the bright celestial beacon was captured just before sunrise in
this astronomical snapshot, taken on September 12.
Venus, at the upper right, shared the early twilight
with an old crescent Moon.
Seen from this stratospheric perspective, mountain peaks and
clouds appear in silhouette along a glowing eastern horizon.
The dramatic, long, low cloud bank was created by ongoing venting
from planet Earth's active volcano
Popocatépetl.
APOD: 2023 August 26 - Crescents of Venus
Explanation:
Just as the Moon goes
through phases, Venus' visible sunlit hemisphere
waxes and wanes.
This sequence of
telescopic
images
illustrates the steady changes for Venus during
its recent 2023 apparition as our evening star.
Gliding along its interior orbit between Earth and Sun, Venus grows
larger during that period because it is approaching planet Earth.
Its crescent narrows though, as the inner planet swings closer to our
line-of-sight to the Sun.
Closest to the Earth-Sun line but passing about 8 degrees south of the
Sun, on August 13 Venus reached its (non-judgmental)
inferior conjunction.
And now Venus shines above the eastern horizon in
predawn skies, completing its transition to planet Earth's
morning star.
On August 21, NASA's Parker Solar Probe completed its sixth
gravity assist flyby of Venus, using the encounter to maneuver
the probe toward its
closest approach yet to the Sun.
APOD: 2023 July 3 – Venus in Ultraviolet from Akatsuki
Explanation:
Why is Venus so different from Earth?
To help find out,
Japan launched the robotic
Akatsuki spacecraft which
entered orbit around Venus late
in 2015 after an unplanned five-year adventure around the inner
Solar System.
Even though Akatsuki was past its original planned lifetime,
the spacecraft and instruments were operating
so well that much of its original mission was
reinstated.
Also known as the
Venus
Climate Orbiter,
Akatsuki's
instruments
investigated unknowns about Earth's sister planet, including whether
volcanoes are still active,
whether lightning occurs in the dense atmosphere, and why wind speeds
greatly exceed the planet's rotation speed.
In the featured image taken by
Akatsuki's
UVI camera, the day-side of
Venus is seen shown with planet-scale
V-shaped cloud pattern.
The image displays three
ultraviolet
colors and indicates a dip in the relative abundance of
sulfur dioxide
shown in faint blue.
Analyses of
Akatsuki images
and data has shown, among
other discoveries, that Venus has
equatorial jet similar to
Earth's jet stream.
APOD: 2023 June 26 – The Belt of Venus over Mount Everest
Explanation:
You've surely seen it, but you might not have noticed it.
During a cloudless
twilight, just before
sunrise or after
sunset, part of the atmosphere
above the horizon appears slightly dark and off-color.
Called the
Belt of Venus,
this transitional band between the dark
eclipsed sky and the bright day sky
can be seen most prominently in the direction
opposite the Sun.
Straight above,
blue sky is normal sunlight reflecting off the atmosphere, while near the horizon the clear sky can
appear more orange or red.
In the Belt of Venus, the atmosphere reflects more
light from the setting (or rising) Sun and so
appears more red.
Featured here, the
Belt of Venus was photographed over several
Himalayan mountains
including, second from the right,
Mount Everest, the
tallest mountain on
Earth.
Although usually
not mentioned, the belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2023 March 25 - Venus and the Da Vinci Glow
Explanation:
On March 23 early evening
skygazers
could watch Venus and a young crescent moon,
both near the western horizon.
On that date Earth's brilliant evening star,
faint lunar night side and slender sunlit crescent
were captured in this telephoto skyscape
posing alongside a church tower from
San Pietro di Cadore, Dolomiti, Italy.
Of course the subtle lunar illumination is
earthshine,
earthlight reflected from the Moon's night side.
A description of earthshine, in terms of sunlight
reflected by Earth's oceans illuminating
the Moon's dark surface, was written over 500 years ago by
Leonardo da Vinci.
On March 24, from
some locations the Moon
could be seen to occult or pass in front of Venus.
Around the planet tonight,
a waxing lunar crescent will appear near
the Pleiades star cluster.
APOD: 2023 March 15 – Jupiter and Venus Converge over Germany
Explanation:
This was a sky to show the kids.
Early this month the two brightest planets in the night sky,
Jupiter and Venus, appeared to
converge.
At their closest, the
two planets
were separated by only about the angular width of the
full moon.
The spectacle occurred just after sunset and was seen and
photographed all across
planet Earth.
The displayed image
was taken near to the time of closest approach from
Wiltingen,
Germany, and features the astrophotographer, spouse, and their two children.
Of course, Venus remains much closer to both the
Sun and the Earth than Jupiter --
the apparent closeness between the planets in the sky of
Earth was only
angular.
Jupiter and Venus have passed and now appear increasingly far apart.
Similar planetary convergence opportunities will
eventually arise.
In a few months, for example,
Mars and Venus
will appear to congregate just as the Sun sets.
APOD: 2023 March 6 – Jupiter and Venus from Earth
Explanation:
It was visible around the world.
The sunset conjunction of Jupiter and Venus in 2012 was visible almost
no matter where you lived on Earth.
Anyone on the planet with a clear western horizon at sunset could see them.
Pictured here in 2012, a creative photographer traveled
away from the town lights of
Szubin,
Poland to image
a near closest approach of the
two planets.
The bright planets were then separated only by
three degrees and his daughter struck a
humorous pose.
A faint red sunset still glowed in the background.
Jupiter and Venus are
together again this month after sunset,
passing within a degree of each other about a week ago.
APOD: 2023 March 5 – Jupiter and Venus over Italy
Explanation:
What are those two bright spots?
Planets.
A few days ago, the two brightest planets in the
night sky passed within a single degree of each other in what is termed a
conjunction.
Visible just after sunset in much of the world,
the two bright spots were
Jupiter (left) and
Venus (right).
The featured image was taken near closest approach from
Cirica,
Sicily,
Italy.
The week before, Venus was rising higher in the
sunset sky to meet the dropping Jupiter.
Now they have
switched places.
Of course, Venus remains much closer to both the
Sun and the Earth than Jupiter --
the apparent closeness between the planets in the sky of
Earth was only
angular.
You can still
see the
popular pair for an hour or so after sunset this month although they continue to separate, and
Jupiter continues to set earlier each night.
APOD: 2023 March 4 - 10 Days of Venus and Jupiter
Explanation:
Venus and Jupiter
may have caught your attention lately.
The impending close conjunction of the two brightest
planets visible in clear evening skies
has been
hard to miss.
With Jupiter at the top, starting on February 21 and ending on March 2,
their close approach is
chronicled daily, left to right, in these
panels from Dhanbad, India.
Near the western horizon, the evening sky colors
and exposures used for each panel depend on the local conditions near sunset.
On February 22, Jupiter and Venus were joined by the
young crescent Moon.
The celestial pair appeared to be only
the width of a full moon apart by March 2.
Of course on that date
the two planets were physically separated by over 600 million
kilometers in their
orbits around the Sun.
In the coming days
Jupiter will slowly settle into the glare at sunset,
but Venus will continue to move farther from the Sun in the
western sky to excel in its current role as the
brilliant evening star.
APOD: 2023 February 27 – Zodiacal Ray with Venus and Jupiter
Explanation:
What's causing that unusual ray of light extending from the horizon?
Dust orbiting the Sun.
At certain times of the year, a band of
sun-reflecting dust from the inner
Solar System appears prominently after sunset or before sunrise and is called
zodiacal light.
The dust was emitted mostly from faint
Jupiter-family comets and slowly spirals into the
Sun.
The featured HDR image, acquired in mid-February
from the
Sierra Nevada National Park in
Spain,
captures the glowing band of
zodiacal light going right in front of
the bright evening planets
Jupiter (upper) and
Venus (lower).
Emitted from well behind the
zodiacal light is a dark night sky that prominently
includes the
Pleiades star cluster.
Jupiter and Venus are
slowly switching places
in the
evening sky,
and just in the next few days nearing their
closest angular approach.
APOD: 2022 June 2 - Lunar Occultation of Venus
Explanation:
On May 27 Venus rose as the morning star, near the
waning crescent Moon
in a predawn sky
already full of planets.
It was close
on the sky to the Moon's crescent and a
conjunction of the second and third brightest celestial beacons
was enjoyed by skygazers around the world.
But seen from locations along a track through southeast Asia
and the Indian Ocean
the Moon actually passed in front of Venus in
a lunar occultation.
In this animated gif the 75 percent illuminated disk of
Venus approaches
and just begins to disappear behind the sunlit southwestern lunar limb.
The telescopic frames
used to construct it were captured
from Reunion Island in the Indian Ocean around 4:50am local time,
with the Moon and Venus very close to the eastern horizon.
At the time Venus
was over 180 million kilometers from Reunion Island,
compared to a lunar distance of a mere 400 thousand kilometers or so.
About 50 minutes later Venus emerged from
behind the Moon.
APOD: 2022 March 29 - Venus and Mars: Passing in the Night
Explanation:
When two planets pass on the night sky, they can usually be seen near each other for a week or more.
In the case of this planetary
conjunction, Venus and Mars passed within 4 degrees of each other earlier
this month.
The featured image was taken a few days prior, when
Venus was slowing rising in the pre-dawn sky, night by night, while
Mars was slowly setting.
The image, a four-part mosaic, was captured in
Brazil from the small town
Teresópolis.
Besides Venus and Mars,
the morning sky now also
includes the more distant planet
Saturn.
Of course, these
conjunctions are only angular --
Venus, Mars, and Saturn continue to
orbit the Sun in very different parts of
our Solar System.
Next week, the angle between
Saturn and Mars will drop to below a quarter of a degree.
APOD: 2022 March 6 - Venus and the Triply Ultraviolet Sun
Explanation:
This was a very unusual type of solar eclipse.
Typically, it is the
Earth's Moon that
eclipses the Sun.
In 2012, though, the planet
Venus took a turn.
Like a solar eclipse by the Moon, the phase of Venus became a continually thinner
crescent as Venus became increasingly better
aligned with the Sun.
Eventually the alignment became perfect and the
phase of Venus dropped to zero.
The dark spot of Venus crossed our parent star.
The situation could technically be labeled a Venusian
annular eclipse with an extraordinarily large
ring of fire.
Pictured here during the occultation, the Sun was imaged in three colors of
ultraviolet light by the Earth-orbiting
Solar Dynamics Observatory,
with the dark region toward the right corresponding to a
coronal hole.
Hours later, as Venus continued in its orbit, a
slight crescent phase appeared again.
The next Venusian transit across the Sun will occur in
2117.
APOD: 2022 January 6 - The Last Days of Venus as the Evening Star
Explanation:
That's not a young crescent Moon
posing behind cathedral towers after sunset.
It's Venus in a crescent phase.
About 40 million kilometers away and
about 2 percent
illuminated by
sunlight, it was captured with camera and telephoto lens in this series
of exposures as it set in western skies on January 1 from Veszprem,
Hungary.
The bright celestial beacon was languishing in the evening
twilight, its days as the
Evening Star
coming to a close as 2022 began.
But it was also growing larger in apparent size and becoming an
ever thinner crescent
in telescopic views.
Heading toward a (non-judgemental)
inferior
conjunction, the inner planet will be positioned
between Earth and Sun on January 9
and generally lost from view in the solar glare.
A crescent Venus will soon reappear though.
Rising in the east by mid-month just before the Sun as the brilliant
Morning Star.
APOD: 2021 July 16 - Love and War by Moonlight
Explanation:
Venus,
named for the Roman goddess of love, and
Mars,
the war god's namesake, come together
by moonlight
in this serene skyview, recorded on July 11
from Lualaba province, Democratic Republic of Congo, planet Earth.
Taken in the western twilight sky shortly after sunset
the exposure also records
earthshine illuminating the otherwise
dark surface of the
young crescent Moon.
Of course the Moon has moved on.
Venus still shines in the west though as the
evening
star, third brightest object in Earth's sky,
after the Sun and the Moon itself.
Seen here above a brilliant Venus,
Mars moved even closer
to the brighter planet and by July 13 could be seen only
about a Moon's width away.
Mars has since slowly wandered away from much brighter Venus in the
twilight, but both are sliding toward bright star Regulus.
Alpha star of the constellation Leo, Regulus lies off the
top of this frame and anticipates a
visit from Venus
and then Mars in twilight skies of
the coming days.
APOD: 2021 March 17 - The Surface of Venus from Venera 14
Explanation:
If you could stand on
Venus
-- what would you see?
Pictured is the view from Venera 14, a robotic
Soviet lander which parachuted and
air-braked down through the thick Venusian atmosphere in March of 1982.
The desolate landscape it saw included flat rocks,
vast empty terrain, and a featureless sky above
Phoebe Regio near
Venus' equator.
On the lower left is the spacecraft's
penetrometer used to make scientific measurements,
while the light piece on the right is part of an ejected lens-cap.
Enduring
temperatures near 450 degrees
Celsius and
pressures
75 times that on Earth, the hardened
Venera spacecraft lasted only about an hour.
Although data from
Venera 14
was beamed across the inner
Solar System
almost 40 years ago, digital processing and merging of
Venera's unusual images continues even today.
Recent analyses of
infrared measurements taken by
ESA's orbiting
Venus Express spacecraft indicate that active
volcanoes may currently exist on Venus.
APOD: 2021 February 25 - A Venus Flyby
Explanation:
On a mission
to explore the inner heliosphere and solar corona,
on July 11, 2020
the Wide-field Imager on board NASA's
Parker Solar Probe
captured
this stunning view
of the nightside of Venus at distance of
about 12,400 kilometers (7,693 miles).
The spacecraft was making the third of seven gravity-assist
flybys of the inner planet.
The gravity-asssist flybys are designed to
use the approach
to Venus to help the probe alter its orbit to
ultimately come within 6 million kilometers (4 million miles)
of the solar surface in late 2025.
A surprising image, the side-looking camera seems to peer through
the clouds to show a dark feature near the center
known as Aphrodite Terra,
the largest highland region on
the Venusian surface.
The bright rim at the edge of the planet is nightglow likely emitted by excited
oxygen atoms recombining into molecules in the upper reaches of the
atmosphere.
Bright streaks and blemishes throughout the image are likely due to
energetic charged particles, and dust near the camera reflecting
sunlight.
Skygazers from planet Earth
probably recognize the familiar stars of Orion's belt and sword
at lower right.
APOD: 2020 November 14 - Venus, Mercury, and the Waning Moon
Explanation:
Yesterday, early morning risers around planet Earth were treated
to a waning Moon low in the east as the sky grew
bright before dawn.
From the Island of Ortigia, Syracuse, Sicily, Italy this
simple snapshot found the slender sunlit crescent
just before sunrise.
Never wandering far from the Sun in Earth's sky, inner planets Venus
and Mercury shared the calm seaside view.
Also in the frame,
right of the line-up of Luna and planets, is bright
star Spica, alpha star of the constellation Virgo and one of the 20
brightest stars
in Earth's night.
Tomorrow the Moon will be
New.
The dark lunar disk means mostly dark nights for planet Earth in
the coming week and a good chance to watch the annual
Leonid Meteor Shower.
APOD: 2020 October 27 - Venusian Volcano Imagined
Explanation:
What would an erupting volcano on Venus look like?
Evidence of
currently active volcanoes on
Venus was
announced
earlier this year with the unexplained warmth of
regions thought to contain only ancient volcanoes.
Although large scale
images of Venus have been
taken with radar, thick
sulfuric acid
clouds would inhibit the taking of optical light vistas.
Nevertheless, an artist's reconstruction of a
Venusian volcano
erupting is featured.
Volcanoes could play an important role in a
life cycle on Venus
as they could push chemical foods into the
cooler upper atmosphere where hungry microbes might float.
Pictured,
the plume from an erupting volcano billows upwards, while a
vast lava field covers part of the hot and cracked
surface of Earth's overheated twin.
The possibility of airborne microbial Venusians is
certainly exciting, but
currently
controversial.
APOD: 2020 September 15 - Biomarker Phosphine Discovered in the Atmosphere of Venus
Explanation:
Could there be life floating in the atmosphere of Venus?
Although
Earth's planetary neighbor
has a surface considered too extreme for any known lifeform, Venus' upper atmosphere may be sufficiently mild for tiny airborne
microbes.
This usually disfavored prospect took an
unexpected upturn yesterday with the announcement of the
discovery of Venusian phosphine.
The chemical
phosphine (PH3) is a considered a
biomarker because it seems so hard to create from
routine chemical processes thought to occur on or around a
rocky world such as
Venus -- but it is known to be created by
microbial life on Earth.
The featured image of Venus and its thick clouds was taken in two bands of
ultraviolet light by
the Venus-orbing
Akatsuki, a
Japanese
robotic satellite that has been orbiting the cloud-shrouded world since 2015.
The phosphine
finding, if confirmed, may set off renewed interest
in searching for other indications of life floating high in the atmosphere of
our Solar System's second planet
out from the Sun.
APOD: 2020 June 21 - Moon Occults Venus
Explanation:
It may look like
Earthrise, but it's actually Venus-set.
Just after sunrise two days ago, both the Moon and Venus also
rose.
But then the Moon overtook
Venus.
In the
featured image sequence
centered on the Moon, Venus is shown increasingly angularly
close to the Moon.
In the
famous Earthrise image taken just over 50 years ago,
the Earth was captured rising over the edge of the Moon, as seen from the
Apollo 8
crew orbiting the Moon.
This similar Venus-set image was taken from Earth, of course, specifically
Estonia.
Venus shows only a thin crescent because last week it passed
nearly in front of the Sun, as seen from Earth.
The Moon shows only a
thin crescent
because it will soon be passing directly in front of the
Sun, as seen from Earth.
Today, in fact, two days after this image was taken, the Moon
will create a solar eclipse, with a thin swath across the Earth treated to an
annular solar eclipse.
APOD: 2020 June 8 - Atmospheric Ring of Venus
Explanation:
Why is Venus surrounded by a bright ring?
Sometimes called a
ring of fire, this
rare ring
is caused by the Sun's light being visible all around an object.
Usually seen
around the Moon during an annular solar eclipse,
the ring of fire is also visible when either
Venus or
Mercury
cross the face of our Sun.
In the
featured pictured taken last week, though,
Venus did not pass directly in front of the Sun --
the complete atmospheric ring was caused by sunlight
scattering
around the planet.
Venus passed within one degree of
the Sun during its
inferior conjunction,
as it moved from the evening to the morning sky.Â
The extreme brightness of the nearby Sun made capturing such an image very difficult -- the featured image was only made possible by using a temporary filter to block direct sunlight.
The image was captured from
Thorton,
Leicestershire,
UK.
The pervasive
blue sky glow
indicates that the image was actually captured
during the day.
APOD: 2020 June 3 - The Dance of Venus and Earth
Explanation:
Every time Venus passes the Earth, it shows the same face.
This
remarkable fact has been known for only
about 50 years, ever since
radio telescopes
have been able to peer beneath
Venus' thick clouds and track its slowly rotating surface.
This
inferior conjunction -- when Venus and Earth are the closest --
occurs today.
The featured animation
shows the positions of the Sun, Venus and Earth between 2010-2023 based on
NASA-downloaded data,
while a mock yellow 'arm' has been fixed to the ground on Venus to indicate rotation.
The reason for this unusual 1.6-year resonance
is the
gravitational influence that Earth has on Venus, which
surprisingly dominates the Sun's tidal effect.
