Astronomy Picture of the Day |
APOD: 2024 April 3 – Unusual Nebula Pa 30
Explanation:
What created this unusual celestial firework?
The nebula, dubbed
Pa 30, appears in the same sky direction now as a bright
"guest star" did in the
year 1181.
Although Pa 30's filaments look similar to that created by a nova
(for example GK Per),
and a planetary nebula (for example
NGC 6751), some astronomers
now propose that it was created by a rare type of
supernova:
a thermonuclear Type Iax, and so is (also) named
SN 1181.
In this model, the supernova was not the result of the
detonation of a single star, but rather a blast that occurred when two
white dwarf stars
spiraled together and merged.
The blue dot in the center is hypothesized to be a
zombie star, the remnant white dwarf that
somehow survived this
supernova-level explosion.
The featured image combines images and data obtained with
infrared
(WISE),
visible
(MDM,
Pan-STARRS),
and X-ray
(Chandra, XMM) telescopes.
Future observations and analyses may
tell us more.
APOD: 2024 March 2 - Odysseus on the Moon
Explanation:
Methalox
rocket engine firing, Odysseus' landing legs absorb
first contact with the lunar surface in this wide-angle snapshot from
a camera on board the robotic Intuitive Machines
Nova-C moon lander.
Following the
landing on February 22,
broken landing legs,
visible in the image,
ultimately left the lander at rest but tilted.
Odysseus' gentle lean
into a sloping lunar surface
preserved the phone booth-sized lander's
ability to operate, collect solar power, and
return images and data to Earth.
Its exact landing site
in the Moon's far south polar region
was imaged by NASA's Lunar Reconnaissance Orbiter.
Donated by NASA,
the American flag seen on the lander's central panel is 1970 Apollo
program flight hardware.
APOD: 2022 April 2 - Nova Scotia Northern Lights
Explanation:
This almost otherworldly
display of northern lights was captured in
clear skies during the early hours of March 31 from
44 degrees north latitude, planet Earth.
In a five second exposure the scene looks north from
Martinique Beach Provincial Park in Nova Scotia, Canada.
Stars of the W-shaped constellation Cassiopeia
shine well above the horizon,
through the red tint
of the
higher altitude auroral glow.
Auroral activity was anticipated by skywatchers
alerted to the possibility of
stormy space weather
by
Sun-staring spacecraft.
The predicted geomagnetic storm was sparked as a
coronal mass ejection, launched from
prolific
solar active region 2975, impacted our
fair planet's magnetosphere.
APOD: 2021 August 22 - Explosions from White Dwarf Star RS Oph
Explanation:
Spectacular explosions keep occurring in the binary star system named
RS Ophiuchi.
Every 20 years or so, the
red giant star dumps enough
hydrogen
gas onto its companion white dwarf star to set off a brilliant
thermonuclear explosion on the
white dwarf's surface.
At about 5,000 light years distant, the resulting
nova explosions cause the
RS Oph system to brighten up by a huge factor and become visible to the unaided eye.
The red giant star is depicted on the right of the
above drawing,
while the white dwarf is at the center of the bright
accretion disk on the left.
As the
stars orbit each other, a stream of
gas moves from the giant star to the white dwarf.
Astronomers
speculate that at some time in the
next 100,000 years, enough matter will have accumulated on the
white dwarf to push it over the
Chandrasekhar Limit,
causing a much more powerful and final explosion known as a
supernova.
Starting early this month,
RS Oph was again
seen exploding in a
bright nova.
APOD: 2021 August 16 - Perseid Meteor, Red Sprites, and Nova RS Oph
Explanation:
This was an unusual sky.
It wasn't unusual because of the central band the
Milky Way Galaxy,
visible along the image left.
Most dark skies show part of the
Milky Way.
It wasn't unusual because of the
bright meteor visible on the upper right.
Many images taken during last week's
Perseid Meteor Shower show meteors,
although this
Perseid was particularly
bright.
This sky wasn't unusual because of the red
sprites, visible on the lower right.
Although
this type of lightning has only been noted in the past few decades,
images
of
sprites are becoming more common.
This sky wasn't unusual because of the
nova, visible just above the image center.
Novas bright enough to be seen with the unaided eye occur
every
few
years, with pictured Nova
RS Ophiuchus
discovered about a
week ago.
