APOD
The Astronomy Picture of the Day is a wonderful web site that puts up a different astronomy-related picture every day. However, the site does not have an RSS feed. This page fixes that deficiency.
Updated: 1 hour 27 min ago
Four Planet Sunset
Four Planet Sunset
This mesmerizing sunset photo was taken from the summit of volcanic
Mount Lawu,
3,265 meters above sea level, on July 21.
The view looks west, toward the city lights of
Surakarta
(aka Solo), Central Java, Indonesia.
Two other volcanic peaks, sharp Merapi (left) and Merbabu
lie along the colorful horizon.
Four planets shine in the twilight sky above them.
Spread out near the
plane of the ecliptic are
Mercury,
Venus,
Mars, and
Saturn, along with bright
Regulus, alpha star of the constellation Leo.
For help finding them, just put your cursor over the picture.
In fact, these four planets still shine in western skies at sunset,
with Venus, Mars, and Saturn
grouped much more tightly
this weekend and in
early August.
By August 12, a young crescent Moon will join
the four planet sunset.
Eclipse on the Beach
Eclipse on the Beach
As the
New Moon's
shadow slid across the southern Pacific
on July 11, people gathered along the white, sandy
Anakena Beach on the north side of
Easter Island to watch a
total
solar eclipse.
The experience was captured in this tantalizing composite image,
constructed from a sequence of 50 consecutive exposures.
At their center is the totally eclipsed Sun surrounded by a
shimmering solar corona.
From the well chosen viewpoint, palm trees appear in silhouette
against a darkened sky and the faint light reflected in the water.
Of course,
towering above the onlookers, at the
boundaries of
land, ocean, and sky are Moai,
the island's
mysterious monolithic statues.
Sunset, Shadowrise
Sunset, Shadowrise
From central Australia,
this serene
360 degree panorama follows a clear horizon as
twilight began on May 28.
At left, a bright western sky is still illuminated by
the setting Sun.
But sweeping right, toward a view centered on the
countryside's dominating sandstone
formation called Uluru or
Ayers Rock,
the sky takes on progressively darker hues
and subtle colors.
Behind Uluru is the
shadow
of planet Earth itself,
a dark blue arch rising in the east.
Cast through the dense atmosphere and still close to the horizon,
Earth's long shadow is bounded above by a pinkish
glow or antitwilight arch.
Known as the Belt of Venus,
the lovely color of the antitwilight arch is due to
backscattering of reddened light from the setting Sun.
On that night, a nearly full
Moon also rose above Earth's shadow
in the eastern sky.
The Trifid Nebula is Stars and Dust
The Trifid Nebula is Stars and Dust
Unspeakable beauty and unimaginable bedlam can be found
together in the
Trifid Nebula.
Also known as M20,
this photogenic nebula is visible
with good binoculars towards the constellation of Sagittarius.
The energetic processes of
star formation create not only the colors but the
chaos.
The red-glowing gas
results from high-energy starlight striking interstellar
hydrogen gas.
The dark dust
filaments that lace
M20 were created in the atmospheres of cool
giant stars and in the debris from
supernovae explosions.
Which bright young stars light up the blue
reflection nebula is still
being investigated.
The light from
M20
we see today left perhaps 3,000 years ago,
although the exact distance remains unknown.
Light takes about 50 years to cross
M20.
The Milky Way Over Bryce Canyon
The Milky Way Over Bryce Canyon
What are those strange rock structures?
They are towers and walls of sedimentary rock that are particularly plentiful in
Bryce Canyon in
Utah,
USA.
The rock columns may rise higher than 50 meters and are called
hoodoos.
On the far left is
Thor's Hammer,
perhaps the most famous
hoodoo.
The tall rock columns were carved, most typically, when a unusually dense cap of rock provided a layer of protection to rock underneath from rain-based
erosion.
In the above panoramic picture taken earlier this month and compressed horizontally, the foreground rocks were momentarily illuminated by a roving spotlight.
Visible in the background are a few
water clouds
a few kilometers away hovering over the nearby Earth.
Visible well beyond that are thousands of
individually discernible stars
averaging a few hundred
light years away in the nearby
Milky Way Galaxy.
Far in the distance lie billions of stars that are thousands of light years away and compose the faintly glowing arch that is the visible
central band of the flat disk of our Milky Way.