If Venus could be seen through the
Sun's glare today,
it would show just a
very slight sliver of a
crescent.
Although previously
visible in the evening sky, starting tomorrow,
Venus
will appear in the morning sky --
on the other side of the Sun as viewed from Earth.
APOD: 2020 May 30 - Green Flashes: Sun, Moon, Venus, Mercury
Explanation:
Follow
a sunset on a clear day against a distant horizon and you might
glimpse green just as the Sun disappears from view.
The green flash
is caused by refraction of light rays traveling to the eye
over a long path through the atmosphere.
Shorter wavelengths refract more strongly than longer redder wavelengths
and the separation of colors lends a green hue to the last
visible vestige of the solar disk.
It's harder to see a
green flash from the Moon,
not to mention the diminutive disks
of Venus
and Mercury.
But a telescope or telephoto lens and camera can help
catch this tantalizing result of atmospheric refraction
when the celestial bodies are near the horizon.
From Sicily, the top panels were recorded
on March 18, 2019 for the Sun and May 8, 2020 for the Moon.
Also from the Mediterranean island,
the bottom panels were shot during the twilight apparition
of Venus and Mercury
near the western horizon on May 24.
APOD: 2020 May 29 - Mercury Meets Crescent Venus
Explanation:
That's not a bright star
and crescent Moon
caught between branches of a eucalyptus tree.
It's Venus in a crescent phase and Mercury.
Near the western horizon after sunset, the two inner planets
closely shared this telescopic field of view on May 22, seen from
a balcony in Civitavecchia, Italy.
Venus, the very bright
celestial beacon,
is wandering lower into the evening twilight.
It grows larger in apparent size and shows a
thinner crescent
as it heads toward its inferior conjunction, positioned between
Earth and Sun on June 3.
Mercury, in
a fuller phase, is climbing in the western sky though,
reaching its maximum angular distance from the Sun on June 4
Still, this
remarkably close pairing
with brilliant Venus made
Mercury, usually lost in bright twilight skies, easier to spot
from planet Earth.
APOD: 2020 May 21 - Phases of Venus
Explanation:
Just as
the Moon goes
through phases,
Venus' visible sunlit hemisphere waxes and wanes.
This composite of backyard
telescopic images illustrates the steady changes for
Venus during
its current stint as our evening star, as the inner planet grows
larger but narrows to a thin crescent.
Images from bottom to top were taken during 2020 on dates
February 27, March 20, April 14, April 24, May 8, and May 14.
Gliding along its interior orbit between Earth and Sun, Venus grows
larger during that period because it is approaching planet Earth.
Its crescent narrows, though, as Venus swings closer to our
line-of-sight to the Sun.
Closest to the Earth-Sun line but passing about 1/2 degree north of the
Sun on June 3, Venus will reach a (non-judgmental)
inferior
conjunction.
Soon after, Venus will shine clearly above the eastern horizon in
predawn skies as planet Earth's
morning star.
After sunset tonight look for Venus above the western horizon
and you can also spot
elusive innermost planet Mercury.
APOD: 2020 April 15 - A Cosmic Triangle
Explanation:
It was an astronomical triple play.
Setting on the left, just after sunset near the end of last month, was
our Moon --
showing a bright crescent phase.
Setting on the right was
Venus,
the brightest planet in the evening sky last month -- and
this month, too.
With a small telescope, you could tell that
Venus' phase was half, meaning that only half of the planet,
as visible from
Earth,
was exposed to direct sunlight and brightly lit.
High above and much further in the distance was the
Pleiades star cluster.
Although the Moon and Venus move with respect to the
background stars,
the Pleiades do not -- because they are background stars.
In the beginning of this month, Venus appeared to move
right in front of
the Pleiades,
a rare event that happens only
once every eight years.
The featured image captured
this cosmic triangle with a series of exposures taken from the same camera over 70 minutes
near Avonlea,
Saskatchewan,
Canada.
The positions of the celestial objects
was predicted.
The only thing unpredicted was the existence of the
foreground tree --
and the astrophotographer is still unsure what type of tree that is.
APOD: 2020 April 11 - Venus and the Pleiades in April
Explanation:
Shared around world in early April skies
Venus, our brilliant evening star,
wandered across the face of the lovely Pleiades star cluster.
This timelapse image follows the path of the inner planet during the
beautiful conjunction showing its daily approach to the
stars of the Seven Sisters.
From a composite of tracked exposures made with a telephoto lens,
the field of view is also appropriate for binocular equipped
skygazers.
While the star cluster and planet were easily seen with the naked-eye,
the spiky appearance of
our sister
planet in the picture is the
result of a diffraction pattern produced by the camera's lens.
All images were taken from a home garden in Chiuduno, Bergamo,
Lombardy, Italy, fortunate in good weather and clear
spring nights.
APOD: 2020 April 4 - Venus and the Sisters
Explanation:
After
wandering
about as far from the Sun on the sky as Venus can get,
the brilliant evening star is crossing paths with the sister stars of the
Pleiades cluster.
Look west after sunset and you can share
the ongoing conjunction
with skygazers
around the world.
Taken on April 2,
this celestial group photo captures the view from Portal, Arizona, USA.
Even bright naked-eye Pleiades stars prove
to be much fainter than Venus though.
Apparent in
deeper telescopic images, the cluster's dusty surroundings
and familiar bluish reflection nebulae aren't quite visible,
while brighter Venus itself is almost overwhelming in the single exposure.
And while Venus and the Sisters do look a little star-crossed,
their spiky appearance is the
diffraction
pattern caused by
multiple leaves in the aperture of the telephoto lens.
The last similar conjunction of Venus and Pleiades
occurred nearly 8 years ago.
APOD: 2020 April 2 - Venus and the Pleiades in April
Explanation:
Venus is currently the brilliant evening star.
Shared around world,
in tonight's sky Venus
will begin to wander across the face of the lovely Pleiades star cluster.
This digital sky map illustrates the path of the
inner planet
as the beautiful conjunction evolves,
showing its position on the sky over the next few days.
The field of view shown is appropriate for binocular equipped
skygazers
but the star cluster and planet are easily seen with the naked-eye.
As viewed from
our fair planet, Venus
passed in front of the stars
of the Seven Sisters 8 years ago, and will again 8 years hence.
In fact, orbiting the Sun
13 Venus years are almost equal to 8 years on planet Earth.
So we can expect our
sister planet to visit nearly the same place
in our sky every 8 years.
APOD: 2020 January 14 - Evidence of an Active Volcano on Venus
Explanation:
Are volcanoes still active on Venus?
More volcanoes are known on Venus than Earth,
but when
Venusian volcanoes last erupted is not directly known.
Evidence bolstering very recent volcanism on Venus has recently been uncovered, though, right here on Earth.
Lab results showed that images of
surface lava
would become dim in the infrared in only months in the dense Venusian atmosphere,
a dimming not seen in ESA's
Venus Express images.
Venus Express entered orbit around
Venus in 2006 and
remained in contact with Earth until 2014.
Therefore, the
infrared
glow (shown in false-color red) recorded by Venus Express for
Idunn Mons and featured here on a NASA
Magellan image
indicates that this volcano erupted very recently -- and is still active today.
Understanding the
volcanics of
Venus might lead to insight about the
volcanics on Earth, as well as
elsewhere
in
our
Solar System.
APOD: 2019 November 28 - Moon and Planets at Twilight
Explanation:
This week's ongoing conjunction
of Venus and Jupiter
may have whetted your appetite for skygazing.
Tonight is the main course though.
On November 28, a young
crescent Moon will join them posing
next to the two bright planets above the western horizon at twilight.
Much like tonight's
visual
feast, this night skyscape shows
a young lunar crescent and brilliant Venus in the western evening
twilight on October 29.
The celestial beacons are setting over distant mountains and the
Minya monastery,
Ganzi Tibetan Autonomous Prefecture, Sichuan,
China, planet Earth.
Then Mercury, not Jupiter, was a celestial companion to Venus and the Moon.
The fleeting innermost planet is just visible here in the bright
twilight,
below and left of Venus and near the center of the frame.
Tomorrow, November 29, the crescent Moon will also help you
spot planet
Saturn
for dessert.
APOD: 2019 November 26 - Venus and Jupiter on the Horizon
Explanation:
What are those two bright objects on the horizon?
Venus and
Jupiter.
The two brightest planets in the night sky
passed very close together --
angularly
-- just two days ago.
In real space, they were just about as far apart as usual,
since Jupiter (on the right) orbits the
Sun around seven times farther out than Venus.
The
planetary duo
were captured together two days ago in a picturesque sunset sky from
Llers,
Catalonia,
Spain between a tree and the astrophotographer's daughter.
These
two planets will continue to stand out in the
evening sky,
toward the west, for the next few days, with a sliver of a
crescent Moon and a fainter
Saturn also visible nearby.
As November ends, Jupiter will sink lower into the
sunset horizon with each subsequent night,
while Venus will rise higher.
The next Jupiter-Venus
conjunction will occur in early 2021.
APOD: 2019 March 4 - Celestial Alignment over Sicilian Shore
Explanation:
This was a sunrise to remember.
About a month ago, just before the
dawn of the Sun, an
impressive alignment of celestial objects was on display to the east.
Pictured, brightest and closest to the horizon, is
the Moon.
The Moon's orange glow is caused by the
scattering away of blue light by the intervening atmosphere.
Next brightest and next closest to the horizon is the
planet Venus.
Compared to
the Moon,
Venus appears more blue -- as can (also) be seen in its reflection from the water.
Next up is
Jupiter, while the bright object above Jupiter is the star
Antares.
Although this display was visible from almost anywhere on
planet Earth, the featured image was taken along a
picturesque seashore near the city of
Syracuse,
on the island of Sicily,
in the country of Italy.
This month
Saturn appears between Venus and Jupiter before sunrise, while
Mars is visible just after sunset.
APOD: 2019 February 10 - Venus Unveiled
Explanation:
What does
Venus look like beneath its thick clouds?
These clouds keep the planet's surface hidden
from even the powerful telescopic eyes of Earth-bound astronomers.
In the early 1990s, though, using imaging radar, NASA's Venus-orbiting
Magellan spacecraft was able to
lift the veil from the
face of Venus and produced spectacular
high resolution images of the planet's surface.
Colors used in this computer generated picture of
Magellan radar data are based on
color images from the surface of Venus transmitted by the
Soviet
Venera 13 and 14 landers.
The bright area running roughly across the middle
represents the largest highland region of Venus known as
Aphrodite Terra.
Venus, on the left, is about the
same size as
our Earth, shown to the right for comparison.
APOD: 2019 February 6 - Moon and Venus Appulse over a Tree
Explanation:
What's that bright spot near the Moon?
Venus.
About a week ago,
Earth's Moon appeared
unusually close to the distant planet Venus,
an angular coincidence known as an
appulse.
Similar to a
conjunction, which is a
coordinate term, an appulse refers more generally to when two celestial objects appear close together.
This Moon and Venus appulse -- once as close as 0.05 degrees -- was
captured
rising during the early morning behind
Koko
crater on the island of
O'ahu in
Hawaii,
USA.
The Moon was in a crescent phase with its lower left reflecting direct sunlight,
while the rest of the Moon is seen because of
Earthshine, sunlight first reflected from the Earth.
Some leaves and branches of a foreground
kiawe
tree are seen in silhouette in front of the bright crescent, while others,
in front of a darker background, appear white because of
forward scattering.
Appulses involving the Moon typically occur
several times a year: for example the Moon is expected
to pass within 0.20
degrees of distant Saturn on March 1.
APOD: 2018 October 5 - The Last Days of Venus as the Evening Star
Explanation:
That's not a young crescent Moon
poised above the hills along the western horizon at sunset.
It's Venus in a crescent phase.
About 54 million kilometers away and less than 20 percent illuminated,
it was captured by telescope and camera on September 30 near Bacau, Romania.
The bright celestial beacon is now languishing in the evening
twilight, its days as the Evening Star in 2018 coming to a close.
But it also grows larger in apparent size and becomes an
ever thinner crescent in
telescopic views.
Heading toward an
inferior
conjunction (non-judgmental), the inner planet will be
positioned between Earth and Sun on October 26 and lost from view
in the solar glare.
At month's end a crescent Venus will reappear in the east though,
rising just before the Sun as the brilliant
Morning Star.
APOD: 2018 July 17 - Moon and Venus over Cannon Beach
Explanation:
What's that spot next to the Moon?
Venus.
Two days ago, the crescent Moon slowly drifted past Venus, appearing
within just one degree at its closest.
This conjunction, though, was just one of several
photographic adventures for our Moon this month
(moon-th),
because, for one, a partial solar eclipse occurred
just a few days before, on July 12.
Currently, the Moon appears to be brightening, as seen from the Earth, as the fraction of its face illuminated by the Sun continues to increase.
In a few days,
the Moon
will appear more than half full, and therefore be in its
gibbous phase.
Next week the face of
the Moon
that always faces
the Earth will become, as viewed from the Earth, completely illuminated by
the Sun.
Even this full phase will bring an adventure, though, as a total eclipse of this
Thunder Moon will occur on July 27.
Don't worry about
our Luna getting tired, though, because she'll be new again next month (moon-th) -- August 11 to be exact -- just as she causes another partial eclipse of the Sun.
Pictured,
Venus and the Moon were captured from
Cannon Beach above a rock formation off the
Oregon
(USA)
coast known as the Needles.
About an hour after this image was taken,
the spin of the Earth caused both
Venus and the Moon to
set.
APOD: 2018 May 19 - Reflections of Venus and Moon
Explanation:
Posing near
the western horizon, a brilliant
evening
star and
slender young crescent shared reflections in a calm sea last
Thursday after sunset.
Recorded in this snapshot from a beach at Santa Marinella
near Rome, Italy, the lovely celestial conjunction of the
two brightest beacons in the night sky could be
enjoyed
around the world.
Seaside, light reflected by briefly horizontal surfaces of
the gentle waves forms the shimmering columns across the water.
Similar reflections by fluttering atmospheric ice crystals can
create sometimes
mysterious
pillars
of light.
Of course, earthlight itself visibly illuminates the faint
lunar night side.
APOD: 2018 March 4 - Clouds, Birds, Moon, Venus
Explanation:
Sometimes the sky above can become quite a show.
In early September of 2010, for example, the
Moon and Venus converged, creating quite a
sight by itself for
sky enthusiasts around the
globe.
From some locations, though, the sky was even more picturesque.
In the featured image taken in
Spain, a crescent Moon and the planet Venus, on the far right,
were captured during sunset posing against a deep blue sky.
In the foreground, dark
storm clouds loom across the image bottom,
while a white anvil cloud shape appears above.
Black specks dot the frame, caused by a
flock of birds taking flight.
Very soon after this picture was taken, however, the
birds passed by, the storm ended, and Venus and the Moon set.
Bright Venus is again visible just after sunset this month
(2018 March) and will appear
quite near Mercury tonight and the rest of this week.
APOD: 2018 February 4 - Venus and the Triply Ultraviolet Sun
Explanation:
An unusual type of solar eclipse occurred in 2012.
Usually it is the
Earth's Moon that
eclipses the Sun.
That year, most unusually, the planet
Venus took a turn.
Like a solar eclipse by the Moon, the phase of Venus became a continually thinner
crescent as Venus became increasingly
better aligned with the Sun.
Eventually the alignment became perfect and the
phase of Venus dropped to zero.
The dark spot of Venus crossed our parent star.
The situation could technically be labeled a Venusian
annular eclipse with an extraordinarily large
ring of fire.
Pictured here during the occultation, the Sun was imaged in three colors of ultraviolet light by the Earth-orbiting
Solar Dynamics Observatory,
with the dark region toward the right corresponding to a
coronal hole.
Hours later, as Venus continued in its orbit, a
slight crescent phase appeared again.
The next Venusian transit across the Sun will occur in
2117.
APOD: 2018 January 30 - Venus at Night in Infrared from Akatsuki
Explanation:
Why is Venus so different from Earth?
To help find out,
Japan launched the robotic
Akatsuki spacecraft which
entered orbit around Venus late
in 2015 after an unplanned five-year adventure around the inner
Solar System.
Even though Akatsuki was past its original planned lifetime,
the spacecraft and instruments were operating
so well that much of its original mission was
reinstated.
Also known as the
Venus
Climate Orbiter,
Akatsuki's
instruments
investigated unknowns about Earth's sister planet, including whether
volcanoes are still active,
whether lightning occurs in the dense atmosphere, and why wind speeds
greatly exceed the planet's rotation speed.
In the featured image taken by
Akatsuki's
IR2 camera, Venus's night side shows a jagged-edged equatorial band
of high dark clouds absorbing infrared light from hotter layers deeper in
Venus' atmosphere.
The bright orange and black stripe on the upper right is a false digital
artifact that covers part of the much brighter day side of
Venus.
Analyses of
Akatsuki images
and data has shown that Venus has
equatorial jet similar to
Earth's jet stream.
APOD: 2017 November 12 - A Happy Sky over Los Angeles
Explanation:
Sometimes, the sky may seem to smile over much of planet Earth.
On this day in 2008,
visible the world over,
was an unusual superposition of our Moon and the planets Venus and Jupiter.
Pictures taken at the right time
show a crescent Moon that appears to be a
smile when paired with the
planetary conjunction of seemingly nearby Jupiter and Venus.
Pictured here is the scene as it appeared from
Mt. Wilson Observatory
overlooking
Los Angeles,
California,
USA
after sunset on 2008 November 30.
Highest in the sky and farthest in the distance is the planet
Jupiter.
Significantly closer and visible to
Jupiter's lower left is
Venus,
appearing through Earth's atmospheric clouds as unusually blue.
On the far right, above the horizon, is our Moon, in a
waxing crescent phase.
Thin clouds illuminated by the Moon appear unusually orange.
Sprawling across the bottom of the image are the hills of Los Angeles,
many covered by a thin haze, while
LA skyscrapers are visible on the far left.
Hours after the taking of this image,
the Moon approached the distant duo, briefly
eclipsed Venus, and then moved on.
This week,
another conjunction of
Venus and Jupiter is occurring
and is visible to much of
planet Earth to the east just before sunrise.
APOD: 2017 March 17 - Phases of Venus
Explanation:
Just as
the Moon goes
through phases,
Venus' visible sunlit hemisphere waxes
and wanes.
This
composite
of telescopic images illustrates the steady changes
for the inner planet, seen in the west as the evening star,
as Venus grows larger but narrows to a thin crescent from
December 20, 2016 through March 10.
Gliding along its interior orbit between Earth and Sun, Venus grows
larger during that period because it is approaching planet Earth.
Its crescent narrows, though, as Venus swings closer to our line-of-sight
to the Sun.
Closest to the Earth-Sun line but passing about 8 degrees north of the Sun
on March 25, Venus will reach a (non-judgmental)
inferior
conjunction.
Soon after, Venus will shine clearly above the eastern horizon in
predawn skies as planet Earth's
morning star.
APOD: 2017 January 27 - Venus Through Water Drops
Explanation:
Now
the brilliant "star" in planet Earth's evening skies,
Venus is captured in this
creative astrophotograph.
Taken with a close-focusing lens on January 18 from
Milton Keynes, UK, it shows multiple images of the sky above the western
horizon shortly after sunset.
The images were created by water drops on a glass pane fixed to a tree.