What was most unusual, though, was to capture all these things together, in a single night, on a single sky.
The
unusual sky occurred above
Zacatecas,
Mexico.
APOD: 2021 June 7 - A Bright Nova in Cassiopeia
Explanation:
What’s that new spot of light in Cassiopeia?
A nova.
Although novas occur frequently throughout the universe, this nova, known as
Nova Cas 2021 or V1405 Cas, became so unusually bright in the
skies of Earth last month that it was visible to the
unaided eye.
Nova Cas 2021 first brightened in mid-March but then, unexpectedly,
became even brighter in mid-May and remained
quite bright for about a week.
The nova then faded back to early-May levels,
but now is slightly brightening again and
remains visible through binoculars.
Identified by the arrow, the nova occurred toward the
constellation of Cassiopeia,
not far from the
Bubble Nebula.
A nova is typically caused by a
thermonuclear explosion on the surface of a
white dwarf star that is
accreting matter from a
binary-star
companion -- although details of this outburst are currently unknown.
Novas don't destroy the underlying star, and are
sometimes seen to recur.
The
featured image
was created from 14 hours of imaging from
Detroit,
Michigan,
USA.
Both professional and amateur astronomers will likely continue to monitor
Nova Cas 2021 and
hypothesize about details of its cause.
APOD: 2021 April 6 - Mars and the Pleiades Beyond Vinegar Hill
Explanation:
Is this just a lonely tree on an empty hill?
To start, perhaps, but
look beyond.
There, a busy universe may wait to be discovered.
First, physically, to the left of the tree, is the planet
Mars.
The red planet, which is the new home to NASA's
Perseverance rover,
remains visible
this month at sunset above the western horizon.
To the tree's right is the
Pleiades,
a bright cluster of stars dominated by several bright blue stars.
The
featured picture is a composite of several separate
foreground and background images taken within a few hours of each other,
early last month, from the same location on
Vinegar Hill in Milford,
Nova Scotia,
Canada.
At that time,
Mars was passing slowly, night after night,
nearly in front of the distant
Seven Sisters star cluster.
The next time Mars will pass
angularly as close to the Pleiades as it did in March will be
in 2038.
APOD: 2020 July 2 - The Galaxy, the Planet, and the Apple Tree
Explanation:
The Old Astronomer's
Milky Way arcs through this peaceful northern sky.
Against faint, diffuse starlight you can follow dark
rifts of interstellar dust clouds stretching from the galaxy's core.
They lead toward
bright star Antares at the right,
almost due south above the horizon.
The brightest beacon in
the twilight
is
Jupiter, though.
From the camera's perspective it seems to hang from the
limb of a tree framing the foreground, an apple tree of course.
The serene
maritime nightscape
was recorded in tracked and untracked
exposures on June 16 from Dover, Nova Scotia, planet Earth.
APOD: 2018 August 6 - Live: Cosmic Rays from Minnesota
Explanation:
Cosmic rays from outer space go through your body every second.
Typically, they do you no harm.
The featured image shows some of these fast moving particles as streaks going through Fermilab's
NOvA Far Detector located in Ash River,
Minnesota,
USA.
Although the image updates every 15 seconds, it only shows
cosmic rays that occurred over a (changing) small fraction of that time, and mostly shows only one type of particle:
muons.
The NOvA
Far Detector's main purpose is not to detect cosmic rays, though, but rather
neutrinos from the
NuMI
beam shot through the Earth from
Fermilab near
Chicago,
Illinois, USA,
810 kilometers away.
Only a few
neutrino events are expected in NOvA per week, though.
The NuMI /
NOvA experiment is allowing humanity to better explore the
nature of neutrinos,
for example how frequently they change type during their trip.
Cosmic rays themselves were
discovered
only about 100 years ago and can not only
alter computer memory,
but may have helped to create
DNA
mutations that resulted in, eventually,
humans.
APOD: 2018 March 25 - Announcing Nova Carinae 2018
Explanation:
How bright will Nova Carinae 2018 become?
The new nova was
discovered only last week.
Although novas
occur frequently throughout the universe, this nova, cataloged as
ASASSN-18fv,
is so unusually bright in the
skies of Earth
that it is now easily visible through binoculars in the
southern hemisphere.
