The APOD site, in addition to displaying excellent images, offers descriptions of the phenomena shown. You could look through the archive, or you could just look through this list of APOD material for the week of September 23, 2012.
Sunday, September 23
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Equinox: The Sun from Solstice to Solstice |
Explanation: Yesterday was
an equinox, a date when day and night are equal. Today, and every day until the
next equinox, the night will
be longer than the day in Earth's northern hemisphere, and the day will be
longer than the night in Earth's southern hemisphere. An equinox occurs midway
between the two solstices,
when the days and nights are the least equal. The picture is a composite of
hourly images taken of the Sun above Bursa, Turkey on key days from solstice
to equinox to
solstice. The bottom Sun band was taken during the winter solstice in 2007
December, when the Sun could not rise very high in the sky nor stay above the
horizon very long. This lack of Sun caused winter. The top Sun band was
taken during the summer
solstice in 2008 June, when the Sun rose highest in the sky and stayed above the horizon
for more than 12 hours. This abundance of Sun caused summer. The middle band was
taken during the Vernal
Equinox in 2008 March, but it is the same sun band that Earthlings saw yesterday,
the day of the Autumnal
Equinox.
Monday, September 24
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NGC 2736: The Pencil Nebula |
Image Credit: ESO
Explanation: This shock wave plows through
space at over 500,000 kilometers per hour. Moving toward to bottom of this beautifully detailed
color composite, the thin, braided filaments are actually long ripples in a
sheet of glowing gas seen almost edge on. Cataloged as NGC
2736, its narrow appearance
suggests its popular name, the
Pencil Nebula. About 5 light-years long and a mere 800 light-years away,
the Pencil Nebula is
only a small part of the Vela supernova
remnant. The Vela remnant
itself is around 100 light-years in diameter and is the expanding debris cloud of
a star that was seen to explode about 11,000 years ago. Initially, the shock wave was moving at
millions of kilometers per hour but has slowed
considerably, sweeping up surrounding interstellar gas.
Tuesday, September 24
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Unusual Spheres on Mars |
Explanation: Why are these
strange little spheres on Mars? The robotic rover Opportunity
chanced across these
unusually shaped beads earlier this month while exploring a place named Kirkwood near the
rim of Mars' Endeavor
Crater. The above
image taken by Opportunity's Microscopic
Imager shows that some ground near the rover is filled with these unusual
spheres, each spanning only about 3 millimeters. At first glance, the
sometimes-fractured balls appear similar to the small rocks dubbed blueberries seen by
Opportunity eight years ago, but these spheres are densely compacted and have
little iron content. Although it is thought that these
orbs formed naturally, which natural processes formed them remain unknown. Opportunity, an older
sibling to the recently deployed Curiosity rover, will
continue to study these spheres with the hope that they will provide a new clue
to the ancient history of the surface of the red planet.
Wednesday, September 26
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A Space Shuttle over Los Angeles |
Explanation: It's not every
day that a space shuttle lands at LAX. Although this was a first for the major
Los Angeles airport hub, it was a last for the space shuttle Endeavour, as it
completed its tour of California skies and landed, albeit atop a 747, for the last time.
During its last
flight the iconic shuttle and its chase planes were photographed near
several of California's own icons including the Golden
Gate Bridge
in San Francisco, the Hollywood
Sign, and the skyline of
Los Angeles. Previously, in May, the space shuttle Enterprise was captured passing behind
several of New York City's icons on its way to the Intrepid Sea, Air, & Space Museum.
Pictured above, the piggybacking
shuttle was snapped on
approach last week to LAX as
it crossed above and beyond a major Los Angeles street. Now retired, the space
shuttles are all museum pieces, with the above shuttle scheduled to be towed
along the streets of LA to the California
Science Center.
Thursday, September 27
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Stars and Dust across Corona Australis |
Image Credit & Copyright:
Marco Lorenzi (Glittering Lights)
Explanation: Cosmic dust
clouds sprawl across a rich field of stars in this
sweeping telescopic vista near the northern boundary of Corona
Australis, the Southern Crown. Probably less than 500 light-years away and
effectively blocking light
from more distant, background stars in the Milky Way, the
densest part of the dust cloud is about 8 light-years long. At its tip
(upper right) is a group of lovely reflection nebulae cataloged as NGC 6726, 6727, 6729,
and IC 4812. A characteristic blue color is produced as light from hot stars is
reflected by the cosmic
dust. The smaller yellowish nebula (NGC 6729) surrounds young variable star R Coronae Australis.
Magnificent globular star
cluster NGC 6723 is toward the upper right corner of the view. While NGC 6723 appears to
be part of the group, it actually lies nearly 30,000 light-years
away, far beyond the Corona
Australis dust clouds.
Friday, September 28
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Stars in a Dusty Sky |
Explanation: Bright star Markab
anchors this dusty skyscape. At the top right corner of the frame, Markab
itself marks a corner of an asterism known as the
Great Square, found within the boundaries of the constellation Pegasus, the flying horse.
The wide and deep telescopic view rides along for some 5 degrees or about 10
times the angular diameter
of the Full Moon, with blue
reflection nebulae scattered around the scene. And even though this line-of-sight looks
away from the plane of our Milky Way galaxy, it covers a region known to be
filled with nearby molecular clouds. The associated dust clouds, high latitude galactic
cirrus, are less than 1,000 light-years distant. Still apparent, but far
beyond the Milky Way, are background galaxies, like the prominent edge-on spiral NGC 7497 near
picture center.
Saturday, September 29
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NGC 7023: The Iris Nebula |
Image Credit & Copyright:
Tony Hallas
Explanation: Like delicate
cosmic petals, these clouds of interstellar dust and gas have blossomed 1,300
light-years away in the fertile star fields of the constellation Cepheus.
Sometimes called the Iris Nebula and dutifully cataloged as NGC 7023 this is
not the only nebula in the sky to evoke the imagery of flowers. Still, this remarkable image shows off the
Iris Nebula's range of colors and symmetries in impressive detail. Within the Iris,
dusty nebular material surrounds a hot, young star. The dominant color of the
brighter reflection nebula is blue, characteristic of dust grains
reflecting starlight. Central
filaments of the dusty clouds glow with a faint reddish photoluminesence as
some dust grains effectively
convert the star's invisible ultraviolet radiation to
visible red light. Infrared observations
indicate that this nebula may contain complex carbon molecules known as PAHs.
The bright blue portion of the Iris Nebula is about six light-years across.
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