Surface
tension has drawn the water drops into
simple lens-like shapes.
Refracting
light, the drops create images that are upside-down,
so the scene has been rotated to allow comfortable right-side up
viewing of a
macro-multiple-skyscape.
APOD: 2016 October 16 - Cylindrical Mountains on Venus
Explanation:
What could cause a huge cylindrical mountain to rise from the surface of Venus?
Such features that occur on Venus are known as coronas.
Pictured here in the foreground is 500-kilometer wide Atete Corona found in a region of
Venus known as the
Galindo.
The featured image was created by combining multiple
radar maps of the region to form a computer-generated three-dimensional perspective.
The series of
dark rectangles that cross the image from top to bottom were created by the imaging procedure and are not real.
The origin of massive coronas remains a
topic of research
although speculation holds they result from volcanism.
Studying Venusian coronas help scientists better understand the
inner structure of both
Venus and
Earth.
APOD: 2016 June 7 - Night on Venus in Infrared from Orbiting Akatsuki
Explanation:
Why is Venus so different from Earth?
To help find out, Japan launched the robotic
Akatsuki spacecraft which
entered orbit around Venus late
last year after an unplanned five-year adventure around the inner
Solar System.
Even though Akatsuki has passed its original planned lifetime, the spacecraft and its instruments are operating so well that much of its original mission has been
reinstated.
In the featured image taken by
Akatsuki late last month, Venus was captured in infrared light showing a surprising amount of
atmospheric structure on its night side.
The vertical orange
terminator stripe
between night and day is so wide because of light is so diffused by
Venus' thick atmosphere.
Also known as the
Venus Climate Orbiter,
Akatsuki has cameras and instruments that will
investigate unknowns about the planet, including whether
volcanoes are still active,
whether lightning occurs in the dense atmosphere, and why wind speeds
greatly exceed the planet's rotation speed.
APOD: 2016 April 14 - Full Venus and Crescent Moon Rise
Explanation:
Inner planet Venus
and a thin crescent Moon are never found
far from the Sun in planet Earth's skies.
Taken
near dawn on April 6, this timelapse composite
shows them both rising just before the Sun.
The mountaintop
Teide Observatory
domes on the fortunate island of
Tenerife appear in silhouette against the twilight.
In fact, the series of telephoto exposures follows the
occultation of Venus
by the Moon in three frames.
Far from Earth in its orbit and in a
nearly full phase, Venus was
96 percent illuminated.
Near perigee or closest approach to Earth,
the Moon's slender crescent represents about 2 percent of the
lunar disk in sunlight.
Seen in the first two exposures, the brilliant morning star only
vanishes in the third as it winks out behind the bright lunar limb.
Five minutes of the dramatic occultation at dawn is compressed into
15 seconds in this
timelapse video (vimeo).
APOD: 2015 December 10 - Daytime Moon Meets Morning Star
Explanation:
Venus now
appears as Earth's brilliant morning star, standing
in a line-up of planets above the
southeastern horizon before dawn.
For most, the silvery celestial
beacon rose predawn in a close pairing
with an old crescent Moon on Monday, December 7.
But also widely
seen from locations in North and Central
America, the lunar crescent
actually
occulted or passed in front of Venus
during Monday's daylight hours.
This time series follows the daytime approach of Moon and morning star
in clear blue skies from Phoenix, Arizona.
The progression of nine
sharp
telescopic snapshots, made between 9:30am and 9:35am local time,
runs from lower left to upper right, when Venus
winked out behind the
bright lunar limb.
APOD: 2015 November 3 - Seeking Venus under the Spitzkoppe Arch
Explanation:
What's that in the sky?
Although there was much to see in
this spectacular panorama
taken during the early morning hours of a day in late September,
the brightest object in the sky was clearly the planet Venus.
In the featured image,
Venus was captured actually through a natural rock bridge, itself picturesque, in
Spitzkoppe,
Namibia.
The planet, on the left of the opening, was complemented by a
silhouette of the astrophotographer on the right.
Above and beyond the
rock bridge were many famous icons of a dark night sky, including, from left to right, the
Pleiades star cluster, the
Orion Nebula, the bright star
Sirius, and the
Large and
Small Magellanic Clouds.
This week,
Venus remains visible to the east in the
pre-dawn sky,
being complemented by Mars, which is
angularly quite close.
APOD: 2015 October 25 - Jupiter and Venus from Earth
Explanation:
It was visible around the world.
The sunset conjunction of Jupiter and Venus in 2012 was visible almost
no matter where you lived on Earth.
Anyone on the planet with a clear western horizon at sunset could see them.
Pictured above in 2012, a creative photographer traveled
away from the town lights of
Szubin,
Poland to image
a near closest approach of the
two planets.
The bright planets were separated only by
three degrees and his daughter striking a
humorous pose.
A faint red sunset still glowed in the background.
Jupiter and Venus will be
at it again this week before sunrise, passing
under two degree from each other -- and even with
bonus planet Mars nearby.
APOD: 2015 July 23 - Comet PanSTARRS, Moon, and Venus
Explanation:
It is the object to the left of the big tree that's generating much recent excitement.
If you look closely, there you can see
Comet PanSTARRS, complete with
two tails.
During July, this comet has
increased markedly in brightness and has just
passed its closest approach to Earth.
The statuesque tree in the center is a
Norfolk Island Pine,
and to either side of this tree are
New
Zealand Pohutukawa trees.
Over the trees, far in the distance, are
bright Venus and an even brighter crescent
Moon.
If you look even more closely, you can find
Jupiter hidden in the branches of the pine.
The featured image was taken a few days ago in
Fergusson Park,
New Zealand, looking over
Tauranga Harbour Inlet.
In the coming days and weeks,
Comet C/2014 Q1 (PANSTARRS)
will slowly move away from the Sun and the Earth,
drift deep into southern skies, and fade.
APOD: 2015 July 3 - Venus and Jupiter are Far
Explanation:
On June 30 Venus and Jupiter were actually far apart, but both
appeared close in western skies at dusk.
Near the culmination of this year's
gorgeous conjunction,
the two bright evening planets are captured in the same telescopic
field of view in this sharp digital
stack of images
taken after sunset from Poznań in west-central Poland.
In fact, banded gas giant Jupiter was about 910 million kilometers
from Poland.
That's over 11 times farther than crescent Venus, only 78 million
kilometers distant at the time.
But since the diameter of giant planet Jupiter is over 11 times
larger than Venus both planets show about the same
angular size.
Of course, 16th century Polish astronomer Nicolaus Copernicus
would also have enjoyed the simultaneous telescopic view
including Jupiter's four Galilean moons and a crescent Venus.
Observations of Jupiter's moons and Venus' crescent phase
were evidence for
the
Copernican or heliocentric model of the solar system.
APOD: 2015 July 2 - Venus and Jupiter are Close
Explanation:
On June 30, Venus and Jupiter were close in western skies at dusk.
Near the culmination of this year's
gorgeous conjunction,
the two bright evening planets are captured in the same telescopic
field of view in this image taken after sunset from Bejing, China.
As the two bright planets set
together in the west,
a nearly Full Moon rose above the horizon to the south and east.
Imaged that night with the same telescope and camera,
the rising Moon from the opposite part of the sky is compared
with the planetary conjunction
for scale in the
digitally composited image.
The full lunar disk covers an angle of about 1/2 degree on the sky.
Visible as well in binoculars and small telescopes are
Venus' crescent and Jupiter's four Galilean moons.
Of course, Venus and Jupiter
are still close.
APOD: 2015 July 1 - Venus, Jupiter, and Noctilucent Clouds
Explanation:
Have you seen the passing planets yet?
Today the planets Jupiter and Venus pass within half a degree of each other
as seen from Earth.
This conjunction, visible all over the world, is
quite easy to see --
just look
to the west shortly after sunset.
The brightest objects visible above the horizon will be
Venus and Jupiter, with Venus being the brighter of the two.
Featured above,
the closing planets were captured two nights ago in a sunset sky
graced also by high-level
noctilucent clouds.
In the foreground, the astrophotographer's sister takes in the vista from a bank of the
Sec Reservoir in the
Czech Republic.
She reported this as the first time she has seen
noctilucent clouds.
Jupiter and Venus will appear even closer
together tonight and will continue to be visible in the same part of the sky until mid-August.
APOD: 2015 June 24 - Triple Conjunction Over Galician National Park
Explanation:
What are those bright objects hovering over the horizon?
Planets -- and the Moon.
First out, the horizon featured is a shoreline of the Atlantic Ocean that occurs at the
Galicia National Park in northern
Spain.
Next furthest out, on the left, is the
Moon.
Easily the brightest object on the night sky, the
Moon
here was in only a
crescent phase.
The next furthest out, on the right, is the planet
Venus, while planet Jupiter
is seen at the top of the triangle.
The long exposure from our rapidly rotating Earth made all of
celestial objects -- including the far distant stars -- appear as slight
arcs.
The featured image was taken last Sunday night.
Although the Moon's orbit has now taken it away from
this part of the sky, the planets
Venus and Jupiter can be seen superposed just after
sunset until mid-August.
The closest apparent separation of
Venus and Jupiter
will occur in one week, when the
two planets will appear
separated by less than the angular diameter of the Moon.
APOD: 2015 April 11 - Venus in the West
Explanation:
In the coming days, Venus shines near the western horizon at sunset.
To find Earth's
sister planet in twilight skies
just look for the brilliant evening star.
Tonight very close
to the Pleiades star cluster, Venus
dominates this springtime night skyscape taken only a few days
ago near the town of Lich in central Germany.
Also known as the Seven Sisters,
the stars of the compact Pleiades cluster appear above Venus in this picture.
The budding tree branches
to its left frame bright star Aldebaran,
the eye of Taurus the Bull, and the V-shaped
Hyades star cluster.
APOD: 2015 March 2 - Lenticular Cloud, Moon, Mars, Venus
Explanation:
It is not every day that such an interesting cloud
photobombs your image.
The original plan was to photograph a rare angular
conjunction
of
Mars and Venus that occurred a week and a half ago,
with the added bonus of a crescent Moon and the
International Space Station (ISS) both passing nearby.
Unfortunately, on
Madeira Island,
Portugal,
this event was clouded out.
During the next day, however, a spectacular
lenticular cloud appeared before sunset, so the
industrious astrophotographer
quickly formulated a new plan.
A close look at the
resulting image reveals the Moon visible toward the left of the frame, while underneath, near the bottom, are the famous planets with Venus being the brighter.
It was the unexpected
lenticular cloud, though, perhaps looking like some sort of futuristic
spaceship, that stole the show.
The setting Sun illuminated the stationary cloud (and everything else) from the bottom, setting up an intricate pattern of shadows, layers, and brightly illuminated regions, all seen evolving in a
corresponding video.
Mars and Venus will
next appear this close on the sky in late August,
but whether any place on Earth will catch them behind such a photogenic cloud is unknown.
APOD: 2015 February 28 - Moon-Venus-Mars Skyline
Explanation:
Taken on February 20,
five different exposures made in rapid succession
were used to created this tantalizing telephoto image.
In combination, they reveal a wide
range
of brightness visible to the eye on that frigid evening, from the
urban glow of the Quebec City skyline to the
triple conjunction of Moon, Venus and Mars.
Shortly after sunset the young Moon shows off its bright crescent
next to brilliant Venus.
Fainter Mars is near the top of the frame.
Though details in the Moon's sunlit crescent are washed out,
features on the dark, shadowed part of the lunar disk are remarkably clear.
Still lacking city lights
the lunar night is illuminated solely
by
earthshine, light reflected from the sunlit side
of planet Earth.
APOD: 2015 February 26 - Love and War by Moonlight
Explanation:
Venus,
named for the Roman goddess of love, and
Mars,
the war god's namesake, came together
by moonlight
in this lovely skyview,
recorded on February 20 from Charleston, South Carolina, USA, planet Earth.
Made in twilight with a digital camera,
the three second time exposure also records
earthshine illuminating the otherwise
dark surface of the
young crescent Moon.
Of course, the Moon has moved on from this much
anticipated triple conjunction.
Venus still shines in the west though as the
evening
star, third brightest object in Earth's sky,
after the Sun and the Moon itself.
Seen here within almost a Moon's width
of Venus, much fainter Mars approached even closer on the
following evening.
But Mars has since been moving slowly away from brilliant Venus,
though Mars is still visible too in the
western twilight.
APOD: 2015 February 20 - An Evening Sky Conjunction
Explanation:
Eight years ago, an evening sky held this lovely
pairing of a young crescent Moon
and brilliant Venus.
Seen near the western horizon, the close conjunction and its
wintry reflection were captured from Bolu, Turkey, planet Earth
on February 19, 2007.
In the 8
Earth years since
this photograph was taken
Venus
has orbited the Sun almost exactly 13 times, so the Sun and
Venus have now returned to the same the configuration in Earth's sky.
And since every 8 years
the Moon
also nearly repeats its phases for a given time of year, a very similar
crescent Moon-Venus conjunction
will again appear in planet Earth's
evening
skies tonight.
But the February 20, 2015 version of the conjunction will also
include
planet Mars.
Much fainter Mars will wander even closer to Venus by the
evening of February 21.
APOD: 2015 January 15 - Venus and Mercury at Sunset
Explanation:
Inner planets
Venus and
Mercury can never
wander far from the Sun in Earth's sky.
This week you've probably seen them both gathered near the
western horizon just
after sunset, a close conjunction of bright
celestial beacons in the fading twilight.
The pair are framed in this early evening skyview captured on
January 13 from the ruins of
Szarvasko Castle in northwestern Hungary.
Above the silhouette of the landscape's prominent volcanic hill
Venus is much the brighter, separated from Mercury by little more
than the width of two Full Moons.
On Friday, planet Earth's
early morning risers will also be
treated to a close conjunction,
when Saturn meets an old crescent Moon
near the southeastern horizon at dawn.
APOD: 2014 August 21 - Venus and Jupiter at Dawn
Explanation:
On Monday morning, Venus and Jupiter gathered close in
dawn
skies, for some separated by about
half the width of a
full moon.
It was their
closest conjunction
since 2000, captured here above the eastern horizon before sunrise.
The serene and colorful view
is from Istia beach near the city of Capoliveri on the island
of Elba.
Distant lights and rolling hills are along Italy's Tuscan coast.
Of course, the celestial pair soon wandered apart.
Brighter Venus headed lower, toward the eastern horizon and
the glare of the Sun, while Jupiter continues to rise a little higher
now in
the sky near dawn.
The two brightest planets
meet
again next June 30th, in the
evening twilight above the western horizon.
APOD: 2014 August 17 - Jupiter and Venus from Earth
Explanation:
It was visible around the world.
The sunset conjunction of Jupiter and Venus in 2012 was visible almost
no matter where you lived on Earth.
Anyone on the planet with a clear western horizon at sunset could see them.
Pictured above in 2012, a creative photographer traveled
away from the town lights of
Szubin,
Poland to image
a near closest approach of the
two planets.
The bright planets were separated only by
three degrees and his daughter striking a humorous pose.
A faint red sunset still glowed in the background.
Early tomorrow (Monday) morning, the two planets will pass even closer -- only 0.2 degrees apart as
visible from some locations -- just before sunrise.
APOD: 2013 October 18 - Venus, Zodiacal Light, and the Galactic Center
Explanation:
The bulging center of
our Milky Way Galaxy
rests on a pillar of light in this luminous skyscape.
Recorded on September 22nd in dark South African skies,
rivers of dust seem to flow downward from the galactic center
towards Antares, yellowish
alpha star of the constellation Scorpius, near the top of the scene.
The brightest celestial beacon present is not a star at all though, but
planet Venus, still dominant in the western sky after sunset.
Of course, the pillar of light stretching upward from the horizon is
Zodiacal light.
Sunlight scattered by dust along the plane of
the ecliptic creates the
zodiacal glow, prominent in the evening after twilight
during the
southern hemisphere spring.
APOD: 2013 September 19 - Moon, Venus, and Planet Earth
Explanation:
In this engaging scene
from planet Earth,
the Moon shines through cloudy skies following sunset
on the evening of September 8.
Despite the fading light, the camera's long exposure still
recorded a colorful, detailed view of a shoreline and
western horizon looking toward the island
San Gabriel from Colonia del Sacramento, Uruguay.
Lights from Buenos Aires, Argentina are along the horizon on the left,
across the broad
Rio de la Plata estuary.
The long exposure strongly overexposed the Moon and sky around it,
though.
So the photographer quickly snapped a shorter one to merge
with the first image in the area around the bright lunar disk.
As the the second image was made with a telephoto setting,
the digital merger captures both Earth and sky, exaggerating
the young Moon's slender crescent shape in relation to
the two nearby bright stars.
The more distant is
bluish Spica, alpha star
of the constellation Virgo.
Closest to the Moon is Earth's
evening star, planet Venus, emerging from
a lunar occultation.
APOD: 2013 September 13 - Crescent Moon Meets Evening Star
Explanation:
On September 8, brilliant planet Venus appearing
as the evening
star stood near a slender, crescent Moon at sunset.
The close celestial pairing or conjunction was a scene
enjoyed by
skygazers around the world.
But from some
locations in South America,
the Moon actually passed in front of Venus in a
lunar occultation.
Captured near Las Cañas, Uruguay,
this
two frame mosaic telescopic view shows the Moon and Venus
before and after the occultation.
The silvery evening star appears at right just before it winked out
behind the dark lunar limb, still in bright twilight skies.
About an hour later Venus emerged (left) along the three
day old Moon's sunlit edge.
APOD: 2013 August 20 - Venus and the Triply Ultraviolet Sun
Explanation:
An unusual type of solar eclipse occurred last year.
Usually it is the
Earth's Moon that
eclipses
the Sun.
Last June, most unusually, the planet
Venus took a turn.
Like a solar eclipse by the Moon, the phase of Venus became a continually thinner
crescent as Venus became increasingly
better aligned with the Sun.
Eventually the alignment became perfect and the
phase of Venus dropped to zero.
The dark spot of Venus crossed our parent star.
The situation could technically be labeled a Venusian
annular eclipse with an extraordinarily large
ring of fire.
Pictured above
during the occultation, the Sun was imaged in three colors of ultraviolet light by the Earth-orbiting
Solar Dynamics Observatory,
with the dark region toward the right corresponding to a
coronal hole.
Hours later, as Venus continued in its orbit, a
slight crescent phase appeared again.
The next Venusian solar eclipse will occur in
2117.
APOD: 2013 June 23 - Venus' Once Molten Surface
Explanation:
If you could look across Venus with radar eyes, what might you see?
This computer reconstruction of the surface of
Venus
was created from data from the
Magellan spacecraft.
Magellan orbited Venus and used
radar to map our
neighboring
planet's
surface between 1990 and 1994.
Magellan found many
interesting surface features,
including the large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism
is thought to have created the
domes, although the precise mechanism remains unknown.
Venus' surface is so hot and
hostile that no surface probe
has lasted
more than a few minutes.
APOD: 2013 May 12 - Clouds, Birds, Moon, Venus
Explanation:
Sometimes the sky above can become quite a show.
In early September of 2010, for example, the
Moon and Venus converged, creating quite a
sight by itself for
sky enthusiasts around the
globe.
From some locations, though, the sky was even more picturesque.
In the above image taken in
Spain, a crescent Moon and the planet Venus, on the far right,
were captured during sunset posing against a deep blue sky.