Over many years, wind and rain will eventually cause the tops of the
hoodoos to topple, whereafter the
underlying column will likely completely erode away.
Lutetia: The Largest Asteroid Yet Visited
Lutetia: The Largest Asteroid Yet Visited
As humans explore the universe, the record for largest asteroid
visited by a spacecraft has increased yet again.
Earlier this month, ESA's robotic
Rosetta spacecraft zipped past the asteroid 21 Lutetia
taking data and snapping images in an effort to better
determine the history of the asteroid and the origin of its
unusual colors.
Although of unknown composition,
Lutetia is not massive enough for gravity to pull it into a sphere.
Pictured above on the upper right, the 100-kilometer across
Lutetia is shown in comparison with the other nine asteroids and four comets that have been visited, so far, by human-launched spacecraft.
Orbiting in the main asteroid belt,
Lutetia
shows itself to be a heavily cratered remnant of the early Solar System.
The Rosetta spacecraft is
now continuing onto
comet Churyumov-Gerasimenko where a landing is planned for 2014.
Happy People Dancing on Planet Earth
Happy People Dancing on Planet Earth
What are these humans doing?
Dancing.
Many humans on Earth exhibit periods of happiness, and one method of displaying happiness is dancing.
Happiness and dancing transcend
political boundaries and occur in practically every human society.
Above, Matt Harding
traveled through many nations on Earth, started dancing, and filmed the result.
The video
is perhaps a dramatic example that
humans from all over
planet Earth
feel a
common bond
as part of a
single species.
Happiness
is frequently contagious -- few people are able to watch the
above video without
smiling.
Diamond Ring and Shadow Bands
Diamond Ring and Shadow Bands
As the total phase of
July 11's solar eclipse came to an end,
sunlight streaming past the edge of the Moon's silhouette
created the fleeting appearance of a glistening
diamond ring
in the sky.
Seen through a thin cloud layer
from the French Polynesian
atoll of Hao it also produced remarkable
shadow bands,
flickering across the dramatic scene.
Projected onto the cloud layer, the shadow bands are parallel
to the sliver of sunlight emerging from behind the Moon's edge.
Caused by turbulence in
Earth's atmosphere refracting the sliver of sunlight,
the narrow bands were captured
in this brief, 1/400th second exposure.
Shining through the cloud droplets, the sunlight also
produced a luminous atmospheric corona, not to be confused with
the solar corona seen during eclipse totality.
The
atmospheric corona is centered on the bright diamond of
emerging sunlight.
Messier 76
Messier 76
"Nebula at the right foot
of
Andromeda ... " begins the description
for the 76th object in Charles Messier's 18th century Catalog
of
Nebulae and Star Clusters.
In fact, M76 is
one of the fainter objects on the Messier list and
is also known by the popular name of the "Little Dumbbell Nebula".
Like its brighter namesake M27
(the Dumbbell Nebula), M76 is recognized
as a planetary
nebula - a gaseous shroud cast off by a
dying sunlike star.
The nebula itself is thought to be shaped more like a donut, while the
box-like appearance of its brighter central
region is due to our nearly edge-on view.
Gas expanding more rapidly away from the donut hole produces the
fainter loops of far flung material.
The fainter material is emphasized in this composite image, highlighted
by showing emission from hydrogen atoms in orange and oxygen atoms
in complementary blue hues.
The nebula's dying star can be picked out in
the
sharp false-color image as blue-tinted star near the
center of the box-like shape.
Distance estimates place M76 about 3 to 5 thousand light-years away,
making the nebula over a
light-year in diameter.
The Meteor of 1860 </b>
The Meteor of 1860
Frederic
Church (1826-1900), American landscape painter
of the Hudson River School, painted what he saw in nature.
And on July 20th, 1860, he saw a spectacular string of
fireball meteors
cross the Catskill evening sky, an extremely
rare Earth-grazing meteor procession.
From New York City, poet
Walt
Whitman (1819-1892)
also wrote of the "... strange huge meteor procession,
dazzling and clear, shooting over our heads" in his poem
Year
of Meteors (1859-60).
But the inspiration for Whitman's words was forgotten.
