_______________________________________________________________
Please vote for the TWO best Astronomy Pictures of the Day (image and text) of January 15-21, 2012.
(Repeated APODs are not included in the poll.)
All titles are clickable and link to the original APOD page.
We ask for your help in choosing an APOW as this helps Jerry and Robert create "
year in APOD images" review lectures, create APOM and
APOY polls that can be used to create a free PDF calendar at year's end, and provides feedback on which images and APODs were relatively well received. You can select two top images for the week.
We are very interested in why you selected the APODs you voted for, and enthusiastically welcome your telling us why by responding to this thread.
Thank you!
_______________________________________________________________
<- Previous week's poll
Cosmic dust clouds ripple across
this infrared portrait of our Milky Way's
satellite galaxy, the Large Magellanic Cloud. In fact, the remarkable composite image from the
Herschel Space Observatory and the
Spitzer Space Telescope show that dust clouds fill this neighboring dwarf galaxy, much like
dust along the plane of the Milky Way itself. The dust
temperatures tend to trace star forming activity. Spitzer data in blue hues indicate warm dust heated by young stars. Herschel's instruments contributed the image data shown in red and green, revealing dust emission from cooler and intermediate regions where star formation is just beginning or has stopped. Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from
views in optical images. But this galaxy's well-known
Tarantula Nebula still stands out, easily seen here as the brightest region to the left of center. A mere 160,000 light-years distant,
the Large Cloud of Magellan is about 30,000 light-years across.
Click to play embedded YouTube video.
Image Credit & Copyright: Nilesh Vayada & Ajay Talwar (TWAN)
Is it dawn or false dawn? During certain times of the year, the horizon near the
rising Sun will begin to glow unusually early. This early glow does not originate directly from the Sun, but rather from sunlight reflected by
interplanetary dust. Called
zodiacal light, the
glowing triangle of light may be mistaken, for a while, for a sunrise, and so may be called a false dawn.
Pictured above, two false dawns were recorded in time lapse movies each spanning about five hours from the perch of the
highest observatory in the world:
Mount Saraswati near
Hanle,
India. At its brightest, the rising
zodiacal triangle on the left glows brighter than even the central disk of our Milky Way Galaxy --
visible as the diagonal
band moving left to right across the frame.
Double, double toil and trouble; Fire burn, and cauldron bubble -- maybe
Macbeth should have
consulted the Witch Head Nebula. This suggestively shaped
reflection nebula is associated with the
bright star Rigel in the
constellation Orion. More formally known as
IC 2118, the Witch Head Nebula glows primarily by
light reflected from bright star
Rigel, located just below the lower edge of the
above image. Fine
dust in the nebula reflects the light. The blue color is caused not only by
Rigel's blue color but because the
dust grains reflect blue light more efficiently than red. The same
physical process causes
Earth's daytime sky to appear blue, although the scatterers in
Earth's atmosphere are molecules of
nitrogen and
oxygen. The nebula lies about 1000
light-years away.
How do stars form? To help study this complex issue, astronomers took a deep
infrared image of
Cygnus X, the largest known star forming region in the entire
Milky Way Galaxy. The
above recently-released image was taken in 2009 by the orbiting
Spitzer Space Telescope and digitally translated into
colors humans can see, with the hottest regions colored the most blue.
Visible are large bubbles of hot gas inflated by the
winds of massive stars soon after they form. Current models posit that these expanding
bubbles sweep up gas and sometimes even collide, frequently creating regions dense enough to gravitationally collapse into yet more stars. The star factory
Cygnus-X spans over 600 light years, contains over a million times the mass of our Sun, and
shines prominently on wide angle
infrared panoramas of the night sky.
Cygnus X lies 4,500 light years away towards the
constellation of the Swan (Cygnus). In a few million years,
calm will likely be restored and a large
open cluster of stars will remain -- which itself will disperse over the next 100 million years.
Begirt with many a blazing star,
Orion, the Hunter, is one of the most easily recognizable
constellations. In this
night skyscape from January 15, the hunter's stars rise in the northern hemisphere's winter sky, framed by bare trees and bounded below by terrestrial lights around Lough Eske (Lake of Fish) in County Donegal, Ireland.
Red giant star Betelgeuse is striking in yellowish hues at Orion's shoulder above and left of center. Rivaling the bright red giant,
Rigel, a blue supergiant star holds the opposing position near Orion's foot.