In the foreground, dark
storm clouds loom across the image bottom,
while a white anvil cloud shape appears above.
Black specks dot the frame, caused by a
flock of birds taking flight.
Very soon after this picture was taken, however, the birds passed by, the storm ended, and Venus and the Moon set.
Bright Venus again becomes visible just after sunset this 2013 May and will appear near Jupiter toward the end of the month.
APOD: 2012 June 20 - Venus Transits the Midnight Sun
Explanation:
Today's solstice,
the astronomical beginning of summer in the north,
is at 23:09 UT when the Sun reaches the northernmost declination in
its yearly trek through planet Earth's sky.
While most in the northern hemisphere will experience the longest
day of the year,
for some the Sun won't set at all,
still standing just above the horizon at midnight as
far south as about 66.6 degrees northern latitude.
Of course, as summer comes to the north the midnight Sun comes earlier
to higher latitudes.
Recorded near midnight,
this
time series from June 6 follows the Sun
gliding above a mountainous horizon
from a latitude of 69 degrees north.
The remarkable scene looks north over the Norwegian Sea from
Sortland, Norway.
The 2012 transit of Venus
is already in progress, with Earth's
sister planet in silhouette at the upper left against the bright
disk of the midnight Sun.
APOD: 2012 June 13 - A Venus Transit Over the Baltic Sea
Explanation:
Waiting years and traveling kilometers -- all to get a shot like this.
And even with all of this planning, a good bit of luck was helpful.
As the Sun rose over the
Baltic Sea last Wednesday as seen from
Fehmarn Island in northern
Germany, photographer
Jens Hackmann
was ready for the very unusual black dot of Venus to appear superimposed.
Less expected
were the textures of clouds and haze that
would tint different levels of the Sun various shades of
red.
And possibly the luckiest gift of all was a flicker of a rare
green flash at the very top of the Sun.
The above image is, of course, just one of
many
spectacular
pictures
taken last week of the last
transit
of the planet Venus across the face of the Sun for the next 105 years.
APOD: 2012 June 11 - A Venus Transit Music Video from SDO
Explanation:
What's that black dot moving across the Sun?
Venus.
Possibly the clearest view of
Venus crossing
in front of the Sun last week was from Earth orbit.
The Solar Dynamics Observatory obtained an uninterrupted vista
recording it not only in optical light but also in bands of
ultraviolet light.
Pictured above is a composite movie of the crossing set to music.
Although the event might prove
successful scientifically for better
determining components of Venus' atmosphere,
the event surely proved
successful culturally by involving
people throughout the world
in observing a rare astronomical phenomenon.
Many spectacular images of this Venus transit from around (and above) the globe are being proudly displayed.
APOD: 2012 June 9 - Venus at the Edge
Explanation:
As its June 6
2012 transit begins
Earth's sister planet
crosses the edge of the Sun in this stunning
view
from the Hinode spacecraft.
The timing of limb crossings during the
rare transits was used historically to
triangulate
the distance to Venus and
determine a value for the Earth-Sun distance
called the astronomical unit.
Still, modern
space-based views
like this one show the event against
an evocative backdrop of the turbulent solar surface with prominences
lofted above the Sun's edge by twisting magnetic fields.
Remarkably, the thin ring of light seen surrounding the planet's dark
silhouette is sunlight refracted by
Venus' thick atmosphere.
APOD: 2012 June 8 - When Venus Rises with the Sun
Explanation:
This dramatic telephoto view
across the Black Sea on June 6
finds Venus rising with the Sun,
the planet in silhouette against a ruddy and ragged solar disk.
Of course, the reddened light is due to scattering in planet
Earth's atmosphere and the rare
transit of Venus didn't
influence the strangely shaped and distorted Sun.
In fact, seeing the Sun in the shape of an
Etruscan Vase
is relatively common, especially compared to
Venus transits.
At sunset and sunrise, the effects of atmospheric refraction
enhanced by long, low, sight lines and strong
atmospheric temperature gradients produce the
visual distortions and mirages.
That situation is often favored by a
sea horizon.
APOD: 2012 June 7 - Venus Transit 2012
Explanation:
Occurring in pairs
separated by over a hundred years,
there have now been only eight transits of Venus
since the invention of the telescope in 1608.
The next will be in December of 2117.
But many modern telescopes and cameras were trained on
this week's
Venus transit, capturing the planet
in rare silhouette
against the Sun.
In this sharp telescopic view from Georgia, USA, a narrowband
H-alpha filter was used to show
the round planetary disk against a mottled solar surface with
dark filaments, sunspots, and prominences.
The transit itself lasted for 6 hours and 40 minutes.
Historically,
astronomers used timings of the transit from
different locations to triangulate the distance to Venus,
while modern astronomers actively search for planets that
transit distant suns.
APOD: 2012 June 5 - Live: Watching for Venus to Cross the Sun
Explanation:
Today Venus moves in front of the Sun.
One way to
follow this rare event
is to actively reload the above live image of the Sun during the
right time interval
and look for an unusual circular dark dot.
The smaller sprawling dark areas are
sunspots.
The circular dot is the planet
Venus.
The dark dot will only appear during a few very specific hours,
from about 22:10 on 2012 June 5 through 4:50 2012 June 6,
Universal
Time.
This transit is the rarest type of solar eclipse known --
much more rare than an eclipse of the Sun by
the Moon or even by the
planet Mercury.
In fact, the next transit of Venus across the Sun will be in 2117.
Anyone with a
clear view of the Sun can go outside and
carefully view
the transit for themselves by projecting sunlight through a
hole in a card
onto a wall.
Because this
Venus transit is so unusual and
visible from so much of the Earth, it is expected to be one of the
more photographed celestial events in history.
The above live image on the Sun is being taken by the Earth-orbiting
Solar
Dynamics Observatory and can be updated about every 15 minutes.
Editor's note: Since the transit has ended, the live image was replaced by one taken just before Venus crossed out of Sun.
APOD: 2012 June 3 - A Picturesque Venus Transit
Explanation:
The rare
transit of Venus across the face of the Sun in 2004 was one of the better-photographed events in sky history.
Both scientific and artistic images flooded in from the areas that could see
the transit: Europe and much of Asia, Africa, and North America.
Scientifically, solar photographers confirmed that the
black
drop effect is really better related to the viewing clarity of the camera or telescope than the atmosphere of Venus.
Artistically, images might be divided into several categories.
One type captures the
transit in front of a highly detailed Sun.
Another category captures a double coincidence such as both Venus and an airplane simultaneously silhouetted, or
Venus and the
International Space Station in low Earth orbit.
A third image type involves a fortuitous arrangement of interesting looking clouds, as shown by example in the
above image
taken from
North Carolina, USA.
Sky enthusiasts worldwide are abuzz about the coming transit of
Venus on Tuesday.
It is perhaps
interesting to wonder whether any person will live to see -- and remember seeing -- both Tuesday's Venus transit and the next one in 2117.
APOD: 2012 April 6 - Venus and the Sisters
Explanation:
After wandering
about as far from the Sun on the sky as Venus can get,
the brilliant evening star
crossed paths with the
Pleiades
star cluster earlier this week.
The beautiful conjunction was enjoyed by
skygazers
around the world.
Taken on April 2,
this
celestial group photo captures the view from Portal, Arizona, USA.
Also known as the Seven Sisters, even the brighter
naked-eye Pleiades stars are seen to be much fainter than Venus.
And while Venus and the sisters do look star-crossed,
their spiky appearance is the
diffraction
pattern caused by
multiple leaves in the aperture of the telephoto lens.
The last similar conjunction of Venus and Pleiades
occurred nearly 8 years ago.
As it did then,
Venus will again move on to
cross paths with the
disk of the Sun in June.
APOD: 2012 March 28 - Earthshine and Venus Over Sierra de Guadarrama
Explanation:
What just above that ridge?
The Moon.
Specifically, the Earth's Moon was caught just above the horizon in a young crescent phase.
The familiar Moon might look a bit odd as the exposure shows significant
Earthshine -- the illumination of the part of the
Moon hidden from direct sunlight by the sun-reflecting Earth.
Also captured in the image is the
bright planet Venus on the right.
Venus and Jupiter passed only three degrees from each other last week during a photogenic
planetary conjunction.
The above image was taken two days ago near
Madrid,
Spain.
The foreground horizon silhouette includes some of the Seven
Peaks of the
Sierra de Guadarrama mountain range.
Just a few minutes after this picture was taken, the Moon set.
APOD: 2012 March 18 - Jupiter and Venus from Earth
Explanation:
It was visible around the world.
The sunset conjunction of Jupiter and Venus was visible last week almost
no matter where you lived on Earth.
Anyone on the planet with a clear western horizon at sunset could see them.
This week the two are
still notable,
even though Jupiter has sunk below the brighter Venus.
And if you look higher in the sky you can see Mars as well.
Pictured
above, a creative photographer traveled
away from the town lights of
Szubin,
Poland to image
a near closest approach of the
two planets
almost a week ago.
The bright planets were separated only by
three degrees and his daughter striking a
humorous pose.
A faint red sunset still glowed in the background.
Although this conjunction is drawing to a close, another conjunction between Venus and Jupiter will occur next May.
APOD: 2012 March 1 - Multicolor Venus
Explanation:
Brilliant Venus now shines in
western
skies at twilight.
Seen as the prominent evening star, the planet is a
tantalizing
celestial beacon even for casual skygazers.
Venus can offer less than satisfying telescopic views though.
The planet is shrouded
in reflective clouds that appear
bright but featureless at the eyepiece.
Still, careful imaging with a series of color filters,
as used in these composite images, can reveal subtle cloud patterns.
Captured early
last month from a backyard observatory in Manchester,
New Hampshire, USA, the images are based on video camera frames.
The data was recorded through near-ultraviolet, green,
and
near-infrared filters (left), and
red, green, and blue filters while Venus stood high above the
western horizon just before sunset.
This season's evening apparition of Venus is the best one for northern
hemisphere observers in 7 years.
It will ultimately end with a
solar transit of the planet, the
last one to occur in your lifetime, on June 5/6.
APOD: 2012 February 29 - Moon and Planets Over Catalonia
Explanation:
Venus and Jupiter will appear unusually close in the sky over the next month.
The
planetary conjunction will be easily visible to the unaided eye because Venus will appear brighter than any background star, and Jupiter will be nearly as bright.
To see the
near-alignment, simply look to the west after sunset.
At their closest, on March 15, the
two planets will appear only about three degrees apart.
The planets will not be significantly closer in space - Venus will just be passing nearly in front of Jupiter as seen from the Earth.
In the above image composite taken late last week from
Catalonia,
Spain,
a bright crescent moon appears to the right of Venus,
while Jupiter appears near the top of the image.
The
distant
sun-illuminated spheres were photographed behind a sculpture depicting the legendary battle between a
warrior and a dragon.
A gallery of conjunction images is visible on the
Asterisk --
APOD's discussion board.
Please feel free to contribute.
The next
Jupiter-Venus conjunction will occur in May 2013.
APOD: 2012 February 13 - An Unusual Venusian Oval
Explanation:
Why would Venus appear oval?
Venus has been seen countless times from the surface of the Earth, and every time the
Earth's atmosphere
has dispersed its light to some degree.
When the air has just the right amount of dust or water droplets, small but distant objects like Venus appear spread out into an angularly large aureole.
Aureoles are not unusual to see and are frequently noted as circular
coronas around the
Sun or
Moon.
Recently, however, aureoles have been imaged that are not circular but distinctly
oval.
The above oval Venusian aureole was imaged by the
astrophotographer
who first noted the unusual phenomenon three years ago.
Initially disputed, the
unusual distortion has now been
confirmed multiple times by several different astrophotographers.
What causes the ellipticity is
currently unknown, and although several
hypotheses hold
that horizontally oriented
ice crystals are responsible, significant
discussions about it are still taking place.
APOD: 2012 February 7 - The Belt of Venus Over Mercedes Argentina
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless twilight, just before
sunrise or after
sunset,
part of the atmosphere above the horizon appears
slightly off-color, slightly pink or orange.
Called the Belt of Venus, this off-color band between the dark
eclipsed sky and the
blue sky can be seen in nearly every direction
including that opposite the Sun.
Straight above, blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the
atmosphere reflects light from the setting (or rising)
Sun which appears more red.
Below the Belt of Venus,
the atmosphere appears more dark because no sunlight reaches it.
The Belt of Venus can be seen from any location with a
clear horizon.
Pictured above
last month over Mercedes,
Argentina, a panoramic vista featuring the Belt of Venus was digitally stitched together from 16 smaller images.
The belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2011 October 16 - A Picturesque Venus Transit
Explanation:
The rare
transit of Venus across the face of the Sun in 2004 was one of the better-photographed events in sky history.
Both scientific and artistic images flooded in from the areas that could see
the transit: Europe and much of Asia, Africa, and North America.
Scientifically, solar photographers confirmed that the
black
drop effect is really better related to the viewing clarity of the camera or telescope than the atmosphere of Venus.
Artistically, images might be divided into several categories.
One type captures the
transit in front of a highly detailed Sun.
Another category captures a double coincidence such as both Venus and an airplane simultaneously silhouetted, or
Venus and the
International Space Station in low Earth orbit.
A third image type involves a fortuitous arrangement of interesting looking clouds, as shown by example in the
above image
taken from
North Carolina, USA.
The next transit of Venus across the Sun will be in 2012 June.
APOD: 2011 July 2 - Moon and Venus at Dawn
Explanation:
Brilliant Venus and a thin crescent Moon stood together
above the eastern horizon just before sunrise on June 30.
The lovely celestial pairing is captured in
this
colorful twilight skyview
overlooking a reservoir near Izmir, Turkey.
For some, the close conjunction could be viewed as a
daylight occultation.
While Venus is nearing the end of its latest
performance as planet Earth's
morning star,
the old lunar cresent, about 24 hours from its New Moon phase,
was also
bidding
farewell for now to the dawn.
In fact, for the next two nights a young Moon
can be spotted just after sunset.
Look for
a thin sunlit sliver
close to the western horizon, not far from bright planet Mercury.
APOD: 2011 February 2 - Moon and Venus over Switzerland
Explanation:
Sometimes a morning sky can be a combination of serene and surreal.
Such a sky perhaps existed before sunrise this past Sunday as viewed from a snowy slope in eastern
Switzerland.
Quiet clouds blanket the above scene, lit from beneath by lights from the village of
Trübbach.
A snow covered mountain,
Mittlerspitz, poses dramatically on the upper left, hovering over the small town of
Balzers,
Liechtenstein far below.
Peaks from the
Alps
can be seen across the far right, just below the freshly
rising Sun.
Visible on the upper right are the
crescent Moon and the bright planet
Venus.
Venus will remain in the
morning sky all month, although it will likely not be found in such a photogenic setting.
APOD: 2010 November 11 - Two Views, Two Crescents
Explanation:
Venus rose in a glowing dawn
sky on November 5th, just before the Sun.
For early morning risers, its brilliant
crescent phase
was best appreciated with binoculars or a small telescope.
On that day the crescent Venus also appeared in close conjunction with
another lovely crescent that hugs the
eastern horizon in planet Earth's morning skies, the waning
crescent Moon.
The celestial photo-op is captured here from two locations.
Left,
separated by less than a degree, the two crescents hover above
a sea of clouds.
The picture was recorded from an Alpine mountain pass not far
from Turin, Italy.
On the right
is a sharp telephoto view taken before an earlier sunrise,
farther east in the Alborz Mountains
of Iran.
In steady skies the slender Moon is still sliding toward Venus,
the bright planet's
compact
crescent just clearing the mountainous horizon.
For now, the crescent phase of Venus remains easy to enjoy
with binoculars in November's dawn skies.
The first observations of the phases of Venus, made by
Galileo with his telescope
in 1610, agreed with the predictions of the heliocentric
Copernican model of the Solar System.
APOD: 2010 October 20 - Venus Just After Sunset
Explanation:
Is that Venus or an airplane?
A common ponderable for sky enthusiasts is deciding
if that bright spot near the horizon is the planet Venus.
Usually, an airplane will show itself by
moving significantly in a few moments.
Venus will set only slowly as the Earth turns.
Still, the identification would be easier if Venus did not keep shifting its position each night.
Pictured above, Venus was captured on 44
different nights during 2006 and 2007 over the
Bolu mountains in
Turkey,
when Earth's sister planet appeared exclusively in the
evening sky.
The average spacing of the images was about five days, while the images were always taken with the
Sun about seven degrees below the horizon.
That bright spot toward the west in your
evening sky this month might be neither Venus nor an airplane, but
Mars.
APOD: 2010 September 28 - Venus South Polar Vortex
Explanation:
What's happening over the South Pole of Venus?
To find out, scientists have been studying images taken by the
robotic Venus Express spacecraft when it passes over the
lower spin axis of Earth's overheated twin.
Surprisingly, recent images from
Venus Express
do not confirm previous sightings of a double storm system there, but rather found a single unusual swirling cloud vortex.
In the above recently released image sequence taken in infrared light and digitally compressed, darker areas correspond to higher temperatures and hence lower regions of Venus' atmosphere.
Also illuminating are
recently released
movies, which show similarities between
Venus' southern vortex
and the vortex that swirls over the
South Pole of Saturn.
Understanding the peculiar dynamics of why, at times, two eddies appear, while at other times a single peculiar eddy appears, may give insight into how
hurricanes evolve on Earth, and remain a topic of research for some time.
In three months, the European
Venus Express spacecraft will be joined around Venus by the Japanese
Akatsuki satellite.
APOD: 2010 September 15 - Clouds, Birds, Moon, Venus
Explanation:
Sometimes the sky above can become quite a show.
Last week, for example, the
Moon and Venus converged, creating quite a
sight by itself for
sky enthusiasts around the
globe.
From some locations, though, the sky was even more picturesque.
In the above image taken last week from
Spain, a crescent Moon and the planet Venus, on the far right,
were captured during sunset posing against a deep blue sky.
In the foreground, dark
storm clouds loom across the image bottom,
while a white anvil cloud shape appears above.
Black specks dot the frame, caused by a
flock of birds taking flight.
Very soon after this picture was taken, however, the birds passed by, the storm ended, and Venus and the Moon set.
The Moon and Venus have now separated, although Venus will
remain visible
at sunset for the rest of this month.
APOD: 2010 August 27 - Brighter Than Mars
Explanation:
Even though you may have just read an email
claiming Mars will be incredibly bright tonight,
the brightest star on the horizon is not Mars.
From central Iran on August 24th,
the brightest star in this
twilight
desert skyview
is Venus, aka the Evening Star.
But a bright Mars is in the picture, just above and right
of more brilliant Venus.
Despite claims in the internet's
annually returning Mars Hoax
that Mars will be as big and bright as the Full Moon,
this celestial scenario is very similar to the western sky you can
see tonight.
Along with Mars, the still beautiful vista includes Spica,
alpha star of the
constellation
Virgo, above and left
of Venus.
Farther right of Venus,
Saturn peeks through the sunset's
fading glow just above the clouds.
Near the opposite horizon, the Full Moon illuminating the
desert is about 400,000 times brighter
than Mars.
APOD: 2010 August 1 - Venus Once Molten Surface
Explanation:
If you could look across Venus with
radar eyes, what might you see?
This computer reconstruction of the surface of
Venus was created from data from the
Magellan spacecraft.