His astronomical reference became a mystery,
the subject of scholarly debate
until
Texas State University physicists Donald Olson and Russell Doescher,
English professor Marilynn Olson, and
Honors Program student Ava Pope,
located reports documenting the date and timing of the
spectacular meteor procession.
The breakthrough was spotting the
connection with Church's relatively little-known painting.
Fittingly, the
forensic
astronomy team's work was just published, on the 150th anniversary of the
cosmic event that inspired both poet and painter.
The Crown of the Sun
The Crown of the Sun
During a total solar eclipse,
the Sun's
extensive outer atmosphere, or corona, is an inspirational sight.
Subtle shades and shimmering features
that engage
the eye span a brightness range of over
10,000 to 1, making them notoriously difficult
to capture in a single photograph.
But this composite of 7 consecutive digital images
over a range of exposure times comes close to revealing
the crown of the
Sun in all its glory.
The telescopic views were recorded from the Isla de Pascua
(Easter Island) during July 11's
total solar eclipse
and also show solar prominences extending
just beyond the edge of the
eclipsed
sun.
Remarkably, features on the dim, near side of the New Moon can also be
made out, illuminated by sunlight reflected from a
Full Earth.
Lightning Over Athens
Lightning Over Athens
Have you ever watched a lightning storm in awe?
Join the crowd.
Oddly, nobody knows exactly how
lightning is produced.
What is known is that charges slowly separate in some clouds causing rapid electrical discharges
(lightning), but how electrical charges get separated in clouds remains a topic of much research.
Lightning usually takes a jagged course,
rapidly heating a thin column of air to about three times the surface temperature of the
Sun.
The resulting shock wave starts
supersonically and decays into the
loud sound known as
thunder.
Lightning bolts are common in clouds during rainstorms, and on average
6,000 lightning bolts occur between clouds and the Earth every minute.
Pictured above, an
active lightning storm was recorded over
Athens,
Greece earlier this month.
Dark River, Wide Field
Dark River, Wide Field
A Dark River of dust seems to run from our Galactic Center,
then pool into a
starfield containing photogenic sky wonders.
Scrolling right will reveal many of these objects including (can you find?) the bright orange star
Antares, a
blue(-eyed) horsehead nebula, the white
globular star cluster M4,
the bright blue star system Rho Ophiuchi,
the dark brown Pipe nebula,
the red Lagoon nebula,
the red and blue Trifid nebula,
the red Cat's Paw Nebula,
and the multicolored but still important
center of our Galaxy.
This wide view
captures in exquisite detail about 50 degrees of the
nighttime sky,
100 times the size of the full Moon, covering constellations from
the Archer
(Sagittarius) through
the Snake Holder
(Ophiuchus), to
the Scorpion
(Scorpius).
The Dark River itself can be identified as the brown dust lane connected to
Antares,
and spans about 100 light years.
Since the Dark River
dust lane lies only about 500 light years away, it only appears as a bridge to the much more distant Galactic Center, that actually lies about 25,000 light years farther away.
The Antennae Galaxies in Collision
The Antennae Galaxies in Collision
Two galaxies are squaring off in
Corvus and
here are the latest pictures.
But when two
galaxies collide, the stars that compose them usually do not.
That's because
galaxies are mostly empty space and, however bright,
stars only take up only a small amount of that space.
During the slow, hundred million year
collision,
one galaxy can still rip the other apart gravitationally, and
dust and
gas common to both galaxies does
collide.
In
this clash of the
titans, dark
dust pillars mark massive
molecular clouds are being compressed during the
galactic encounter,
causing the rapid birth of millions of stars,
some of which are gravitationally bound together in
massive star clusters.
Galaxies in the River
Galaxies in the River
Large galaxies grow by eating small ones.
Even our own galaxy practices
galactic cannibalism,
absorbing small galaxies that get too close and
are captured by
the Milky Way's gravity.
In fact, the practice is common in the universe and
illustrated by this striking pair of interacting galaxies
from the banks of the southern constellation
Eridanus
(The River).
Located over 50 million light years away,
the large, distorted spiral NGC 1532 is seen locked in a
gravitational
struggle with dwarf galaxy NGC 1531, a struggle the smaller galaxy
will eventually lose.
Seen edge-on, spiral NGC 1532 spans about 100,000 light-years.