Of course, the sword of Orion hangs from the hunter's three belt stars near picture center, but the middle star in the sword is not a star at all. A slightly fuzzy pinkish glow hints at its true nature, a nearby stellar nursery visible to the unaided eye known as
the Orion Nebula.
A Full Moon
rising can be a
dramatic celestial
sight, and Full Moons can have many names. Captured on January 8 from Ötersund, Sweden, this
evocative moonrise portrait might make you feel the cold of winter in the north. If you can also imagine wolves howling in the distance then you probably understand why Native Americans would have called it the Wolf Moon, their
traditional name for the first Full Moon in January. The photographer reports that no wolves were heard though, as he watched this beautiful Full Moon rise in fading light over the eastern horizon,
echoing the yellow color of the
setting Sun. Of course, due this year on February 7, the next Full Moon will be the
Snow Moon.
From solstice to solstice, this six month long exposure
compresses time from the 21st of June till the 21st of December, 2011, into a single point of view.
Dubbed a solargraph, the unconventional picture was recorded with
a pinhole camera made from a drink can lined with a piece of photographic paper. Fixed to
a single spot for the entire exposure, the simple camera continuously records the Sun's path each day as a glowing trail burned into the photosensitive paper. In this case, the spot was chosen to look out over the domes and radio telescope of the University of Hertfordshire's
Bayfordbury Observatory. Dark gaps in the daily arcs are caused by cloud cover, whereas continuous bright tracks record glorious spells of sunny weather. Of course, in June, the Sun trails begin higher at the northern hemisphere's
summer solstice. The trails sink lower in the sky as December's
winter solstice approaches. Last year's autumn was one of the balmiest on record in the UK, as the many bright arcs in the lower part of this picture testify.
<- Previous week's poll
[size=200][color=#FF0000]_______________________________________________________________[/color][/size]
Please vote for the TWO best Astronomy Pictures of the Day (image and text) of January 15-21, 2012.
(Repeated APODs are not included in the poll.)
All titles are clickable and link to the original APOD page.
We ask for your help in choosing an APOW as this helps Jerry and Robert create "[url=http://www.youtube.com/watch?v=NAQXYYbBa1s]year in APOD images[/url]" review lectures, create APOM and [url=http://asterisk.apod.com/viewtopic.php?f=29&t=22695&p=141942#p141942]APOY polls[/url] that can be used to create a free PDF calendar at year's end, and provides feedback on which images and APODs were relatively well received. You can select two top images for the week.
We are very interested in why you selected the APODs you voted for, and enthusiastically welcome your telling us why by responding to this thread.
Thank you!
[size=200][color=#FF0000]_______________________________________________________________[/color][/size]
[size=110][url=http://asterisk.apod.com/viewtopic.php?f=29&t=26741][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]
[hr][/hr]
[c][url=http://apod.nasa.gov/apod/ap120115.html][size=150][b]Infrared Portrait of the Large Magellanic Cloud (2012 Jan 15)[/b][/size][/url][/c]
[float=left][img6="Credit: ESA / NASA / JPL-Caltech / STScI"]http://apod.nasa.gov/apod/image/1201/PIA15254_LMC900c.jpg[/img6][hr][/hr][/float]Cosmic dust clouds ripple across [url=http://www.spitzer.caltech.edu/images/4872-ssc2012-01a-Dusty-Space-Cloud]this infrared portrait[/url] of our Milky Way's [url=http://www.atlasoftheuniverse.com/sattelit.html]satellite galaxy[/url], the Large Magellanic Cloud. In fact, the remarkable composite image from the [url=http://herschel.esac.esa.int/overview.shtml]Herschel Space Observatory[/url] and the [url=http://www.spitzer.caltech.edu/mission]Spitzer Space Telescope[/url] show that dust clouds fill this neighboring dwarf galaxy, much like [url=http://apod.nasa.gov/apod/ap110902.html]dust along the plane[/url] of the Milky Way itself. The dust [url=http://coolcosmos.ipac.caltech.edu/cosmic_classroom/ir_tutorial/index.html]temperatures[/url] tend to trace star forming activity. Spitzer data in blue hues indicate warm dust heated by young stars. Herschel's instruments contributed the image data shown in red and green, revealing dust emission from cooler and intermediate regions where star formation is just beginning or has stopped. Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from [url=http://apod.nasa.gov/apod/ap110426.html]views in optical images[/url]. But this galaxy's well-known [url=http://apod.nasa.gov/apod/ap110111.html]Tarantula Nebula[/url] still stands out, easily seen here as the brightest region to the left of center. A mere 160,000 light-years distant, [url=http://apod.nasa.gov/apod/ap081219.html]the Large Cloud of Magellan[/url] is about 30,000 light-years across.