Identified by the arrow,
the nova occurs near the direction of the picturesque
Carina Nebula.
A nova is typically
caused by a thermonuclear explosion on the surface of a
white dwarf star that is accreting matter from a binary companion,
although details of this
outburst are currently unknown.
Both professional and amateur astronomers will be
monitoring this
unusual stellar outburst in the coming weeks, looking to see how
Nova Carinae
2018
evolves, including whether it becomes bright enough to be visible to the unaided eye.
APOD: 2017 June 29 - Symbiotic R Aquarii
Explanation:
A long recognized naked-eye
variable star, R Aquarii
is actually an interacting binary star system, two
stars that seem to have a
close,
symbiotic relationship.
About 710 light years away, it consists of a cool red giant star
and hot, dense white dwarf star in mutual orbit around their common
center of mass.
The binary system's visible light is dominated by the red giant,
itself a Mira-type long period variable star.
But material in the cool giant star's extended envelope is pulled by gravity
onto the surface of the smaller, denser white dwarf,
eventually triggering
a thermonuclear explosion and blasting material into space.
Optical image data (red) shows the still expanding ring of debris
originating from a blast that would have been seen in the early 1770s.
The
evolution of less understood energetic events producing
high energy emission in the R Aquarii system has been
monitored since 2000 using Chandra X-ray Observatory data (blue).
The composite field of view is less that a light-year across at the
estimated distance of R Aquarii.
APOD: 2016 November 21 - Nova over Thailand
Explanation:
A nova in Sagittarius is bright enough to see with binoculars.
Discovered last month by the
All-Sky Automated Survey for Supernovae (ASAS-SN),
the
stellar explosion
even approached the limit of naked-eye visibility last week.
A classical
nova results from a
thermonuclear explosion
on the surface of a
white dwarf star --
a dense star having the size of our Earth but the mass of our Sun.
In the featured image, the nova was
captured last week above ancient
Wat
Mahathat in
Sukhothai,
Thailand.
To see
Nova Sagittarius 2016 yourself,
just go out just after sunset and locate near the western horizon the constellation of the Archer
(Sagittarius), popularly identified with an
iconic teapot.
Also visible near the
nova is the very bright planet Venus.
Don’t delay, though, because not only is the
nova fading,
but that part of the sky is setting continually closer to sunset.
APOD: 2015 March 25 - Naked Eye Nova Sagittarii 2015 No 2
Explanation:
It quickly went from obscurity to one of the brighter stars in Sagittarius -- but it's fading.
Named
Nova Sagittarii 2015 No. 2, the
stellar explosion is the brightest
nova visible from Earth in
over a year.
The featured image was captured four days ago from
Ranikhet in the
Indian
Himalayas.
Several stars in western
Sagittarius make an
asterism known as the
Teapot, and the nova, indicated by the arrow,
now appears like a new emblem on the side of the
pot.
As of last night,
Nova Sag has faded from
brighter than visual
magnitude 5 to the edge of unaided visibility.
Even so, the nova should still be easily
findable with binoculars in dark skies before sunrise over the next week.
APOD: 2015 January 11 - Cataclysmic Dawn
Explanation:
Will this dawn bring another nova?
Such dilemmas might be pondered one day by
future humans
living on a planet orbiting a
cataclysmic variable
binary star system.
Cataclysmic variables involve gas falling from a large star onto an
accretion disk surrounding a massive but compact
white dwarf star.
Explosive cataclysmic events such as a
dwarf nova
can occur when a clump of gas in the interior of the
accretion disk
heats up past a certain temperature.
At that point, the clump will fall more quickly onto the
white dwarf and land with a bright flash.
Such dwarf novas will not destroy either star,
and may occur irregularly on time scales from a few days to tens of years.
Although a nova is much less energetic than a supernova, if
recurrent novas are not
violent enough to expel more gas than is falling in,
mass will accumulate onto the
white dwarf star until it passes its
Chandrasekhar limit.
At that point, a
foreground cave may provide little protection,
as the entire white dwarf star will explode in a
tremendous supernova.
APOD: 2013 December 7 - Naked Eye Nova Centauri 2013
Explanation:
Brightest stellar beacons of the constellation Centaurus,
Alpha and Beta
Centauri are easy to spot from the southern hemisphere.