Nicely detailed in this sharp image, the
NGC 1532/1531 pair is thought to be similar
to the well-studied system of face-on spiral and small companion
known as M51.
Shaping NGC 6188
Shaping NGC 6188
Dark shapes with bright edges winging their way through dusty
NGC
6188 are tens of light-years long.
The emission nebula is found near the edge of an
otherwise dark large molecular cloud in the southern
constellation
Ara, about 4,000 light-years away.
Formed in that region only a few million years ago, the massive young
stars of the embedded Ara
OB1 association
sculpt the fantastic shapes and
power the nebular glow with
stellar winds and intense ultraviolet radiation.
The recent
star
formation itself was likely triggered by
winds and supernova explosions, from previous generations of massive
stars, that swept up and compressed the molecular gas.
A false-color
Hubble palette was used to create the
this sharp close-up image
and shows emission from sulfur, hydrogen, and oxygen atoms
in red, green, and blue hues.
At the estimated distance of NGC 6188, the picture spans
about 200 light-years.
Andes Sunset Eclipse
Andes Sunset Eclipse
On July 11, after a long
trek eastward
across the southern Pacific Ocean, the Moon's shadow reached
landfall in South America.
In a
total solar eclipse
close to sunset,
silhouetted Moon and Sun hugged the western horizon,
seen here above the Andes mountains
near the continent's
southern tip.
To enjoy a
good
vantage point, the photographer hiked to
a windy spot about 400 meters above a lake, Lago Argentino,
climbing into the picture after setting up his camera on a tripod.
At left, the sky outside the shadow cone
is still bright.
Below, the lights of El Calafate, Patagonia, Argentina,
shine by the lake shore.
Easter Island Eclipse
Easter Island Eclipse
Makemake,
a god in Easter Island mythology, may have
smiled for a moment as
clouds parted long enough to reveal this glimpse of
July 11's total solar eclipse to skygazers.
In the foreground of
the dramatic scene,
the island's famous large,
monolithic statues (Moai)
share a beachside view of the shimmering
solar corona and the
darkened daytime sky.
Other opportunities to see the total phase of this
eclipse
of the Sun were also hard to come by.
Defined by the dark part of the
Moon's shadow, the
path of totality tracked
eastward across the
southern Pacific Ocean, only making significant landfall at
Mangaia (Cook Islands) and
Easter Island (Isla de Pascua),
ending shortly after reaching southern Chile and Argentina.
But a partial eclipse phase could be enjoyed over a broader region,
including many
southern Pacific islands and wide swath of South America.
Mosaic: Welcome to Planet Earth
Mosaic: Welcome to Planet Earth
Welcome to Planet
Earth, the third planet from a
star named the
Sun.
The Earth
is shaped like a sphere and
composed
mostly of rock.
Over 70 percent of the
Earth's surface is water.
The planet has a relatively thin
atmosphere composed mostly of
nitrogen and
oxygen.
This picture of Earth, dubbed
Blue Marble,
was taken from
Apollo 17
in 1972 and features Africa and Antarctica.
It is thought to be one of the most
widely distributed photographs
of any kind.
Here,
the world famous image has been recast as a spectacular
photomosaic
using
over
5,000 archived images of Earth and space.
With its abundance of liquid
water,
Earth
supports a large variety of
life forms,
including potentially intelligent species such as
dolphins and humans.
Please
enjoy your stay on Planet Earth.
Moons Beyond the Rings of Saturn
Moons Beyond the Rings of Saturn
What's happened to that moon of Saturn?
Nothing -- Saturn's moon Rhea is just partly hidden behind Saturn's rings.
In April, the robotic Cassini spacecraft now orbiting Saturn took this
narrow-angle view looking across the
Solar System's most
famous rings.
Rings visible in the foreground include the thin
F ring on the outside and the much wider
A and B rings just interior to it.
Although it seems to be hovering
over the rings, Saturn's moon
Janus is actually far behind them.
Janus is one of
Saturn's smaller
moons
and measures only about 180 kilometers across.
Farther out from the camera is the heavily cratered
Rhea, a much larger moon
measuring 1,500 kilometers across.
The top of Rhea is visible only through
gaps in the rings.
The Cassini mission around Saturn has
been extended to
2017
to better study the complex planetary system as its season changes from
equinox to
solstice.