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[c][url=http://apod.nasa.gov/apod/ap120116.html][size=150][b]Zodiacal Light and the False Dawn (2012 Jan 16)[/b][/size][/url][/c]
[float=left][youtube6]http://www.youtube.com/watch?v=TLJiXAnHkGg[/youtube6]
[size=85]Image Credit & Copyright: Nilesh Vayada & Ajay Talwar (TWAN)[/size][hr][/hr][/float]Is it dawn or false dawn? During certain times of the year, the horizon near the [url=http://apod.nasa.gov/apod/ap111010.html]rising Sun[/url] will begin to glow unusually early. This early glow does not originate directly from the Sun, but rather from sunlight reflected by [url=http://apod.nasa.gov/apod/ap010813.html]interplanetary dust[/url]. Called [url=http://en.wikipedia.org/wiki/Zodiacal_light]zodiacal light[/url], the [url=http://apod.nasa.gov/apod/ap070925.html]glowing triangle[/url] of light may be mistaken, for a while, for a sunrise, and so may be called a false dawn. [url=http://www.youtube.com/watch?v=TLJiXAnHkGg]Pictured above[/url], two false dawns were recorded in time lapse movies each spanning about five hours from the perch of the [url=http://en.wikipedia.org/wiki/Indian_Astronomical_Observatory]highest observatory[/url] in the world: [url=http://www.webcamgalore.com/EN/webcam/India/Mount-Saraswati/1904.html]Mount Saraswati[/url] near [url=http://en.wikipedia.org/wiki/Hanle_(village)]Hanle[/url], [url=http://en.wikipedia.org/wiki/India]India[/url]. At its brightest, the rising [url=http://apod.nasa.gov/apod/ap100913.html]zodiacal triangle[/url] on the left glows brighter than even the central disk of our Milky Way Galaxy -- [url=http://apod.nasa.gov/apod/ap110730.html]visible[/url] as the diagonal [url=http://apod.nasa.gov/apod/ap110710.html]band[/url] moving left to right across the frame.
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[c][url=http://apod.nasa.gov/apod/ap120117.html][size=150][b]IC 2118: The Witch Head Nebula (2012Jan 17)[/b][/size][/url][/c]
[float=left][img6="Image Credit & Copyright: Gimmi Ratto & Davide Bardini (Collecting Photons)"]http://apod.nasa.gov/apod/image/1201/witch_ratto_900.jpg[/img6][hr][/hr][/float]Double, double toil and trouble; Fire burn, and cauldron bubble -- maybe [url=http://the-tech.mit.edu/Shakespeare/macbeth/]Macbeth[/url] should have [url=http://astrosphere.org/Surveys/APOD/survey_APOD.php]consulted[/url] the Witch Head Nebula. This suggestively shaped [url=http://apod.nasa.gov/apod/reflection_nebulae.html]reflection nebula[/url] is associated with the [url=http://www.astro.uiuc.edu/~kaler/sow/rigel.html]bright star Rigel[/url] in the [url=http://www.astro.uiuc.edu/~kaler/sow/orion-p.html]constellation Orion[/url]. More formally known as [url=http://en.wikipedia.org/wiki/IC_2118]IC 2118[/url], the Witch Head Nebula glows primarily by [url=http://apod.nasa.gov/apod/ap091229.html]light reflected[/url] from bright star [url=http://adsabs.harvard.edu/abs/1997MNRAS.290..521I]Rigel[/url], located just below the lower edge of the [url=http://www.collectingphotons.com/Astro/Nebulae/ERI_WH_ASA_1600.jpg]above image[/url]. Fine [url=http://apod.nasa.gov/apod/ap030706.html]dust[/url] in the nebula reflects the light. The blue color is caused not only by [url=http://en.wikipedia.org/wiki/Rigel]Rigel[/url]'s blue color but because the [url=http://leo.astronomy.cz/mix/mix.html]dust grains reflect blue light[/url] more efficiently than red. The same [url=http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html]physical process[/url] causes [url=http://math.ucr.edu/home/baez/physics/General/BlueSky/blue_sky.html]Earth's daytime sky to appear blue[/url], although the scatterers in [url=http://csep10.phys.utk.edu/astr161/lect/earth/atmosphere.html]Earth's atmosphere[/url] are molecules of [url=http://periodic.lanl.gov/7.html]nitrogen[/url] and [url=http://periodic.lanl.gov/8.html]oxygen[/url]. The nebula lies about 1000 [url=http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html]light-years[/url] away.