For now, so is new naked eye
Nova Centauri 2013.
In this night skyscape recorded near Las Campanas Observatory in
the Chilean southern Atacama desert on December 5,
the new star joins the old in the expansive constellation,
seen at early morning hours through a
greenish airglow.
Caught by nova hunter
John Seach from Australia on December 2
as it approached near naked eye
brightness, Nova Cen 2013
has been spectroscopically
identified as a classical nova, an interacting binary star system
composed of a dense, hot white dwarf and cool, giant companion.
Material from the companion star builds up as it
falls onto the white dwarf's surface triggering a thermonuclear event.
The
cataclysmic blast
results in a drastic increase in brightness
and an expanding shell of debris.
The stars are not destroyed, though.
Classical novae are thought to recur when
the flow of material onto the white dwarf
eventually resumes and produces another outburst.
APOD: 2013 August 23 - A Spectrum of Nova Delphini
Explanation:
When a new star
appeared in the constellation Delphinus late last week,
astronomers
found its spectrum hinted at the apparition's true nature.
Now known as Nova Delphini 2013, its
visible light spectrum near
maximum
brightness
is centered in this image of the nearby
star field captured with
prism and
telescope on the night of August 16/17 at the
Sternwarte Bülach,
Switzerland.
Strong absorption lines due to hydrogen atoms
are seen as the darkest bands in the nova's spectrum, but
the strong absorption lines are bordered along their redward edge by bright
bands of emission.
That pattern is the
spectral signature
of material blasted from
a type of catalysmic binary system known as
a classical nova.
Other stars in field are fainter, identified by their
Hipparcus
catalog numbers, brightness in
magnitudes, and
spectral types.
By chance, the faint emission line from
planetary nebula NGC 6905
was also included, indicated at the lower right.
APOD: 2013 August 17 - M8: The Lagoon Nebula
Explanation:
This beautiful cosmic cloud is a popular stop on telescopic tours of
the constellation
Sagittarius.
Eighteenth century cosmic tourist
Charles
Messier cataloged the bright
nebula as M8.
Modern day astronomers recognize the Lagoon Nebula as an active
stellar nursery about 5,000 light-years distant, in the direction
of the center of our Milky Way Galaxy.
Hot stars in the embedded open star cluster
NGC 6530
power the nebular glow.
Remarkable features can be traced through
this sharp picture, showing off
the Lagoon's
filaments of glowing gas and dark dust clouds.
Twisting near the center of the Lagoon,
the small, bright hourglass shape is the turbulent
result of extreme stellar winds and intense starlight.
The alluring color view
was captured with a telescope and
digital camera while M8 was high in dark, rural Argentina skies.
At the nebula's estimated distance, the picture
spans
over 60 light-years.
APOD: 2013 August 16 - Nova Delphini 2013
Explanation:
Using a small telescope to scan the skies on August 14,
Japanese amateur astronomer Koichi Itagaki
discovered a "new" star
within the boundaries of the constellation Delphinus.
Indicated in this skyview captured on August 15 from Stagecoach,
Colorado, it is now appropriately designated Nova Delphini 2013.
Sagitta,
the Arrow, points the way to the
newcomer's location
high in the evening sky, not far from bright star Altair
and the asterism known to
northern hemisphere skygazers as the Summer Triangle.
The nova is reported to be easy
to
spot with binoculars, near the limit of naked-eye visibility
under dark skies.
In fact, previous deep sky charts do show a much fainter
known star (about 17th
magnitude) at the position of Nova Delphini,
indicating this star's apparent brightness suddenly
increased over 25,000 times.
How does a star undergo such a
cataclysmic change?
The spectrum
of Nova Delphini
indicates it
is a classical nova, an interacting binary star system in which one star
is a dense, hot
white dwarf.
Material from a cool, giant companion star
falls onto the surface of the white dwarf,
building up until it triggers a thermonuclear event.
The drastic increase in brightness and an expanding shell
of debris is the result - but
the stars are not destroyed!
Classical novae are
believed to recur when the flow of material onto the white dwarf
resumes and produces another outburst.
APOD: 2013 August 15 - The Magellanic Stream
Explanation:
In
an astronomical version
of the search for the source
of the Nile,
astronomers now have strong evidence for the origin of the
Magellanic Stream.