Magellan orbited Venus and used
radar to map our
neighboring
planet's
surface between 1990 and 1994.
Magellan found many
interesting surface features,
including the large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism
is thought to have created the
domes, although the precise mechanism remains unknown.
Venus' surface is so hot and
hostile that no surface probe
has lasted more than a few minutes.
APOD: 2010 May 21 - Calm, Crescent Moon, and Venus
Explanation:
Last weekend, the
Moon and Venus formed a beautiful close
pair in the west after
sunset, a scene enjoyed by skygazers all
over the world.
In this lovely view of the
conjunction from Sweden,
a calm lake Vallentuna lies in the foreground with
sunset colors
still fading behind the treeline on the far shore.
The young Moon's sunlit crescent is bright, but its entire outline
can be seen
by Earthshine, light reflected from
planet Earth itself.
For well-placed skygazers,
on Sunday, May 16 the Moon actually
occulted (passed in front of) brilliant Venus.
For many, the occultation was visible
during daylight hours.
APOD: 2010 May 16 - Crescent Venus and Moon
Explanation:
There's something behind these clouds.
Those faint graceful arcs, upon inspection, are actually far, far in the distance.
They are the
Earth's Moon and the
planet Venus.
Both the Moon and Venus
are bright enough to be seen during the day, and both are quite capable of showing a
crescent phase.
To see Venus, which appears quite small, in a
crescent phase requires
binoculars or a telescope.
In the
above dramatic daytime image taken from
Budapest,
Hungary in 2004, the
Moon and Venus shared a similar crescent
phase a few minutes before the
Moon eclipsed the larger but more distant world.
Similarly, visible today in parts of Africa and Asia, a crescent Moon will again
eclipse Venus during the day.
About an hour after the above image was taken, Venus reappeared.
APOD: 2010 April 22 - Venus, Mercury, and Moon
Explanation:
Earlier this month, Venus and Mercury
climbed into the western twilight,
entertaining skygazers around
planet Earth
in a lovely conjunction of evening stars.
Combining 8 images spanning April 4 through April 15, this composite
tracks their progress through skies
above Portsmouth, UK.
Each individual image was captured at 19:50 UT.
The sequential path for both bright planets begins low and to the left.
But while Venus
continues
to swing away from the setting Sun, moving
higher above the western horizon,
Mercury first rises then falls.
Its highest point is from the image taken on April 11.
Of course on April 15, Venus and Mercury were joined by a young
crescent Moon.
APOD: 2010 April 12 - Mercury and Venus Over Paris
Explanation:
Go outside tonight and see one of the more interesting
planetary conjunctions of recent years.
Just after
sunset, the planets
Mercury and
Venus
are visible quite near each other.
Now Venus, being commonly
discernible as one of the brightest objects in the sky,
is frequently mistaken for an airplane. (Venus will set quite slowly, though.)
Mercury, however, is dimmer and usually harder to find.
Recently, though, Mercury can be
found just to the right of Venus,
appearing increasingly below the
brighter planet over the next week.
Pictured above,
Venus and Mercury were imaged next to the famous
Notre Dame Cathedral in
Paris, France.
A careful inspection of the image will further reveal
that the bright object nearly below Venus is iconic
Eiffel Tower.
APOD: 2010 April 7 - Venus and Mercury in the West
Explanation:
In this twilight skyview, a
windmill
stands in silent witness to a lovely
pairing of planets in the west.
The picture was recorded on April 5 from
Gallegos del Campo, Zamora, Spain.
Venus (left) and Mercury (right) are near their much
anticipated conjunction
in the early evening sky.
But even in the coming days, these two
evening stars will remain
close in the western
sky at sunset.
In fact, with brighter Venus as a marker,
sky watchers will have an excellent guide for
spotting Mercury
nearby, a planet often hidden in the Sun's glare.
APOD: 2010 April 4 - The Belt of Venus over the Valley of the Moon
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless twilight, just before
sunrise or after
sunset,
part of the atmosphere above the horizon appears
slightly off-color, slightly pink.
Called the Belt of Venus, this off-color band between the dark
eclipsed sky and the
blue sky can be seen in nearly every direction
including that opposite the Sun.
Straight above, blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the
atmosphere reflects light from the setting (or rising)
Sun which appears more red.
The Belt of Venus can be seen from any location with a
clear horizon.
Pictured above, the Belt of Venus was photographed above
morning fog in the
Valley of the Moon, a famous wine-producing region in northern
California,
USA.
The belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2009 April 24 - Moon and Morning Star
Explanation:
Wednesday, the Moon and Venus rose together in early morning skies.
Even through clouds, both show off a lovely crescent in this
well-composed skyscape
from Rutherford College, North Carolina, in the eastern US.
Farther west, North American skygazers could also witness
the Moon
passing in front
of Venus.
The bright planet disappeared behind the Moon's sunlit crescent
and reappeared along its darkened limb as morning
twilight gave way to
daylight hours.
Of course the dimmer lunar crescent was waning, approaching
today's New Moon phase.
Beginning a stint as the brilliant
Morning Star, Venus'
crescent is
waxing though, and will grow thicker in the coming months as
Venus rises higher
in morning skies.
APOD: 2009 April 9 - Venus Near Inferior Conjunction
Explanation:
This remarkable picture of a slender crescent Venus
was made during
daylight hours on March 26.
Venus was then very near
inferior
conjunction, its closest approach
to a point on a line directly
between Earth and the Sun.
So, daylight was a good time to carefully
record the telescopic view when both
Venus
and Sun were high in the daytime sky.
Near inferior conjunction, Venus is closest
to us and at its largest apparent size,
but Venus is also strongly backlit by sunlight, presenting
its night side partially outlined by a narrow crescent.
What makes the image remarkable are the faint arcs extending
beyond the sunlit crescent around to the night side of Venus,
due to sunlight filtering through the planet's
dense atmosphere.
Astronomer Eddie Guscott reports from his site in Essex, England
that the faint extensions came and went as the Earth's atmospheric
blurring
changed.
His image was constructed from 85 of the sharpest frames
chosen from thousands taken with a webcam and telescope.
APOD: 2009 March 6 - Crescent Moon and Venus
Explanation:
Last Friday, the Moon and Venus shared the early
evening sky in a beautiful conjunction.
Separated by only
about 2 degrees, they also were both in a crescent
phase.
Just like our Moon,
Venus
can appear as a full disk or a
thin crescent.
Frequently the brightest object in the post-sunset or pre-sunrise sky,
Venus is so small that it usually requires
binoculars or a
small telescope to clearly see its phase.
This
telescopic
image of Friday's conjunction shows off the
similar crescent phases, with the tiny
crescent Venus at the upper right.
APOD: 2008 December 6 - Lunar Diamond
Explanation:
Cameras around the globe
pointed skyward this week to
capture the
spectacular conjunction
of a crescent Moon and bright planets Venus and Jupiter.
But astronomer-artist Deirdre Kelleghan
recorded
her observations in
sketches of
the celestial event.
From Greystones, County Wicklow, Ireland, her small telescope
allowed her to follow the
accompanying lunar occultation as a
brilliant Venus disappeared behind the Moon's dark edge, then reappeared
along the bright lunar limb.
Her lovely drawing of the reemergence of Venus was made with
pastels and conte crayons on A3 size paper under very cold conditions.
She remarks, "The view as Venus once again sparkled like a
diamond stuck on the moon was stunning."
APOD: 2008 December 5 - Smile in the Sky
Explanation:
At sunset, Monday's western sky showed off stunning colors
and dramatic clouds reflected in
Brisbane Water on the Central Coast of New South Wales, Australia.
It also featured the
remarkable conjunction
of the crescent Moon,
Venus, and Jupiter forming a twilight smiley face.
While the gathering of the two bright planets and Moon
awed skygazers
around planet Earth, astronomer Mike Salway
reports taking special pains to record
this gorgeous view,
braving mosquitos and rain squalls along a soggy shore.
His southern hemisphere
perspective finds brilliant Venus at the highest point
in the celestial grouping.
For now, a bright pairing of Venus and Jupiter continues
to dominate the western horizon after sunset but the Moon has
moved on and tonight is near its
first quarter phase.
APOD: 2008 December 4 - Venus in the Moon
Explanation:
On December 1, bright planets Venus and Jupiter gathered near the
young crescent Moon, an inspiring
celestial scene
in early evening skies
around
the world.
But from
some locations
the Moon actually passed in front of Venus,
interrupting the tight grouping with a lunar occultation.
Captured from Wildon, Austria,
this twilight view shows the
silvery evening star about five minutes before it
slipped behind
the dark lunar limb and vanished from sight for more than hour.
The image is a combination of long and short exposures showing
details of the lunar surface illuminated by both faint
earthshine
and bright sunlight.
In the inset, recorded later in darkened
skies over Breil-sur-Roya in
southeastern France, a dazzling Venus has reappeared below the
bright lunar crescent.
Of course, Jupiter, at the upper right about 2 degrees from
Venus and Moon, is
sporting moons of its own seen as
tiny pinpricks of light on either side of the bright planet.
APOD: 2008 December 3 - A Happy Sky Over Los Angeles
Explanation:
Sunday, the sky seemed to smile over much of planet Earth.
Visible the world over was an unusual superposition of our Moon and the planets Venus and Jupiter.
Pictures taken at the right time show a crescent Moon that appears to be a smile when paired with the
planetary conjunction of seemingly nearby Jupiter and Venus.
Pictured above is the scene as it appeared from
Mt. Wilson Observatory
overlooking
Los Angeles,
California,
USA
after sunset on 2008 November 30.
Highest in the sky and farthest in the distance is the planet
Jupiter.
Significantly closer and visible to Jupiter's lower left is
Venus,
appearing through Earth's atmospheric clouds as unusually blue.
On the far right, above the horizon, is our Moon, in a
waxing crescent phase.
Thin clouds illuminated by the Moon appear unusually orange.
Sprawling across the bottom of the image are the hills of Los Angeles, many covered by a thin haze, while
LA skyscrapers are visible on the far left.
The conjunction of
Venus and Jupiter will
continue to be
visible
toward the west after sunset during much of this month.
Hours after the taking of this image, however,
the Moon approached the distant duo, briefly
eclipsed Venus, and then moved on.
APOD: 2008 February 26 - Mysterious Acid Haze on Venus
Explanation:
Why did an acidic haze spread across Venus?
The unusual clouds were discovered last July by
ESA's robotic
Venus Express
spacecraft currently orbiting
Venus.
The bright and smooth
haze was found by Venus Express to be rich in
sulfuric acid, created when an unknown process lifted water vapor and
sulphur dioxide
from lower levels into
Venus' upper atmosphere.
There, sunlight broke these molecules apart and some of them recombined into the
volatile sulfuric acid.
Over the course of just a few days last July, the smooth acidic clouds spread from the
South Pole of Venus across half the planet.
The above false-color picture of Venus was taken last July 23rd in
ultraviolet light,
and shows the unusual haze as relatively smooth regions across the image bottom.
The cause of the dark streaks in the clouds is also not yet understood and is being researched.
APOD: 2008 February 2 - Venus and Jupiter in Morning Skies
Explanation:
These two celestial beacons shining brightly in the east before
sunrise are actually
children of the Sun,
the planets Venus and Jupiter.
The second and third brightest objects in
the sky at Night
after the Moon,
Venus and Jupiter
appeared separated by about 2 degrees
when this picture was taken on January 30th, but closed to within
nearly half a degree early yesterday morning.
In the serene foreground is the
shoreline along the
Miankaleh
Peninsula and Gorgan Bay, an important
bird and wildlife
refuge in the
southeastern Caspian Sea.
Over the next two days, early morning risers around the globe
will be able to enjoy a close pairing of Venus and Jupiter
with an old crescent Moon.
APOD: 2007 November 8 - VERITAS and Venus
Explanation:
Early morning risers and late to bed astronomers have recently
enjoyed
bright planets in predawn skies, with
brilliant Venus above the eastern horizon.
On November 5, Venus was joined by the waning crescent
Moon.
This self-portrait by astronomer Larry Ciupik captures the
lovely pairing of the two brightest celestial beacons on the scene,
though the Moon, right of Venus, is strongly over exposed.
Included at the far left in the 30 second exposure is the bright
streak of the International
Space Station still docked with shuttle orbiter
Discovery.
Together in Earth orbit, the
spacefaring combination was momentarily
the third brightest
sky
light in view.
In dim silhouette, a multi-mirrored unit of the
Very Energetic Radiation Imaging Telescope Array System
(VERITAS)
is also visible in the foreground.
VERITAS operates at the Whipple Observatory near Tucson, Arizona
to detect high-energy gamma-rays
from the cosmos.
APOD: 2007 July 18 - Planets over Pony Express Lake
Explanation:
Beautiful sunset
sky colors
are reflected in
Pony Express Lake in
this
twilight skyview from
northern Missouri, USA, planet Earth.
Recorded on Monday, a two day old crescent Moon and
brilliant planet Venus shine through thin clouds.
Joining the
conjunction on the right of the Moon's
sunlit crescent is fellow
wanderer Saturn, with Regulus, alpha star of the
constellation Leo, above and right of Venus.
Moonlight and
Venus
light streak the almost-calm lake waters.
APOD: 2007 July 4 - Red, White, and Blue Sky
Explanation:
Contrasting colors in this
beautiful sunset sky
were captured on June 30 from
Clear Creek Canyon Observatory in central Arizona, USA.
The twilight scene includes
brilliant Venus as the
evening
star, with a bright Saturn just above it,
shining through thin clouds.
The two wandering
planets were
a mere 1 degree apart or so,
about twice the width of the full Moon rising above the
eastern horizon on the other side of the sky.
In fact, such serene
skyviews were possible from
all over planet Earth as Venus and Saturn approached a
conjunction.
Regulus, alpha star of the
constellation
Leo, is above and to the left of the close planetary pairing.
At dusk, lights in tonight's sky will also feature
Venus and Saturn low in the west and separated by
about 2 degrees.
APOD: 2007 June 20 - A Daylight Eclipse of Venus
Explanation:
Something was about to happen.
Just two days ago, two of the three celestial objects easily visible during the day appeared to collide.
But actually,
Earth's Moon
passed well in front of the distant
planet Venus.
The occultation was caught from
Switzerland
in the hours before
sunset.
Moments after this image was taken, the Moon, visible as the crescent on the right of the
above image,
eclipsed Venus, appearing near
half phase on the lower left.
Clouds that once threatened to obscure the
whole event, were visible on the far left.
About
90 minutes later,
Venus re-appeared just to the right of the
bright crescent.
APOD: 2007 May 23 - Venus Near the Moon
Explanation:
The two brightest objects in the night sky appeared to go right past each other last week.
On the night of May 19,
Earth's Moon and the
planet Venus were visible in the same part of the sky,
and at closest approach were less than one degree apart.
The conjunction was captured in the above image taken from near
Quebec City,
Quebec,
Canada.
Venus appears on the lower left of the above photo.
The spires that appear to emanate from
Venus are
diffraction spikes caused by the camera itself.
The image is so clear that
craters on the Moon are resolved.
Of course, the real physical distance between the
two heavenly bodies was not unusually small -- the apparent
conjunction was really just an
illusion of
perspective.
Although Earth's Moon passes Venus once each month, such a
close passing visible in the
evening sky is more rare.
APOD: 2007 May 1 - Swirling Clouds Over the South Pole of Venus
Explanation:
What's happening over the South Pole of Venus?
To find out, scientists sent the
robot Venus Express spacecraft now orbiting
Venus
directly over the lower spin axis of Earth's overheated twin.
Venus Express
confirmed there a spectacular massive swirling storm system with
similarities to the
vortex recently imaged over Saturn's South Pole.
The above composite image in
infrared light features Venus' daytime side on the left,
shining primarily by reflected sunlight, and nighttime side on the right,
shining primarily by
thermal light.
A Venusian polar vortex is visible as
the small circular feature near the center of the thermal infrared image pictured on the right.
Close inspection of
other South Pole images unexpectedly showed a second vortex,
meaning that the unusual swirling clouds are like an
Earth-hurricane that has two eyes.
Why a double vortex has formed is now a topic of
research.
The above image was taken last year, and
more recent images from Venus Express
are being processed that have as much as 100 times more detail.
APOD: 2007 April 14 - Venus by the Lake
Explanation:
Finding Venus
in the night sky is not too hard these days.
Now appearing as the evening star, Venus rules as the brightest
celestial beacon in west just
after
sunset.
And if you can find Venus tonight, you can also easily
find the lovely Pleiades star cluster
(aka M45) close by.
In this serene skyview, recorded on Tuesday near
Bolu, Turkey, Venus and
the Pleiades are on the right, with
brilliant Venus reflected in the calm waters
of the small lake in the foreground.
Left of Venus, the bright star
Aldebaran anchors the V-shaped
Hyades star cluster.
Farther left are stars of the familiar constellation Orion with
Rigel, at the foot of Orion, also reflected in the lake.
Meanwhile, Sirius, in Canis Major,
is the brightest star on the
left side of the view.
But the bright terrestrial light below Sirius is not a reflection,
it's just a light near the lake shore.
APOD: 2006 October 30 - Crescent Venus and Moon
Explanation:
There's something behind these clouds.
Those faint graceful arcs, upon inspection, are actually far, far in the distance.
They are the
Earth's Moon and the
planet Venus.
Both the Moon and Venus
are bright enough to be seen during the day, and both are quite capable of showing a
crescent phase.
To see Venus, which appears quite small, in a
crescent phase requires
binoculars or a telescope.
In the
above dramatic daytime image taken from
Budapest,
Hungary, the
Moon and Venus shared a similar crescent
phase a few minutes before the
Moon eclipsed the larger but more distant world.
About an hour later, Venus reappeared.
APOD: 2006 July 23 - The Belt of Venus over the Valley of the Moon
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless twilight, just before
sunrise or after
sunset,
part of the atmosphere above the horizon appears
slightly off-color, slightly pink.
Called the Belt of Venus, this off-color band between the dark
eclipsed sky and the
blue sky can be seen in nearly every direction
including that opposite the Sun.
Straight above, blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the
atmosphere reflects light from the setting (or rising)
Sun which appears more red.
The Belt of Venus can be seen from any location with a
clear horizon.
Pictured above, the Belt of Venus was photographed above
morning fog in the
Valley of the Moon, a famous wine-producing region in northern
California,
USA.
The belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2006 July 17 - Venus Express Arrives at Venus
Explanation:
Humanity now has a spacecraft orbiting Venus.
The robotic
Venus Express spacecraft
launched by the
European Space Agency in 2005 November arrived at
Venus in 2006 April.
Venus Express is now orbiting Earth's sister planet and returning pictures.
Pictured above is a false-color, time-lapse movie in
ultraviolet light
captured by the Venus Express spacecraft as it flew over
Venus' northern hemisphere in late May.
Venus Express is scheduled to orbit
Venus for three years and collect data that might help in answering
questions that include why Venus continually generates
hurricane-force winds,
why Venus became
so hot in the past, and if there is any current volcanic activity on
Venus.
It is hoped that a better understanding of
Venus's hot and inhospitable climate will help humanity better understand
Earth's climate as well.
APOD: 2006 June 15 - Gordel van Venus
Explanation:
Scroll right and
enjoy this 180 degree panorama across the
South African Astronomical
Observatory's hilltop
Sutherland observing station.