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[c][url=http://apod.nasa.gov/apod/ap120118.html][size=150][b]Cygnus-X: The Inner Workings of a Nearby Star Factory (2012 Jan 18)[/b][/size][/url][/c]
[float=left][img6="Image Credit: NASA/JPL-Caltech/Harvard-Smithsonian CfA"]http://apod.nasa.gov/apod/image/1201/cygnusx_spitzer_900.jpg[/img6][hr][/hr][/float]How do stars form? To help study this complex issue, astronomers took a deep [url=http://missionscience.nasa.gov/ems/07_infraredwaves.html]infrared[/url] image of [url=http://www.cfa.harvard.edu/cygnusX/abst.html]Cygnus X[/url], the largest known star forming region in the entire [url=http://apod.nasa.gov/apod/ap110118.html]Milky Way Galaxy[/url]. The [url=http://www.spitzer.caltech.edu/images/4868-ssc2012-02a-Stars-Brewing-in-Cygnus-X]above recently-released image[/url] was taken in 2009 by the orbiting [url=http://www.spitzer.caltech.edu/mission/32-The-Mission]Spitzer Space Telescope[/url] and digitally translated into [url=http://www.colorpicker.com/]colors[/url] humans can see, with the hottest regions colored the most blue. [url=http://www.cfa.harvard.edu/cygnusX/2012_AustinAASposter.pdf]Visible[/url] are large bubbles of hot gas inflated by the [url=http://apod.nasa.gov/apod/ap000318.html]winds[/url] of massive stars soon after they form. Current models posit that these expanding [url=http://apod.nasa.gov/apod/ap070714.html]bubble[/url]s sweep up gas and sometimes even collide, frequently creating regions dense enough to gravitationally collapse into yet more stars. The star factory [url=http://www.nasa.gov/mission_pages/spitzer/multimedia/pia15253.html]Cygnus-X[/url] spans over 600 light years, contains over a million times the mass of our Sun, and [url=http://www.cfa.harvard.edu/cygnusX/DIRBE_140um.jpg]shines prominently[/url] on wide angle [url=http://apod.nasa.gov/apod/ap000517.html]infrared panoramas[/url] of the night sky. [url=http://www.cfa.harvard.edu/cygnusX/whatis.html]Cygnus X[/url] lies 4,500 light years away towards the [url=http://en.wikipedia.org/wiki/Cygnus_%28constellation%29]constellation of the Swan[/url] (Cygnus). In a few million years, [url=http://eatgoodlivegoodfeelgood.files.wordpress.com/2012/01/relaxed.jpg]calm[/url] will likely be restored and a large [url=http://asterisk.apod.com/viewtopic.php?f=24&t=18009]open cluster[/url] of stars will remain -- which itself will disperse over the next 100 million years.
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[c][url=http://apod.nasa.gov/apod/ap120119.html][size=150][b]The Hunter's Stars (2012 Jan 19)[/b][/size][/url][/c]
[float=left][img6="Image Credit & Copyright: Brendan Alexander (Donegal Skies)"]http://apod.nasa.gov/apod/image/1201/LoughEske2_alexander900.jpg[/img6][hr][/hr][/float]Begirt with many a blazing star, [url=http://www.clarkfoundation.org/astro-utah/vondel/slimone.html]Orion, the Hunter[/url], is one of the most easily recognizable [url=http://www.astro.wisc.edu/~dolan/constellations/extra/constellations.html]constellations[/url]. In this [url=http://www.hwlongfellow.org/poems_poem.php?pid=106]night skyscape[/url] from January 15, the hunter's stars rise in the northern hemisphere's winter sky, framed by bare trees and bounded below by terrestrial lights around Lough Eske (Lake of Fish) in County Donegal, Ireland. [url=http://apod.nasa.gov/apod/ap100106.html]Red giant star Betelgeuse[/url] is striking in yellowish hues at Orion's shoulder above and left of center. Rivaling the bright red giant, [url=http://stars.astro.illinois.edu/sow/rigel.html]Rigel, a blue supergiant[/url] star holds the opposing position near Orion's foot. [url=http://www.gb.nrao.edu/~rmaddale/Education/OrionTourCenter/optical.html]Of course, the sword[/url] of Orion hangs from the hunter's three belt stars near picture center, but the middle star in the sword is not a star at all. A slightly fuzzy pinkish glow hints at its true nature, a nearby stellar nursery visible to the unaided eye known as [url=http://apod.nasa.gov/apod/ap110913.html]the Orion Nebula[/url].