This composite image shows the long ribbon of gas,
discovered at radio wavelengths in the 1970s,
in pinkish hues against an optical all-sky view across the plane
of our Milky Way galaxy.
Both Large and Small
Magellanic Clouds, dwarf satellite galaxies
of the the Milky Way, are seen near the head of the stream at the right.
Data from Hubble's Cosmic Origins Spectrograph
were used to
explore abundances
of elements along sightlines to quasars that
intersect the stream.
The results indicate that most of the stream's material comes from the
Small Magellanic Cloud.
The Magellanic Stream is likely the result of gravitational
tidal interactions
between the two dwarf galaxies
some 2 billion years ago, the Small Magellanic Cloud
losing more material in the encounter because of its lower mass.
APOD: 2011 November 5 - GK Per: Nova of 1901
Explanation:
Early in the
20th century, GK Persei
briefly became one of the brightest stars in planet Earth's sky,
an event known as Nova Persei 1901.
Documented in
this modern day composite of two images
from 2003 and 2011 the ejecta from the explosion,
popularly called the Firework Nebula, continues to expand into space.
These images are part of a
time lapse video
tracking the nebula's expansion over the last 17 years.
About 1500 light-years away, the nebula is still just under
a light-year in diameter.
GK Per and similar
cataclysmic variable stars known as
classical novae are understood to be binary
systems consisting of a compact
white dwarf star and
swollen cool giant star in a close orbit.
The build up of mass transferred to the surface of the
white dwarf from the giant star through an accretion disk
eventually triggers a thermonuclear outburst, blasting
the stellar material into space without destroying the
white dwarf star.
With a 2 day orbital period, the
GK Per system has produced
much smaller outbursts
in recent years.
APOD: 2009 November 17 - Dawn Before Nova
Explanation:
Will this dawn bring another nova?
Such dilemmas might be pondered one day by
future humans
living on a planet orbiting a
cataclysmic variable
binary star system.
Cataclysmic variables involve gas falling from a large star onto an
accretion disk surrounding a massive but compact
white dwarf star.
Explosive cataclysmic events such as a
dwarf nova
can occur when a clump of gas in the interior of the
accretion disk
heats up past a certain temperature.
At that point, the clump will fall more quickly onto the
white dwarf and land with a
bright flash.
Such dwarf novas will not destroy either star, and may occur irregularly on time scales from a few days to tens of years.
Although a nova is much less energetic than a supernova, if
recurrent novas are not
violent enough to expel more gas than is falling in,
mass will accumulate onto the white dwarf star until it passes its
Chandrasekhar limit.
At that point, a foreground cave may provide little protection,
as the entire white dwarf star will explode in a
tremendous supernova.
APOD: 2007 February 19 - Nova Over Iran
Explanation:
A bright new nova is being studied by astronomers.
The officially dubbed
Nova Scorpii 2007
has become so bright in recent days that it is
now visible
to the unaided eye.
Adventurous early morning
sky enthusiasts should look in dark skies toward the
constellation of the
Scorpion, just below Jupiter and
Antares.
The above image may help as a sky chart.
A nova this bright occurs only
every few years.
Novas
are caused by
thermonuclear explosions
casting off the outer layers of a
white dwarf star.
Pictured above on Friday, the nova was being studied through a
small telescope as it appeared over the
Varzaneh Desert in
Isfahan,
Iran.
The
nova will likely fade but remain
visible with binoculars for at least a few more days.
APOD: 2006 July 26 - Explosions from White Dwarf Star RS Oph
Explanation:
Spectacular explosions keep occurring in the binary star system named
RS Ophiuchi.
Every 20 years or so, the
red giant star dumps enough
hydrogen
gas onto its companion white dwarf star to set off a brilliant
thermonuclear explosion on the
white dwarf's surface.
At about 2,000 light years distant, the resulting
nova explosions cause the
RS Oph system to brighten up by a huge factor and become visible to the unaided eye.
The red giant star is depicted on the right of the
above drawing,
while the white dwarf is at the center of the bright
accretion disk on the left.
As the stars orbit each other, a stream of
gas moves from the giant star to the white dwarf.