Featured are
SAAO
telescope domes and buildings, along
with the dark, wedge-shaped shadow of planet Earth stretching into
the distance, bounded above by the delicately
colored antitwilight arch.
Visible along the antisunward horizon
at sunset,
(or sunrise)
the pinkish
antitwilight arch
is also known as the Belt of Venus.
In order, the significant structures from left to right house;
the giant SALT 11-meter instrument,
the internet telescope
MONET,
the 1.9 meter Radcliffe,
the 1.0 meter Elizabeth,
a 0.75 meter reflector,
a 0.5 meter reflector,
a garage,
YSTAR,
BiSON,
ACT,
IRSF (open),
and a storage building.
(Note to SAAO fans: in this east-facing view the planet-hunter
SuperWASP south
is hidden behind the IRSF.)
APOD: 2006 March 3 - Venus and Comet Pojmanski
Explanation:
Shining brightly in the east at dawn,
Venus
dominates the sky in this view over a suburban
landscape from Bursa, Turkey.
An otherwise familiar scene for astronomer Tunc Tezel, his
composite picture of the morning sky recorded on March 2nd
also includes a surprise visitor to the inner solar system,
Comet Pojmanski.
Cataloged as C/2006 A1, the comet was discovered
on January 2nd by Grzegorz Pojmanski of Warsaw University
Astronomical Observatory
in Poland.
At the time
very
faint and tracking through
southern skies, the comet
has now moved north and grown just bright enough to be a good target for
early-rising skygazers with binoculars.
Enhanced and framed in this picture, the comet's
tail has
also grown to a length of several degrees.
The comet will be at its closest approach to planet Earth, just
over 100 million kilometers away, on March 5.
For northern hemisphere observers in the next few days, the beginning
of morning twilight really will be the best time to
spot Comet Pojmanski.
APOD: 2006 February 1 - Venus Just After Sunset
Explanation:
Is that Venus or an airplane?
A common ponderable for
sky enthusiasts is deciding if that bright spot
near the horizon is the planet
Venus.
Usually, an airplane will show itself by moving significantly in a few moments.
Venus will set only slowly as the
Earth turns.
Still, the identification would be easier if Venus did not keep
shifting its position each night.
Pictured above,
Venus was captured 38 different nights during 2005 and 2006 over
Bursa,
Turkey, when
Earth's sister planet appeared exclusively in the evening sky.
The average spacing of the images was about five days, while the images
were always taken with the Sun about 7 degrees below the horizon.
Venus' orbit
around the Sun will now confine it to Earth's
morning sky until October 2006.
APOD: 2006 January 10 - The Phases of Venus
Explanation:
Venus goes through phases.
Just like our Moon,
Venus
can appear as full as a disk or as a
thin as a crescent.
Venus, frequently the brightest object in the post-sunset or pre-sunrise sky,
appears so small, however, that it usually requires
binoculars or a
small telescope to clearly see its current phase.
The above time-lapse sequence, however, was taken over the
course of many months and shows not only how Venus changes phase
but how it's apparent
angular size also changes.
In the middle negative image, Venus is in a new phase, the same phase that occurred during its
rare partial eclipse of the Sun in 2004.
APOD: 2005 December 9 - December Moon Meets Evening Star
Explanation:
If you've been outdoors near sunset, then you've probably
noticed Venus low in the west as the
brilliant evening star.
Sometimes mistaken for a tower light
near the horizon,
Venus is the third brightest celestial beacon, after
the Sun and Moon, in planet Earth's sky.
That distinction is particularly easy to appreciate in
this
peaceful scene featuring the crescent Moon, Venus, and
sunset colors captured on
December 4th near Albany, Missouri, USA.
As this season's evening star,
Venus
will be at its most brilliant
tonight, but as December progresses the bright
planet will begin to
fall out of the western sky.
By early next week, December's Moon will have moved on to meet
another bright planet overhead -- Mars.
APOD: 2005 September 9 - Moon River
Explanation:
Shortly
after
sunset on September 6th, sky gazers around the world
were treated to a lovely
crescent
Moon in western skies --
joined by
bright planets Venus and Jupiter.
In this colorful telephoto view from near Quebec City,
Canada the Moon is nestled just above the wide
St.
Lawrence River.
Lights on the horizon are along the river's southern shore.
Also known as the evening star,
Venus is at the upper left
and Jupiter at the upper right, while
another prominent
celestial
beacon, Spica, can be seen shining
through the twilight below Venus.
Spica, actually a very close pair of hot blue stars some 260 light-years
away, is the brightest star in the
constellation
Virgo.
APOD: 2005 September 3 - Venus Unveiled
Explanation:
The surface of Venus is perpetually
covered by a veil of thick clouds
and remains hidden from even the powerful
telescopic eyes of earth-bound astronomers.
But in the early 1990s, using imaging radar, the Venus orbiting
Magellan
spacecraft was able to lift the veil from the
face of Venus and
produced spectacular high resolution images
of the planet's surface.
Colors used in this
computer generated picture of
Magellan radar data are based on color images from the surface
of Venus transmitted by the
Soviet Venera
13 and 14 landers.
The bright area running roughly across the middle
represents the largest highland region
of Venus known as
Aphrodite Terra.
APOD: 2005 August 9 - The Belt of Venus over Elwood Beach
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless twilight, just before
sunrise or after
sunset,
part of the atmosphere above the horizon appears
slightly off-color, slightly pink.
Called the Belt of Venus, this off-color band between the dark
eclipsed sky and the
blue sky can be seen in nearly every direction
including that opposite the Sun.
Straight above, blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the
atmosphere reflects light from the setting (or rising)
Sun which appears more red.
The Belt of Venus can be seen from any location with a
clear horizon.
Pictured above, the Belt of Venus was photographed behind
Elwood
Beach in
Melbourne,
Australia.
The belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2005 July 2 - Three Planets by the Sea
Explanation:
On Tuesday, June 28th, the setting Sun flooded the horizon with
a beautiful warm light in
this view from
the beach beside the pier at Brighton in Adelaide,
South Australia.
The Sun also illuminated three planets gathered in the
western sky,
Mercury, Venus, and Saturn.
From this perspective
Mercury is at the
highest point in the celestial triangle, brilliant
Venus
is just below, and Saturn
stands farther to the left and below the
close pair.
Of course, the planets only appear close together on the sky
but are actually quite far apart in space.
The orbits
of Mercury and Venus are both interior to
Earth's orbit, while gas giant
Saturn lies in the outer
solar system, over nine
astronomical units
from the Sun.
Late next week,
Venus and Mercury will share western
skies with the young
crescent Moon.
APOD: 2005 June 30 - Three Planets from Mt Hamilton
Explanation:
Venus, Mercury, and Saturn
wandered close together
in western evening skies last week.
On Saturnday,
June 25, astronomer R. Jay GaBany recorded
this snapshot of their eye-catching planetary conjunction,
from historic Lick Observatory
on Mt. Hamilton,
California, USA.
The view looks toward the Pacific shortly after sunset
with the lights of San Jose and the southern San Francisco
Bay area in the foreground.
Of course, Venus is
the brightest of the trio.
Mercury is nearby on the right
and Saturn is below and left,
closest to the horizon.
Farther to the right of the planetary triangle are
Pollux and Castor,
twin
stars of Gemini, with
Regulus,
bright star
of the constellation Leo, at the very upper left corner of the
picture.
In the
coming days, Venus and Mercury remain close,
while Saturn continues to drop below them, toward the horizon.
APOD: 2005 June 25 - Venus: Just Passing By
Explanation:
Venus, the second closest planet to the Sun,
is by far the brightest of the
three planets gathered in this weekend's
western sky at sunset.
It has also proven to be a popular
way-point for spacecraft headed for the
gas giant planets
in the outer reaches of the solar system.
Why visit Venus first?
Using a gravity assist maneuver,
spacecraft can swing by planets and gain energy during their brief
encounter, saving fuel for use at the end of
their long interplanetary voyage.
This
colorized image of Venus was recorded by the Jupiter-bound
Galileo spacecraft shortly after its gravity assist flyby of Venus
in February of 1990.
Galileo's glimpse of
the veiled planet shows structure in
swirling sulfuric acid clouds.
The bright area is
sunlight glinting off the upper cloud deck.
APOD: 2005 June 24 - Planets in the West
Explanation:
This weekend
three planets will grace
the western sky,
forming a lovely trio easily visible shortly after sunset.
Saturday evening in particular will find
Saturn,
Venus, and
Mercury all within a 2 degree circle
(about the size of your thumb held at arm's length)
above the western horizon.
Recorded last Sunday, June 19, this image shows the same
three planets arrayed along the
ecliptic plane above a Colorado
Rocky Mountain skyline.
Venus is easiest to pick out of the twilight, the brightest
celestial beacon below picture center, with Saturn
above and to the left of Venus, and Mercury closest to the
horizon, right of prominent Pinnacle Peak.
By Saturday, the
wandering planets
will draw even closer together.
For help spotting the planets here, put your cursor over the
picture.
APOD: 2005 June 9 - Venus Returns to the Evening Sky
Explanation:
This serene image
of boats moored in the harbor of
l'Île-Tudy, Bretagne, France was taken on June 1st,
about an hour after sunset.
It also features Venus,
third brightest celestial object
after the Sun and Moon.
For casual skygazers, this month marks
Venus' return
to the evening sky as the
brilliant 'star',
shining low in the west-northwest shortly after sunset.
In the picture,
astrophotographer
and APOD translator
Laurent Laveder notes that Venus is easily mistaken for
a light atop a sailboat's tall mast, giving
the otherwise stunning celestial beacon an unremarkable
appearance.
Of course, a year ago Venus' appearance was quite remarkable.
On June 8, 2004,
Venus crossed the Sun's disk,
the first transit of Venus since 1882.
Late this week
Venus shares the evening sky with the young
crescent Moon, and will next transit the Sun on June 6,
2012.
APOD: 2005 April 10 - Venus' Once Molten Surface
Explanation:
If you could look at Venus with
radar eyes - this is what you might see.
This computer reconstruction of the surface of
Venus was created from data from the
Magellan spacecraft.
Magellan orbited Venus and used
radar to map our
neighboring planet's surface between 1990 and 1994.
Magellan found many interesting surface features,
including the large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism
is thought to have created the
domes, although the precise mechanism remains unknown.
Venus' surface is so hot and
hostile that no surface probe
has lasted more than a few minutes.
APOD: 2005 January 7 - S is for Venus
Explanation:
Planet Venus
traced out this
S
shape in Earth's sky during 2004.
Following the second planet from the Sun in a series
of 29 images recorded from April 3rd
through August 7th
(top right to bottom left) of that year, astronomer Tunc Tezel
constructed this composite illustrating the
wandering planet's
path against the background stars.
The series reveals Venus' apparent
retrograde motion
transporting it from a brilliant evening star to
morning's celestial beacon.
Of course, in 2004, after sinking into the
evening twilight
but before rising above the predawn
horizon, Venus
was seen in silhouette against
the Sun (near center) - the first
transit of Venus since 1882.
The next time Venus will wander across the
solar disk is in 2012.
APOD: 2004 November 13 - Moon Over Shiraz
Explanation:
Early morning risers
around the world have enjoyed the
sight of bright planets
in this week's predawn skies -
further enhanced by the celestial spectacle of the waning
crescent Moon.
From some locations the Moon was seen to pass in front
of
Jupiter or Venus, a lunar occultation.
Recorded near sunrise on November 10th from
Shiraz, Iran, this
eastern horizon view finds Jupiter (top) and a brilliant Venus
in line with
the Moon, a lovely conjunction of the three brightest
objects in the night sky.
Although the Moon has
now
fallen out of the early morning
scene,
Venus and Jupiter (along with a much fainter Mars) still precede
the rising Sun above the eastern horizon.
APOD: 2004 November 8 - Jupiter and Venus at Sunrise
Explanation:
What are those bright objects in the
morning sky?
Early morning dog walkers, among many others across our world's Northern Hemisphere,
have likely noticed tremendously bright
Venus hanging in the
eastern sky just before sunrise.
Looking a bit like an approaching airplane,
Venus holds its place in the sky and never seems to land.
Last week, impressive but less bright
Jupiter appeared within a degree of the
Venusian orb, creating a
dazzling sky that you might appreciate a bit more than your dog.
This night sky early show will
change slightly over the next week, with the
planets moving past each other,
Mars moving into the picture, guest stars like
Spica appearing to shift in the background, and even a crescent Moon stopping in for a cameo.
Pictured above last week, Jupiter and Venus were photographed rising before the Sun over the city of Bursa,
Turkey.
APOD: 2004 July 20 - Space Station, Venus, Sun
Explanation:
On June 8,
Venus was not the only celestial object to pass in front of the Sun.
A few well-situated photographers caught the
International Space Station
also crossing the Sun simultaneously.
Pictured above is a unique time-lapse image of the unprecedented double transit, a rare event that was visible for less than a
second from a narrow band on
Earth.
The above image is a combination of
12 frames taken 0.033 seconds apart and each
themselves lasting only 1/10,000 th of a second.
The image was taken from the small village of
Stupava in
Slovakia.
The next time Venus will
appear to
cross the Sun from
Earth will be in 2012.
APOD: 2004 July 17 - Transit of Venus Stereogram
Explanation:
Venus glides in front of an
enormous solar disk in these two frames from the
TRACE satellite imaging
of the inner planet's 2004 transit.
Arranged in a "right/left" stereogram, the
frames are intended
to be viewed at a comfortable distance from the
screen with your eyes gently crossed, allowing the images
to merge and produce a pleasing stereo effect.
Shown during the ingress (beginning) phase of the transit,
the silhouetted portion of the planet appears to
float dramatically
in front of the Sun's granulated surface.
Of course, the dense
Cytherian
(Venusian) atmosphere also scatters
and refracts the intense sunlight.
The effect is visible across the portion of the planet
still beyond
the Sun's edge and
viewed against
the blackness of space.
APOD: 2004 July 3 - Cassini to Venus
Explanation:
Saturn
Orbiter Cassini with
Titan
Probe Huygens attached
rocketed into early morning
skies on October 15, 1997.
The mighty Titan 4B Centaur rocket
is
seen here across the water, arcing away
from Launch Complex 40 at
Cape Canaveral Air Station.
Cassini, a sophisticated
robot
spacecraft was actually headed toward
inner planet Venus,
the first way point in its 7 year, 2.2 billion mile
interplanetary journey to Saturn.
In fact, Cassini swung by Venus during
April 1998 and June 1999, Earth
in August 1999, and Jupiter
in December 2000.
During each of these
"gravity assist" encounters the six ton
spacecraft picked up speed,
reaching Saturn only three days ago.
Cassini is now orbiting the ringed gas giant, with
the Huygens Probe scheduled to separate from the spacecraft
in December.
The probe's descent to the surface of
Saturn's large moon
Titan
will be the most distant
landing ever attempted.
APOD: 2004 June 23 - A Picturesque Venus Transit
Explanation:
The rare
transit of Venus across the face of the Sun earlier this month was one of the better-photographed events in sky history.
Both scientific and artistic images have been flooding in from the areas that could see the transit: Europe and much of Asia, Africa, and North America.
Scientifically, solar photographers confirmed that the
black drop effect
is really better related to the viewing clarity of the camera or telescope than the atmosphere of Venus.
Artistically, images might be divided into several categories.
One type captures the
transit in front of a highly detailed Sun.
Another category captures a double coincidence such as both Venus and an airplane simultaneously silhouetted, or Venus and the International Space Station in low Earth orbit.
A third image type involves a fortuitous arrangement of interesting looking clouds, as shown by example in the
above image
taken from
North Carolina,
USA.
There the distant orb of giant
Venus might have been mistaken, at first glance, for a small but unusually circular cloud.
APOD: 2004 June 15 - A Rare Annular Venusian Solar Eclipse
Explanation:
An unusual type of solar eclipse occurred last week.
Usually it is the
Earth's Moon that
eclipses
the Sun.
Last week, for the first time in over 100 years, the planet
Venus took a turn.
Like a solar eclipse by the Moon, the phase of Venus became a continually thinner
crescent as Venus became increasingly
better aligned with the Sun.
Eventually the alignment became perfect and the
phase of Venus dropped to zero.
The dark spot of Venus crossed our parent star.
The situation could technically be labeled a Venusian
annular eclipse with an extraordinarily large
ring of fire.
From above the
thick cloud tops of Venus,
the Earth appeared in its fullest phase, brighter in the
Venusian sky than even
Mars appeared from Earth last August.
Hours later, as Venus continued in its orbit,
a slight crescent phase appeared again.
The next Venusian solar eclipse will occur in 2012.
APOD: 2004 June 11 - Venus and the Chromosphere
Explanation:
Enjoying the 2004
Transit of Venus from Stuttgart, Germany,
astronomer Stefan Seip recorded
this fascinating, detailed image of the Sun.
Revealing a network of cells and dark
filaments against
a bright solar disk with spicules and
prominences along
the Sun's limb, his telescopic picture
was taken through an H-alpha filter.
The filter
narrowly transmits only the red light from
hydrogen atoms and emphasizes the
solar chromosphere --
the region of the Sun's atmosphere immediately above
its photosphere or normally visible surface.
Here, the dark disk of Venus seems to be imitating a giant
sunspot that looks perhaps a little too round.
But in H-alpha pictures
like this one, sunspot regions
are usually dominated by bright splotches (called
plages) on the
solar chromosphere.
APOD: 2004 June 10 - Venus at the Edge
Explanation:
With Venus in transit at the Sun's edge on June 8th, astronomers
captured this tantalizing
close-up view
of the bright solar surface
and partially silhouetted disk.
Enhanced in the sharp picture, a delicate arc of sunlight
refracted through the Venusian atmosphere is
also visible
outlining the planet's edge against the blackness of space.
The arc is part of a luminous ring or atmospheric
aureole, first noted and offered as evidence that Venus
did posses an atmosphere following observations of
the planet's 1761 transit.
The image was recorded using the 1-meter
Swedish Solar Telescope
located on La Palma in the Canary Islands.
For the Institute for Solar Physics,
Dan Kiselman, Goran Scharmer, Kai Langhans, and Peter Dettori were
at the telescope, while Mats Lofdahl produced the final image.
Excellent movies of
the
transit - including one of the emergence of
Venus' atmospheric aureole - are
available from the
Dutch Open Telescope, also observing
from La Palma.
APOD: 2004 June 9 - Venus Transit at Sunrise
Explanation:
Did you see the transit?
While some watched by webcast, sky gazers in Europe, the Middle
East, Africa, and Asia were
able
to witness the complete
6 hour journey of Venus' silhouetted disk across the face
of the Sun.
As seen
from North America, the much heralded
Venus Transit of 2004 was
nearing its final stages at sunrise yesterday in this
telescopic image.
The view looks across the Atlantic from Tybee Island near
Savannah, Georgia, USA.
In fact, many in eastern North America
experienced
a dramatic view of a perfect, dark, round Venus against a
reddened Sun filtered by banks of low clouds.
Ironically, the Sun takes on the appearance of
a cloud covered planet itself as
Venus marches
toward the right through this dreamlike scene.
APOD: 2004 June 8 - A Planet Transits the Sun
Explanation:
Today an astronomical event will occur that no living person has ever seen:
Venus will cross directly in front of the Sun.
A Venus crossing, called a transit, last occurred in 1882 and was
front-page
news
around the world.