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[c][url=http://apod.nasa.gov/apod/ap120120.html][size=150][b]The Wolf's Moon (2012 Jan 20)[/b][/size][/url][/c]
[float=left][img6="Image Credit & Copyright: Göran Strand"]http://apod.nasa.gov/apod/image/1201/GS_20120108_Moon_0010_900.jpg[/img6][hr][/hr][/float]A Full Moon [url=http://apod.nasa.gov/apod/ap110320.html]rising[/url] can be a [url=http://apod.nasa.gov/apod/ap070926.html]dramatic[/url] celestial [url=http://apod.nasa.gov/apod/ap031011.html]sight[/url], and Full Moons can have many names. Captured on January 8 from Ötersund, Sweden, this [url=http://home.hiwaay.net/~krcool/Astro/moon/moonwords/moonpoems.htm]evocative[/url] moonrise portrait might make you feel the cold of winter in the north. If you can also imagine wolves howling in the distance then you probably understand why Native Americans would have called it the Wolf Moon, their [url=http://www.msnbc.msn.com/id/45911225/ns/%20technology_and_science-space/t/how-s-full-moons-got-their-strange-names/]traditional name for[/url] the first Full Moon in January. The photographer reports that no wolves were heard though, as he watched this beautiful Full Moon rise in fading light over the eastern horizon, [url=http://apod.nasa.gov/apod/ap050127.html]echoing[/url] the yellow color of the [url=http://apod.nasa.gov/apod/ap081122.html]setting Sun[/url]. Of course, due this year on February 7, the next Full Moon will be the [url=http://apod.nasa.gov/apod/ap110228.html]Snow Moon[/url].
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[c][url=http://apod.nasa.gov/apod/ap120121.html][size=150][b]Days in the Sun (2012 Jan 21)[/b][/size][/url][/c]
[float=left][img6="Image Credit & Copyright: Regina Valkenborgh"]http://apod.nasa.gov/apod/image/1201/Bayfordbury_Solargraph900.jpg[/img6][hr][/hr][/float]From solstice to solstice, this six month long exposure [url=http://www.moma.org/collection/browse_results.php?object_id=79018]compresses time[/url] from the 21st of June till the 21st of December, 2011, into a single point of view. [url=http://www.solargraphy.com/index.php?option=com_content&task=view&id=4&Itemid=5]Dubbed a solargraph[/url], the unconventional picture was recorded with [url=http://www.pinholephotography.org/Solargraph%20instructions%202.htm]a pinhole camera made from[/url] a drink can lined with a piece of photographic paper. Fixed to [url=http://extragalactic.info/Bayfordbury/bfbphotos/img/camerainsitue.JPG]a single spot[/url] for the entire exposure, the simple camera continuously records the Sun's path each day as a glowing trail burned into the photosensitive paper. In this case, the spot was chosen to look out over the domes and radio telescope of the University of Hertfordshire's [url=http://extragalactic.info/Bayfordbury/main.php]Bayfordbury Observatory[/url]. Dark gaps in the daily arcs are caused by cloud cover, whereas continuous bright tracks record glorious spells of sunny weather. Of course, in June, the Sun trails begin higher at the northern hemisphere's [url=http://apod.nasa.gov/apod/ap100621.html]summer solstice[/url]. The trails sink lower in the sky as December's [url=http://apod.nasa.gov/apod/ap071222.html]winter solstice[/url] approaches. Last year's autumn was one of the balmiest on record in the UK, as the many bright arcs in the lower part of this picture testify.
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[size=110][url=http://asterisk.apod.com/viewtopic.php?f=29&t=26741][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]