Astronomers speculate that at some time in the next 100,000 years, enough matter will have accumulated on the
white dwarf to push it over the
Chandrasekhar Limit,
causing a much more powerful and final explosion known as a
supernova.
APOD: 2006 February 24 - Recurrent Nova RS Ophiuci
Explanation:
This pretty star field in the constellation
Ophiucus is
centered on a star not often seen - RS Ophiuci.
In fact, early last week
RS Oph suddenly became
visible to the naked eye for the first time since 1985.
A type of cataclysmic variable star
classified
as a recurrent nova, RS Oph
dramatically
increased in brightness from 11th
magnitude,
too faint to appear on some star charts.
Historically,
RS Oph was seen to go through only four
similar outbursts
since 1898.
Such stars are now
modeled
as interacting binary star
systems, composed of a compact white dwarf star co-orbiting
with a swollen red giant.
As material falls away from the red
giant it collects in a rotating accretion
disk before ultimately falling on to the white dwarf.
Disk instabilities, or a build up of material on
the compact star result in the occasional but rapid release of
energy through nuclear burning.
At an estimated distance of 3,000 light-years,
RS Ophiuci is
now reported to be fading rapidly.
This telescopic view spans about 2 degrees (4 full moons)
and was captured on the morning of February 16 from the
RAS Observatory
under New Mexico skies.
APOD: 2005 November 27 - Light Echoes from V838 Mon
Explanation:
What caused this outburst of V838 Mon?
For reasons unknown, star V838 Mon's
outer surface suddenly greatly expanded with the
result that it became the brightest star in the entire
Milky Way Galaxy in January 2002.
Then, just as suddenly, it faded.
A stellar flash like this has never been seen before --
supernovas
and novas expel matter out into space.
Although the V838 Mon flash appears to expel material into space, what is seen in the
above image from the
Hubble Space Telescope
is actually an outwardly moving
light echo of the bright flash.
In a light echo, light from the flash is
reflected by successively more distant rings in the complex array of ambient
interstellar dust
that already surrounded the star.
V838 Mon lies about 20,000
light years away toward the constellation of the unicorn
(Monoceros), while the
light echo above spans about six
light years in diameter.
APOD: 2005 January 16 - Nebula Nova Cygni Turns On
Explanation:
Old photographs show no evidence of the above nebula.
In 1992, a white dwarf star toward the constellation of Cygnus blew off its outer layers in a classical nova explosion: an event called
Nova Cygni 1992.
Light flooded the local
interstellar neighborhood, illuminated this existing gas cloud,
excited the existing
hydrogen,
and hence caused the red emission.
The only gas actually expelled by the
nova can be seen as a small red ball just above the
photograph's center.
Eventually, light from the nova shell will fade, and this nebula will again become invisible.
APOD: 2002 October 3 - V838 Mon: Mystery Star
Explanation:
A leading candidate for the most mysterious star found in recent
times is variable star
V838 Monocerotis.
At a distance of about 8,000 light-years, V838
Mon was
discovered
to be in outburst in January of this year.
Initially thought to be a familiar type of
classical nova, astronomers
quickly realized that instead, V838 Mon may be a totally new addition to
the astronomical zoo.
Observations indicate
that the erupting star transformed itself
over a period of months from a small under-luminous star a little
hotter than the Sun, to a highly-luminous, cool supergiant star undergoing
rapid and complex brightness changes.
The transformation defies the conventional understanding of
stellar life cycles.
A most notable feature of V838 Mon is the "expanding" nebula which
now appears to surround it.
Seen above in two separate images from the
South African Astronomical
Observatory's 1 meter telescope,
the nebula is probably a light echo
from
shells of formerly unseen material lost by the star
during its previous evolution.
Light-years in diameter, the shells progressively reflect
the light from
V838 Mon's
outbursts, providing
an opportunity to look back at the history of this
remarkable star's behaviour.
APOD: 2002 August 25 - Nebula Nova Cygni Turns On
Explanation:
Old photographs show no evidence of the above nebula.
In 1992, a white dwarf star toward the
constellation of Cygnus blew off its outer layers in a classical
nova explosion: an event called
Nova Cygni 1992.
Light flooded the local
interstellar neighborhood, illuminated this existing gas cloud,
excited the existing
hydrogen,
and hence caused the red
emission.