Today's transit will be visible in its entirety throughout
Europe and most of Asia and Africa.
The northeastern half of
North America will see the Sun rise with the
dark dot of Venus already superposed.
Never look directly at the Sun, even when
Venus is in front.
Mercury's closer proximity to the Sun cause it to transit every few years.
In fact, the above image mosaic of Mercury
crossing the Sun is from
two
transits
ago, in November 1999.
Will anyone living see the next Venus transit? Surely yes since it occurs in 2012.
APOD: 2004 May 21 - Phases of Venus
Explanation:
Venus is currently
falling out of the
western evening sky.
Second planet from the Sun and
third brightest celestial object after the Sun and Moon,
Venus has been appreciated by casual sky gazers as a brilliant beacon
above the horizon after sunset.
But telescopic
images have also revealed its dramatic phases.
In fact, this thoughtful composite of
telescopic views nicely illustrates the
progression of phases
and increase in apparent size undergone by Venus over
the past few weeks.
Gliding along its interior orbit, Venus has been
catching up with planet Earth, growing larger as it draws
near.
At the same time, just as the Moon goes
through phases,
Venus' visible sunlit hemisphere has presented an
increasingly slender, crescent shape.
Now sharing the sky with a crescent Moon, on
June 8th Venus
will actually cross the face of the Sun, the first such
transit since 1882.
APOD: 2004 May 16 - Venus: Earth's Cloudy Twin
Explanation:
This picture by the
Galileo spacecraft shows just how cloudy
Venus is.
Venus is very similar to Earth in size
and mass - and so is sometimes referred to as Earth's sister planet - but
Venus
has a quite different climate.
Venus' thick clouds and closeness to the
Sun
(only Mercury is closer) make it
the hottest planet - much hotter than the
Earth.
Humans could not survive there, and no life of any sort has ever been found.
When Venus is visible it is usually the brightest object in the sky
after the Sun and the Moon.
More than 20 spacecraft have visited
Venus
including Venera 9, which landed on the surface, and
Magellan,
which used radar to peer through the clouds and make a map of the
surface.
This visible light picture of Venus
was taken by the Galileo spacecraft
that orbited Jupiter from 1995 to 2003.
Many things about Venus remain unknown, including the cause of
mysterious bursts of radio waves.
APOD: 2004 April 15 - Venus and the Pleiades
Explanation:
Venus still rules
the western skies after sunset as the
brilliant evening star.
While wandering the ecliptic
with its fellow naked-eye planets
earlier this month, it passed
near
the Pleiades star cluster,
providing a striking photo opportunity for earthbound skygazers.
Cataloged as M45, the
Pleiades stars make for
a lovely sight on their own,
often shown in long exposure images immersed in hazy
blue reflection nebulae.
In
this picture though, recorded on the evening of
April 3rd, brilliant Venus closes with the
Seven Sisters
and overwhelms the light from the delicate cosmic clouds.
The view offers a study in contrasts as Venus
appears about 700
times brighter than Alcyone, the
Pleiades
brightest star.
With Venus just over 5 light-minutes from Earth, Alcyone and the
other Pleiades cluster stars are about 400 light-years distant.
Formed out of the contracting nebula which gave birth to
the Sun, Venus is also roughly 4.5 billion years old.
The stars of the Pleiades are likely aged a mere hundred
million years.
APOD: 2004 April 2 - Mercury and Venus in the West
Explanation:
Doing their part in the
ongoing dance of the planets,
Mercury and Venus both reached their greatest
elongation or maximum apparent distance from the Sun
only a few days ago, on March 29th.
Eager to record their celestial accomplishment, astronomer
Jimmy Westlake snapped this view of the two
inner most planets
shining in western twilight skies above Yampa,
Colorado, USA.
The picture was taken using a digital camera mounted on a tripod.
Mercury is easily the brightest
celestial object near the horizon, appearing to the right of the
foreground structure and
just above a thin cloud silhouetted by fading sunlight.
Still, near the top of the picture
brilliant Venus dominates the scene as the
magnificent evening star.
After climbing in western skies throughout the month of March,
Venus lies just
below the Pleiades star cluster.
Tonight and tomorrow night,
skygazers can spot Venus
at the southern edge of the Pleiades.
APOD: 2004 March 23 - Lava Flows on Venus
Explanation:
The hot surface of
Venus shows clear signs of ancient
lava flows.
Evidence of this was bolstered by the
robot spacecraft Magellan, which orbited
Venus in the early 1990s.
Using imaging radar,
Magellan
was able to peer beneath the thick perpetual
clouds
that cover Earth's closest planetary neighbor.
Picture above, lava apparently flowed down from
the top of the image and pooled in the light colored
areas visible across the image middle and bottom.
The lava cut a channel across the darker ridge that
runs horizontally across the image center.
The picture covers about 500 kilometers across.
The lava originates from a caldera named Ammavaru that lies about 300 kilometers off the
image top.
The hot dense climate makes Venus a more difficult planet on which to
land spacecraft and
rovers.
Venus currently
sparkles as the brightest object in the western sky after sunset.
APOD: 2004 March 8 - Moon and Venus over Corona Del Mar Beach
Explanation:
The crescent Moon passed nearly in front of Venus two weeks ago.
The close conjunction of the
night sky's
two brightest objects created a striking pose for many
viewing the evening sky just after sunset.
Such a pose, shown above, was captured between clouds over
Corona Del Mar Beach in
California,
USA.
To be precise, the Moon
appeared to pass only about three degrees from
Venus
on February 23.
A similar conjunction will occur later this month,
on March 24, when
Venus appears near its furthest from the
Sun while the
Moon passes only about 2 degrees away.
APOD: 2003 December 25 - Venus and the 37 Hour Moon
Explanation:
At Table
Mountain Observatory, near Wrightwood California, USA
on October 26, wild fires were approaching
from the east.
But looking toward the west just
after sunset,
astronomer James Young could still enjoy this comforting
view of a
young
crescent Moon and brilliant
Venus through the the fading twilight.
Setting over the horizon of Mt. Baden-Powell, the thin crescent
was only about 37 hours "old", or 37 hours after its exact New
Moon phase.
After disappearing from morning
twilight in August,
Venus was
becoming prominent in its role
in western skies as the
evening star.
A similar lovely pairing of thin crescent Moon and stunning
evening star can be seen toward the west in
today's evening twilight.
Happy Holidays and Best Wishes from
APOD!
APOD: 2003 November 30 - A Venus Landing
Explanation:
This image is part of the first color panoramic view from
Venus.
A TV camera on the
Soviet Venera 13 lander that parachuted to the surface on 1982 March 1 transmitted it.
Venus' clouds are composed of
sulfuric acid droplets while its surface temperature
is about 482 degrees
Celsius at an atmospheric pressure of 92 times that of
sea-level on Earth.
Despite these harsh conditions, the
Venera 13 lander survived long enough to
send back a series of images and perform an analysis of the
Venusian soil.
Part of the lander itself is visible in the
lower right portion of the image.
An earlier Soviet Venus lander,
Venera 7 (1970), was the first spacecraft
to return data from the surface of another planet.
APOD: 2003 October 21 - The Belt of Venus over the Valley of the Moon
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless twilight, just before
sunrise or after
sunset,
part of the atmosphere above the horizon appears
slightly off-color, slightly pink.
Called the Belt of Venus, this off-color band between the dark
eclipsed sky and the
blue sky can be seen in nearly every direction
including that opposite the Sun.
Straight above, blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the
atmosphere reflects light from the setting (or rising)
Sun which appears more red.
The Belt of Venus can be seen from any location with a
clear horizon.
Pictured above, the Belt of Venus was photographed above
morning fog in the
Valley of the Moon, a famous wine-producing region in northern
California,
USA.
The belt is
frequently
caught
by
accident
in
other
photographs.
APOD: 2003 May 14 - The North Pole of Venus
Explanation:
If you could look down on the
North Pole of Venus what would you see?
The Magellan probe that orbited
Venus from 1990 to 1994 was able to peer through the
thick Venusian clouds
and build up the
above image by emitting and re-detecting cloud-penetrating
radar.
Visible as the bright patch below central North is Venus'
highest mountain
Maxwell Montes.
Other notable features include numerous mountains,
coronas,
impact craters, tessera, ridges, and lava flows.
Although the size and mass of
Venus are similar to the Earth, its thick carbon-dioxide atmosphere has
trapped heat so efficiently that surface temperature usually exceeds 700 kelvins, hot enough to melt
lead.
APOD: 2003 April 27 - Venus' Once Molten Surface
Explanation:
If you could look at Venus with
radar eyes - this is what you might see.
This computer reconstruction of the surface of
Venus was created from data from the
Magellan spacecraft.
Magellan orbited
Venus and used
radar to map our
neighboring planet's
surface between 1990 and 1994.
Magellan found many interesting surface features,
including the
large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism
is thought to have created the
domes, although the
precise mechanism remains unknown.
Venus'
surface is so hot and hostile that no
surface probe
has lasted more than a few minutes.
APOD: 2002 December 4 - Moon, Mars, Venus, and Spica
Explanation:
Gliding toward today's total eclipse
of the Sun,
the crescent Moon has been rising early, just before dawn.
And as a prelude to its close solar alignment,
the Moon also completed a lovely celestial triangle, closing
with bright planets
Mars and Venus
on the morning of December 1.
While the total solar eclipse
can only
be seen
from a
narrow corridor, skygazers around the globe could
appreciate this
lunar-planetary conjunction.
This view is from near Nashville Tennessee, USA, and finds
brilliant Venus at the lowest corner of the triangle with a much fainter
Mars immediately to the right of the Moon.
The Moon's sunlit crescent is overexposed, but details of the lunar night side
are revealed by earthshine.
Above and to the right of the trio is
Spica, brightest star in
the constellation Virgo.
APOD: 2002 September 29 - Venus: Just Passing By
Explanation:
Venus,
the second closest planet to the Sun, is a popular
way-point for spacecraft headed for the
gas giant planets
in the outer reaches of the solar system.
Why visit Venus first?
Using a "gravity assist " maneuver,
spacecraft can swing by planets and gain energy during their brief
encounter saving fuel for use at the end of
their long interplanetary voyage.
This colorized image of Venus was recorded by the Jupiter-bound
Galileo spacecraft shortly after its gravity assist flyby of Venus in
February of 1990.
Galileo's glimpse of
the veiled planet shows structure in
swirling sulfuric acid clouds.
The bright area is sunlight
glinting off the upper cloud deck.
A recent intriguing but controversial
hypothesis holds that living
microbes might exist in the
upper clouds of
Venus.
APOD: 2002 September 10 - Venus Beyond the Storm
Explanation:
A thunderstorm, lightning, a bright star and
a bright planet all graced an evening sky for a short while near
Bismarck,
North Dakota,
USA two weeks ago.
Thick thunderclouds from a passing storm are the
origin of a strong cloud to ground
lightning strike.
Small areas of rain darken portions of the orange
sunset,
visible at the horizon above the vast prairie.
The planet Venus peeks below the clouds
on the lower left of the image.
Blue sky shines high above the distant storm,
streaked with high white cirrus clouds.
The bright star
Arcturus glitters near the image top, just left of center.
Just a few minutes later, only a memory and this picture remained.
APOD: 2002 June 25 - Venus and Jupiter Over Belfast
Explanation:
Venus and Jupiter appeared to glide right
past each other earlier this month.
In a slow day-by-day march,
Jupiter sank into the sunset horizon
while Venus remained high and bright.
The conjunction ended the
five-planet party
visible over the last two months.
Jupiter, of course,
is much further away from the
Earth and
Sun than
Venus, so the passing was really just an
angular illusion.
Pictured above on June 3, a fading sunset finds
Venus shining over Jupiter above clouds, mountains, and the city lights of
Belfast,
Northern Ireland.
APOD: 2002 June 19 - The Moon and Venus Over Geneva
Explanation:
The Moon, fresh from a
biting encounter with the
Sun last week,
appeared next to threaten Venus.
The waxing Moon appeared to glide right past, however, just a
few degrees away.
Venus, of course,
is much further away from the
Earth than the Moon,
so the passing was really just an
angular illusion.
Pictured above on June 13, a fading sunset finds the
crescent Moon and
Venus between clouds and above
the city lights of
Geneva,
Switzerland.
APOD: 2002 May 24 - Love and War by Moonlight
Explanation:
Venus,
named for the Roman goddess of love, and
Mars,
the war god's namesake, approach each other by
moonlight
in this lovely sky view
recorded on May 14th from Dunkirk, Maryland, USA.
The four second time exposure made in twilight with a digital camera
also records
earthshine
illuminating the otherwise dark surface
of the young crescent Moon.
Venus shines as the third brightest object in Earth's sky,
after the Sun and the Moon itself, and has been appearing
as the brilliant
evening star in the
pantheon of planets
arrayed in the west during April and May.
Here, Venus' light is so intense that it produces a noticeable spike
in the sensitive camera's image.
Much fainter Mars is lower in the picture, caught between tree
limbs swaying in a gentle evening breeze.
By early June, Mars will be harder to
spot as it wanders toward the horizon, but Venus and
father
Jupiter will draw closer together,
presenting a spectacular pair of bright
planets in the west.
APOD: 2002 March 30 - Venus Unveiled
Explanation:
The surface of Venus is perpetually
covered by a veil of thick clouds
and remains hidden from even the powerful
telescopic eyes of earth-bound astronomers.
But in the early 1990s, using imaging radar, the Venus orbiting
Magellan
spacecraft was able to lift the veil from the
face of Venus and
produced spectacular high resolution images
of the planet's surface.
Colors used in this
computer generated picture of
Magellan radar data are based on color images from the surface
of Venus transmitted by the
Soviet Venera 13 and 14 landers.
The bright area running roughly across the middle
represents the largest highland region
of Venus known as
Aphrodite Terra.
APOD: 2002 March 12 - Atete Corona on Venus
Explanation:
What could cause a huge cylindrical mountain
to rise from the surface of
Venus?
Such features that occur on
Venus are known as
coronas.
Pictured above in the foreground is 500-kilometer wide
Atete Corona found in a region of Venus known as the Galindo.
The image was created by combining multiple
radar maps of the region to form a
computer-generated three-dimensional perspective.
The series of dark rectangles that crosses the image from
top to bottom were created by the imaging procedure and are not real.
The origin of massive
coronas remains a mystery although
speculation holds they result from some form of
volcanism.
Studying Venusian coronas help scientists better understand the
inner structure of both Venus and
Earth.
APOD: 2001 December 11 - Venusian Half Shell
Explanation:
Venus,
second planet from the Sun, appears above imaged for
the first time ever in x-rays (left) by the
orbiting Chandra Observatory.
Chandra's smoothed, false-color, x-ray
view is compared to
an optical image (right) from a small earthbound telescope.
Both show Venus illuminated by the Sun from the right, with
only half the sunward hemisphere visible, but at least one
striking difference is apparent.
While the optical image in
reflected sunlight is filled and
bright at the center, Venus in x-rays is bright around the edge.
Venus' x-rays are produced
by
fluorescence rather than reflection.
About 120 kilometers or so above the surface,
incoming solar x-rays
excite atoms in the Venusian atmosphere
to unstable energy levels.
As the atoms
rapidly decay back to their stable ground states they emit
a "fluorescence" x-ray, creating a glowing x-ray
half-shell above the sunlit hemisphere.
More x-ray emitting
material can be seen looking at the edge
of the shell, so the edge appears brighter in the x-ray image.
APOD: 2001 December 9 - The Belt of Venus
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless
twilight, just before sunrise or after sunset, part of the atmosphere above the
horizon appears slightly off-color, slightly pink.
Visible in the
above photograph, this off-color band between the
dark eclipsed sky and the
blue sky can best be seen in the direction opposite the Sun
and is called the Belt of
Venus.
Straight above,
blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the atmosphere reflects light
from the
setting (or rising) Sun which
appears more red.
The Belt of Venus can be seen from any location
with a clear horizon.
It is frequently
caught
by
accident
in
other
photographs.
APOD: 2001 September 16 - Venus Once Molten Surface
Explanation:
If you could look at Venus with radar eyes -
this is what you might see.
This computer reconstruction of the surface of
Venus was created from data from the
Magellan spacecraft.
Magellan orbited
Venus
and used radar to map our
neighboring planet's
surface between 1990 and 1994.
Magellan found many interesting surface features,
including the
large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism
is thought to have created the
domes, although the
precise mechanism remains unknown.
Venus'
surface is so hot and hostile that no
surface probe
has lasted more than a few minutes.
APOD: 2001 June 1 - Venus' Evening Loop
Explanation:
From September 2000 through March 2001, astronomer Tunc Tezel
patiently photographed the planet Venus on 25 different dates
as it wandered through the evening twilight.
The pictures were taken from the same spot on the campus of
the Middle East Technical University near Ankara, Turkey, and
timed so that for each photo
the
Sun was 7 degrees below the horizon.
Carefully registering and combining the pictures, he produced
this composite image -- a stunning demonstration of
Venus' grand looping
sky motion
during its recent stint as planet Earth's
evening star.
As indicated, the first picture, taken September 28, 2000,
finds Venus close to the western
horizon and drifting south (left)
with the passing days.
By December however, Venus
was climbing well above the horizon after sunset and
in January 2001 it reached its maximum apparent distance
(elongation) from the Sun.
March found Venus falling from
the evening sky while
moving rapidly north, finally appearing (far right) as
a faint dot against the sunset glow on March 24.
This month, Venus rises before dawn as the brilliant
morning star.
APOD: 2001 May 15 - A Radar Image of Venus
Explanation:
The largest radio telescopes in the world are working
together to create a new map of the surface of Venus.
The surface of
Venus
is unusually hidden by a thick atmosphere of mostly
carbon dioxide gas.
These
thick clouds are transparent,
however, to radar signals sent and received from Earth.
The two
radio telescopes generating the
most powerful radar ever are the
Arecibo Telescope in
Puerto Rico and the new
Robert C. Byrd Green Bank Telescope in
West Virginia.
The new survey will resolve details as fine a one-kilometer across,
and will be inspected for changes since the
last major radar map was made by NASA's
Magellan spacecraft that orbited
Venus from 1990 to 1994.
Pictured above is part of a preliminary image showing
details as small as five-kilometers across.
APOD: 2001 May 7 - One Hundred Kilometer Terrain on Venus
Explanation:
Even the hot and cracked surface of
Venus has rolling hills.
Although never actually photographed from up-close,
images of the
Venusian surface like that shown above have been
constructed in recent years by digitally merging distant photographs from
height-sensitive radar.
Isolated
above is a 100-kilometer wide swath
inside a volcanic region
known as Yavine Corona.
Visible in
the frame are
numerous fractures
in the surface.
Data is missing from the dark lane on the upper right.
The surface of Venus is so hot and oppressive that
robot spacecraft
landed there
have lasted for only a few hours.
APOD: 2001 March 8 - Bright Venus
Explanation:
Have you seen a bright evening star
in the western sky lately?
That's no star, that's planet Venus the second "rock"
from the Sun.
Blazing at -4.6
magnitude, Venus, after the Sun and Moon,
is the third brightest celestial body in
planet Earth's sky.
Venus is closer to the Sun than Earth and
as Venus orbits
the Sun it is seen to go through
phases similar to the Moon.
But unlike the Moon, as
Venus waxes and wanes
its distance from Earth and hence its apparent size changes drastically.