The only gas actually expelled by the
nova can be seen as a small red ball just above the
photograph's center.
Eventually, light from the
nova shell will fade,
and this nebula will again become invisible!
APOD: 2000 November 28 - BZ Cam Bow Shock
Explanation:
BZ Cam is a
binary star system
that is not well understood.
In most cataclysmic variables, matter from a
normal star accumulates on the surface of the companion
white dwarf star,
eventually causing a
nova-like flare as the
material becomes hot enough to ignite
nuclear fusion.
In BZ Cam, however, light appears to flicker unpredictably,
and an unusually large
wind of particles is being expelled.
Pictured above,
BZ Cam's wind creates a large
bow-shock as the system moves through surrounding
interstellar gas.
BZ Cam lies about 2500
light-years away toward the constellation of
Camelopardalis.
APOD: 2000 August 16 - Unusual Giant Galaxy NGC 1316
Explanation:
Can unusual giant galaxy NGC 1316 help calibrate the universe?
Quite possibly -- if it turns out this atypical galaxy
is composed of typical stars.
NGC 1316,
pictured above, is most obviously strange because
it has a size and shape common for an
elliptical galaxy but
dust lanes and a disk
more commonly found in a
spiral galaxy.
These attributes could be caused by
interactions with
another galaxy over the past billion years.
Most recently,
NGC 1316 has been monitored to find
novae, explosions emanating from
white dwarf stars that should
have a standard brightness.
Again,
NGC 1316 was found atypical in that the nova rate
was unexpectedly high.
If, however, the stars and
white dwarfs that compose
NGC 1316 are typical, then the
novae observed should be just as bright as
novae in other galaxies so that astronomers can
use them to compute an accurate distance.
This distance can then be used to calibrate other
distance indicators and result in a more accurate
scale for distances throughout the
universe.
APOD: December 15, 1999 - A Nova In Aquila
Explanation:
On December 1st,
experienced
observers patroling the night sky
with binoculars noticed what seemed to be
a new star in the constellation
of Aquila (The Eagle).
It wasn't really a new star though.
A comparison with detailed skymaps revealed the amazing truth,
there was a known star at that position in the sky ... its brightness
had simply increased by about 70,000 times.
The star, now fondly known to
variable star observers as Nova
V1494 Aquilae, continued to grow brighter for several days,
becoming easily visible to the unaided eye before starting
to slowly fade away.
Its position within the constellation is indicated on
this wide-angle picture taken on December 4th, near the time
it was brightest.
What would cause a star to undergo such a cataclysmic change?
This "new star" appears to be a
classical nova.
Classical novae are thought to be
interacting binary star systems in which one of the pair
is a dense, hot white dwarf.
Material from the companion falls onto the surface of the white dwarf,
building up until it triggers a thermonuclear blast.
A stunning increase in brightness and an expanding shell of
debris result - but the binary system is likely not destroyed!
Classical novae are
believed to recur as the flow
of material resumes and produces another outburst
in perhaps hundreds of years time.
APOD: May 24, 1999 - Introducing Nova Velorum 1999
Explanation:
A bright nova was discovered Saturday that is
currently visible to the unaided eye in southern skies.
Nova Velorum 1999 was recorded near visual magnitude 3
independently by discoverers Peter Williams and
Alan C. Gilmore (Mt. John U. Obs.),
making it more luminous than many famous bright stars.
The last nova this bright was
Nova Cygni 1975, which peaked just brighter than
magnitude 2.
Nova Velorum 1999 is brighter now than the well-studied
Nova Cygni 1992 ever
appeared.
A nova occurs when the surface of a
white dwarf star
undergoes a tremendous
thermonuclear explosion, throwing off its outer layers.
How the nova will appear over the next few weeks is uncertain,
but the exploding debris will likely fade beyond detectability
over the next few years.
The
above photograph of Nova Velorum 1999 was
taken yesterday from Australia. The
cross-hair like spikes
that appear around it were caused by the
photographing telescope and camera.
APOD: September 11, 1998 - Help Map The Moon
Explanation:
You can help map
the Moon.
Early tomorrow morning
(Saturday, September 12) the Moon will occult, or pass in front of,
the bright star
Aldebaran as viewed from some Southern and Eastern areas
of the U.S. as well as regions in the Caribbean Sea,
Nova Scotia, Newfoundland, Mexico, and Central America.