This causes
Venus to look brighter
as it looms large in its
crescent phases than when it is smaller and nearly full.
Taken on January 28th, this dramatic picture finds a crescent
Venus near its brightest to the right of a crescent Moon.
The brilliant rivals seem poised above a satellite dish of the
Scripps Satellite Oceanography Facility.
Closer to the horizon,
just below and to the right of the satellite dish,
Mercury pierces the twilight glow.
APOD: 2000 July 28 - Moon And Venus Share The Sky
Explanation:
July is drawing to a close and in the past few days,
some early morning risers could have
looked east and seen a crescent Moon
sharing the pre-dawn skies with planets Jupiter and Saturn.
Planet Mercury will also pass
about 2 degrees from
the thin waning crescent
Moon
just before sunrise near the eastern horizon
on Saturday, July 29.
And finally, on the evening of July 31st, Venus will take its turn
near the crescent Moon.
But this time it will be a day-old crescent Moon near the western horizon,
shortly after sunset.
In
fact, on July 31 (August 1 Universal Time)
the Moon will occult
(pass in front of) Venus for
northwestern observers in North America.
This telescopic picture taken on 31 December 1997, shows a lovely young
crescent Moon and brilliant crescent
Venus in the early evening sky near
Bursa,
Turkey.
And what about the Sun? On Sunday, July 30, a
partial eclipse of the Sun will be visible from
some locations in North America.
APOD: 2000 April 6 - Venus, Moon, and Neighbors
Explanation:
Rising before the Sun on February 2nd,
astrophotographer Joe Orman
anticipated this apparition of the bright
morning star
Venus near a lovely crescent Moon above a neighbor's house
in suburban Phoenix, Arizona, USA.
Fortunately, the alignment of bright planets and the Moon is
one of the most inspiring sights in the
night sky and one
that is often easy to enjoy and share without any special equipment.
Take tonight, for example.
Those blessed with clear skies can simply step
outside near sunset
and view a young crescent Moon very near three bright planets
in the west
Jupiter,
Mars, and
Saturn.
Jupiter will be the unmistakable brightest star near the Moon
with a reddish Mars just to Jupiter's north and pale yellow
Saturn directly above.
Of course, these
sky
shows create an
evocative picture but the
planets and Moon just appear to be near each other --
they are actually only approximately lined up and
lie in widely separated orbits.
Unfortunately, next month's highly publicized
alignment of planets on May 5th will be lost from
view in the Sun's glare but such
planetary
alignments occur repeatedly and
pose no danger to planet Earth.
APOD: 2000 March 26 - Venus Once Molten Surface
Explanation:
If you could look at Venus with radar eyes -
this is what you might see.
This computer reconstruction of the surface of
Venus was created from data from the
Magellan spacecraft.
Magellan orbited
Venus
and used radar to map our
neighboring planet's
surface between 1990 and 1994.
Magellan found many interesting surface features,
including the
large circular domes,
typically 25-kilometers across, that are depicted above.
Volcanism is thought to have created the domes, although the
precise mechanism remains unknown.
Venus'
surface is so hot and hostile that no
surface probe
has lasted more than a few minutes.
APOD: November 28, 1999 - Beneath Venus Clouds
Explanation:
If the thick clouds covering Venus were removed,
how would the surface appear?
Using an imaging radar technique, the Magellan spacecraft was able to
lift the veil from the Face of Venus and produce this spectacular high resolution image of
the planet's surface.
Red, in this false-color map, represents
mountains, while blue represents valleys.
This 3-kilometer resolution
map is a composite of Magellan images compiled between 1990 and 1994.
Gaps were filled in by the Earth-based
Arecibo Radio Telescope.
The large yellow/red area in the north is
Ishtar Terra featuring Maxwell Montes,
the largest mountain on Venus.
The large highland regions are analogous to continents on Earth.
Scientists are particularly interested in
exploring the geology of
Venus because of its similarity to Earth.
APOD: November 10, 1999 - The Belt of Venus
Explanation:
Although you've surely seen it, you might not have noticed it.
During a cloudless
twilight, just before sunrise or after sunset, part of the atmosphere above the
horizon appears slightly off-color, slightly pink.
Visible in the
above photograph, this off-color band between the
dark eclipsed sky and the
blue sky can best be seen in the direction opposite the Sun
and is called the Belt of
Venus.
Straight above,
blue sky is normal sunlight reflecting off the atmosphere.
In the Belt of Venus, however, the atmosphere reflects light
from the
setting (or rising) Sun which
appears more red.
The Belt of Venus can be seen from any location
with a clear horizon.
APOD: September 3, 1999 - Venus Falls Out of the Evening Sky
Explanation:
Orbiting closer to the Sun than planet Earth,
bright Venus
always appears to be near the Sun's position
in our sky and
often shines near the
horizon in
twilight hours.
In fact, after posing as the brilliant
evening star
for the first half of this year, Venus has now
swung around its orbit and is emerging in the predawn twilight as the
morning star.
Taken during its stint as the evening star, this
imaginative long-exposure photo,
of Venus and a 2-day-old crescent Moon gives the
illusion of the pair "falling out" of the western sky.
After an initial short exposure captured the Moon and
Venus, the lens was covered for a few minutes, then left uncovered to
record the
trails until the Moon had set.
APOD: June 19, 1999 - Venus on the Horizon
Explanation:
Venus can appear as a brilliant evening star.
Besides the sun and moon,
Venus is the brightest object visible in Earth's sky.
Because it is closer to the sun than Earth, Venus never strays far
from the sun in
its apparent position and is seen during the year as either
a bright morning or evening star.
This beautiful sunset imaged from low earth orbit by the
Atlantis space shuttle crew
in May 1989 also reveals the planet Venus blazing above Earth's horizon.
It is a fitting image for this
mission and crew.
It was recorded following the successful release of the
robot Venus-explorer Magellan,
the first planetary probe to be deployed from a space shuttle.
APOD: June 12, 1999 - Venus: Just Passing By
Explanation:
Venus,
the second closest planet to the Sun, is a popular
way-point for spacecraft headed for the
gas giant planets
in the outer reaches of the solar system.
Why visit Venus first?
Using a " gravity assist " maneuver,
spacecraft can swing by planets and gain energy during their brief
encounter saving fuel for use at the end of
their long interplanetary voyage.
This colorized image of Venus was recorded by the Jupiter-bound
Galileo spacecraft shortly after its gravity assist flyby of Venus in
February of 1990.
Galileo's glimpse of
the veiled planet shows structure in
swirling sulfuric acid clouds.
The bright area is sunlight
glinting off the upper cloud deck.
The Saturn-bound Cassini spacecraft will
complete its own second flyby of
Venus on June 24th.
Launched in October of 1997,
Cassini should reach Saturn in July 2004.
APOD: May 18, 1999 - A Laguna Triangle
Explanation:
High above
Laguna Beach last month hung bright celestial orbs.
Visible after the California sunset were,
from left to right, the
Moon,
Saturn, and
Venus.
Tonight and for the next few days,
Venus and the Moon
will again be
visible together. Nearby stars will include
Pollux, Castor, and Procyon.
Venus now sets hours after the Sun and is so bright it might be mistaken for an
airplane or
UFO. Binoculars should enable the viewing of
craters on the Moon, and phases for Venus.
APOD: March 8, 1999 - A Jupiter Venus Conjunction
Explanation:
Venus and
Jupiter appeared unusually close together in the sky last month.
The conjunction was easily visible to the unaided eye because
Venus
appears brighter than any background star.
The two planets were not significantly closer in space -
Venus just passed nearly in front of Jupiter as seen from the
Earth.
Visible in the
above photograph are actually five planets.
The faint dot near the top is
Saturn.
Venus is the brightest spot near the center, and
Jupiter is just above it.
Perhaps the hardest to see is Mercury,
visible below Venus but above the foreground
Earth.
A single line nearly connects all the
planets,
a result of all planets orbiting the
Sun in a single plane called the
ecliptic.
APOD: January 24, 1999 - A Venus Landing
Explanation:
This image is part of the first color panoramic view from
Venus.
It was transmitted by a TV camera on the
Soviet Venera 13 lander
which parachuted to thesurface
on March 1, 1982.
Venus' clouds
are composed of sulfuric acid droplets
while its surface temperature is about 900 degrees Fahrenheit
(482 degrees C) at an atmospheric
pressure of 92 times that of sea-level on Earth.
Despite these harsh conditions, the
Venera 13 lander survived
long enough to send back a series of images
and perform an analysis of the
Venusian soil.
Part of the lander itself
is visible in the lower right portion of the image.
An earlier Soviet Venus lander,Venera 7 (1970), was the first spacecraft to return data
from the surface of another planet.
APOD: January 10, 1999 - Venus Once Molten Surface
Explanation:
If you could look at Venus with radar eyes - this is what you might see.
This computer reconstruction of the surface of
Venus
was created from data from the
Magellan
spacecraft.
Magellan orbited
Venus
and used radar to map our neighboring planet's surface between 1990 and 1994.
Magellan found many interesting surface features, including the
large circular domes, typically
25-kilometers across, that are
depicted
above. Volcanism is thought to have created the domes, although the
precise mechanism remains unknown.
Venus'
surface is so hot and hostile that no
surface probe has lasted more than a few minutes.
APOD: August 25, 1998 - Moon, Venus, Jupiter, Phoenix
Explanation:
Before a relaxing sunrise, the sky begins to glow
with unusual delights. Such was the view from Papago Park in
Phoenix,
Arizona this April.
The glittering objects visible in
this photograph are, from lower left to upper right:
Phoenix, our Moon,
Venus, and
Jupiter.
Such proximity is somewhat unusual. Jupiter will be
visible in the evening sky through the rest of the year,
while Venus can be seen in the early morning sky during the month of
September.
APOD: May 1, 1998 - Venus: Just Passing By
Explanation:
Venus,
the second closest planet to the Sun, is a popular
way-point for spacecraft headed for the
gas giant planets
in the outer reaches of the solar system.
Why visit Venus first?
Using a " gravity assist " maneuver,
spacecraft can swing by planets and gain energy during their brief
encounter saving fuel for use at the end of
their long interplanetary voyage.
This colorized image of Venus was recorded by the Jupiter-bound
Galileo spacecraft shortly after its gravity assist flyby of Venus in
February of 1990.
Galileo's glimpse of
the veiled planet shows structure in
swirling sulfuric acid clouds.
The bright area is sunlight
glinting off the upper cloud deck.
The Saturn-bound Cassini spacecraft just
completed its own flyby of
Venus on April 26.
Launched in October of 1997,
Cassini should reach Saturn in July 2004.
APOD: January 20, 1998 - Arachnoids on Venus
Explanation:
Arachnoids are large structures of unknown origin
that have been found only on the surface of
Venus. Arachnoids get their name from their resemblance to
spider-webs.
They appear as concentric ovals surrounded
by a complex network of fractures,
and can span 200 kilometers.
Radar echoes from the
Magellan spacecraft that orbited Venus from 1990 to 1994 built up this image.
Over 30 arachnoids have been identified on
Venus, so far.
The Arachnoid might be a strange relative to the
volcano,
but possibly different
arachnoids are formed by different processes.
APOD: October 16, 1997 - Cassini To Venus
Explanation:
NASA's Saturn Explorer Cassini with
ESA's Titan Probe Huygens attached
successfully rocketed into the skies early yesterday morning.
The mighty Titan 4B Centaur rocket
is seen here across the water gracefully arcing away
from Launch Complex 40 at Cape Canaveral Air Station.
Cassini, a sophisticated,
bus-sized robot spacecraft
is now on its way ... to Venus,
the first planetary way point in its 7 year, 2.2 billion mile
journey to Saturn.
The mission profile calls for Cassini to swing by Venus during
April 1998 and June 1999, Earth in August 1999,
and Jupiter in December 2000.
During each of these
"gravity assist" encounters the six ton
spacecraft will pick up energy needed to
reach Saturn in July 2004.
Cassini's mission is the most ambitious voyage of
interplanetary exploration ever mounted
by humanity and the Huygens Probe's planned descent to
the surface of Titan
will be the most distant landing ever attempted.
APOD: October 14, 1997 - Venus On The Horizon
Explanation:
The month of October features a sky full of planets, including Venus
as the brilliant evening star.
Besides the sun and moon,
Venus is the brightest object visible in Earth's sky.
This month,
Venus appears in early evening near the
red planet Mars
and Mars' red giant
rival Antares
above the southwestern horizon.
Because it is closer to the sun than Earth, Venus never strays far
from the sun in
its apparent position and is seen during the year as either
a bright morning or evening star.
This beautiful sunset imaged from low earth orbit by the
Atlantis space shuttle crew
in May 1989 also reveals the planet Venus blazing above Earth's horizon.
It is a fitting image for this
mission and crew.
It was recorded following the successful release of the
robot Venus-explorer Magellan,
the first planetary probe to be deployed from a space shuttle.
APOD: June 3, 1997 - Venus' Once Molten Surface
Explanation:
If you could look at Venus with radar eyes - this is what you might see.
This computer reconstruction of the surface of
Venus
was created from data from the
Magellan
spacecraft.
Magellan orbited
Venus
and used radar to map our neighboring planet's surface between 1990 and 1994.
Magellan
found many interesting surface features, including the
large circular domes, typically
25-kilometers across, that are
depicted
above. Volcanism is thought to have created the domes, although the
precise mechanism remains unknown.
Venus'
surface is so hot and hostile that no
surface probe has lasted more than a few minutes.
APOD: May 7, 1997 - Ultraviolet Venus
Explanation:
The forecast for Venus is cloudy, cloudy, cloudy. Although similar to the
Earth in size and mass,
Venus'
slightly closer orbit to the
Sun create for it a much thicker
atmosphere and a much hotter surface. The thick atmosphere was
photographed above in
ultraviolet light in 1979 by the
Pioneer
Venus Orbiter. Whether or not
Venus has a moon was the center of a
great
controversy in the 1700s and 1800s. Today we know
Venus has no natural satellites.
Venus's extremely
uncomfortable climate was likely caused by a runaway
greenhouse
effect. Could Earth ever undergo
runaway greenhouse
heating like Venus?
APOD: September 24, 1996 - Beneath Venus' Clouds
Explanation: If the thick clouds covering Venus were removed,
how would the surface appear? Using an imaging radar
technique, the Magellan spacecraft
was able to lift the veil from the Face of Venus
and produce this spectacular high resolution imageof
the planet's surface. Red, in this false-color map, represent
mountains, while blue represents valleys This 3-kilometer resolution
map is a composite of Magellan
images compiled between 1990 and 1994. Gaps were filled in by
the Earth-based Arecibo Radio Telescope.
The large yellow/red area in the north is Ishtar Terra
featuring Maxwell Montes,
the largest mountain on Venus. The
large highland regions are analogous to continents on Earth. Scientists
are particularly interested in exploring the geology of Venus
because of its similarity to Earth.
APOD: September 23, 1996 - Venus: Earth's Cloudy Twin
Explanation: If Venus weren't so cloudy it would be more
similar to Earth. This picture by the Galileo spacecraft
shows just how cloudy Venus
is. Venus
is very similar to Earth in size
and mass - and so is sometimes referred to as Earth's sister planet
- but Venus
has a quite different climate. Venus'
thick clouds and closeness to the Sun
(only Mercury is closer) make it
the hottest planet - much hotter than the Earth. Humans could
not survive there, and no life of any sort has ever been found.
When Venus is visible
it is usually the brightest object in the sky after the Sun and
the Moon. More than 20 spacecraft
have visited Venus
including Venera 9,
which landed on the surface, and Magellan,
which used radar to peer through the clouds and make a map of
the surface. This visible light picture of Venus
was taken by the Galileo spacecraft now
in orbit around Jupiter. Many things about Venus remain unknown,
including the cause of mysterious bursts of radio waves.
APOD: June 24, 1996 - A View from Venus: Rift Valley
Explanation:
Color information from the
Soviet Venera landers and radar data from
the Magellan spacecraft
were used to construct this striking perspective view of the
Venusian landscape. (In this computer
generated image, the vertical scale has been exagerated.)
In the foreground is the edge of a rift valley created by faulting in
the crust of
Venus.
The valley runs all the way to the base of
Gula Mons, a 2 mile high volcano seen here on the right,
some 450 miles in the distance.
On the left is another volcano, Sif Mons.
Using radar to pierce the dense clouds continuously shrouding
the Face of Venus, Magellan was
able to explore over 98% of the Venusian surface, revealing a a diverse and
tantalizing topography.
APOD: April 18, 1996 - Hyakutake, Venus, Orion, and Pond
Explanation:
Can you find
Comet
Hyakutake in the above picture? In this gorgeous
photo, the starry
night sky of April 9th is pictured with its new comet visitor.
In the foreground is a pond
with the lights of Kansas City, Missouri on the western horizon.
On the upper left, the constellation of
Orion is visible.
At the center, the
brightest object in the picture is the
planet Venus. Venus's reflection
can be seen in the pond. On the right - halfway between Venus and the
photograph's edge - can be seen two bright objects fairly close to each
other. Of these two, look closely at lower right object. See the tail?
Comet Hyakutake is
still visible for Northern observers
in the Western sky and now has begun to
brighten again as it nears the Sun.
APOD: September 27, 1995 - A Venus Landing
Explanation:
This image is part of the first color panoramic view from
Venus.
It was transmitted by a TV camera on the
Soviet Venera 13 lander
which parachuted to the
surface
on March 1, 1982. Venus' clouds
are composed of sulfuric acid droplets
while its surface temperature is about 900 degrees Fahrenheit
(482 degrees C) at an atmospheric
pressure of 92 times that of sea-level on Earth.
Despite these harsh conditions, the
Venera 13 lander survived
long enough to send back a series of images
and perform an analysis of the Venusian soil. Part of the lander itself
is visible in the lower right portion of the image.
An earlier Soviet Venus lander,
Venera 7 (1970), was the first spacecraft to return data
from the surface of another planet.
APOD: August 22, 1995 - Venus UnVeiled
Explanation:
The surface of Venus is perpetually
covered by a veil of thick clouds and remains hidden from even the powerful
telescopic eyes of earth-based astronomers. However, using an
imaging radar
technique, the
Magellan
spacecraft was able
to lift the veil from the
Face of Venus
and produce spectacular high resolution images
of the planet's surface. The bright area running across the middle
of this picture represents the largest highland region of Venus
known as
Aphrodite
Terra. The large highland regions are
analogous to continents on Earth. Scientists are particularly interested
in exploring the geology of Venus because of its similarity
to Earth. For more information about Venus and this image see the
Overview
of Venus.
APOD: August 15, 1995 - Venus: Earth's Sister Planet
Explanation:
This picture in visible light was taken by the
Galileo spacecraft.
Venus is very similar to
Earth in size and mass - and so is sometimes referred to as
Earth's sister planet - but Venus has a quite different climate.
Venus'
thick clouds and closeness to the
Sun (only
Mercury is closer) make it the hottest planet - much hotter than
the Earth. Humans could not survive
there, and no life of any sort has ever been found. When
Venus is visible
it is usually the brightest object in the sky after the Sun and the Moon.
More than 20 spacecraft have visited Venus including
Venera 9, which landed on the surface, and
Magellan, which used radar to peer through the clouds
and make a map of the surface. There are still many things about Venus's
unusual atmosphere that astronomers don't understand.