Aldebaran will
disappear behind the bright edge of the third quarter
moon and
reappear behind the darkened edge.
Accurately timed home video camera recordings
from different locations
can be used to make improved maps of the height of the lunar terrain
at these occultation points.
Interested?
Follow
the instructions on the
International Occultation Timing Association HomePage
which detail how to tape a familiar TV channel,
take your running camcorder outside to record the occultation,
and then return to tape a few more minutes of the TV channel.
(First, determine if the occultation will be visible from your location!)
You can then donate your tape by mailing it to the address given.
Leave yourself plenty of time
for a practice run and be sure to check the weather
before going to a lot of trouble!
This mosaic
mapping the North polar region of the lunar surface was
constructed from images recorded by the Galileo spacecraft in 1992.
APOD: July 4, 1998 - The Firework Nebula
Explanation:
Imaged by the WIYN Telescope,
the Firework Nebula
is the result of a type of stellar explosion called a nova.
In a nova,
a nuclear detonation on the surface of a compact
white dwarf star blasts away material
that has been
dumped on its surface by a companion star.
Also known as
GK Persei or Nova
Persei,
this nova became one of the brightest stars in the night sky
in the year 1901.
As it faded, astronomers could see an
expanding shell of
gas that eventually became this spectacular nebula.
While not exactly predictable,
GK Per undergoes minor outbursts every three or four years.
APOD: September 25, 1997 - T Pyxidis: Recurrent Nova
Explanation:
What happens when a
thermonuclear blast occurs on the surface of a
white dwarf
star?
Over the years astronomers have watched (at a safe distance ...) as,
6,000 light years from Earth in
the southern constellation Pyxis,
a binary star known as T Pyxidis
repeatedly produces these fearsome explosions.
This Hubble Space Telescope
image of nova T Pyx captures what appear to be
blobs rather than the expected shells
of material expanding from this interacting star system.
Like other binary star systems which
produce nova outbursts,
T Pyx is composed of
a dense white dwarf and a close companion star.
An outburst occurs when the temperature and density of the sea of
matter dumped from the companion
onto the surface of the white dwarf reach
the nuclear flash point for hydrogen.
While material is violently blown off, the
white dwarf
itself is not disrupted and soon begins to accumulate
more matter from its companion, repeating the cataclysm a few years
later.
APOD: December 16, 1996 - Nebula Nova Cygni Turns On
Explanation: Old photographs show no evidence of the above
nebula. In 1992, a white dwarf star in Cygnus
blew off its outer layers in a classical nova explosion:
an event called Nova Cygni 1992.
Light flooded the local interstellar neighborhood, illuminated
this existing gas cloud,
excited the existing hydrogen,
and hence caused the red emission. The only gas actually expelled
by the nova
can be seen as a small red ball just above the photograph's center.
Eventually, light from the nova shell
will fade, and this nebula will again become invisible!
APOD: December 27, 1995 - Nova Cygni 1992
Explanation:
In 1992 a tremendous explosion occurred in the
constellation of
Cygnus.
Dubbed Nova Cygni 1992, this event most probably occurred in an
accretion disk binary system. Astronomers
hypothesize that this system's
white dwarf
had so much gas dumped onto it's surface that conditions became ripe for
nuclear fusion.
The resulting thermonuclear detonation blasted much of
the surrounding gas into an expanding shell. The
Hubble Space Telescope
photographed this expanding shell in 1994. Nova Cygni 1992 was the
brightest nova in recent history - at its brightest it could be seen
without a telescope. It was observed in every part
of the
electromagnetic spectrum.
APOD: July 4, 1995 - The Firework Nebula
Explanation:
The Firework Nebula, known to astronomers as "GK Per", is the result of
a type of stellar explosion called a nova. In a nova, a very compact
star called a white dwarf blasts away gas that had accumulated on its
surface. In this case the nova occurred in the year 1901 and is called
Nova Persei 1901. This nova became as bright as one of
the brighter stars we see in the night sky, but then faded until only a
telescope could see it. Soon astronomers could see an expanding shell
of gas that eventually became this spectacular nebula. The unusual
"fireworks" type feature of this nebula is still a matter of research
and discussion.