_______________________________________________________________
Please vote for the TWO best Astronomy Pictures of the Day (image and text) of June 26-July 2, 2011.
(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 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.
An expansive nebula of dust is seen to surround red
supergiant star Betegeuse in this remarkable high resolution composite, an infrared
VLT image from the European Southern Observatory.
Betelgeuse itself is outlined by the small, central red circle. If found in our own solar system
its diameter would almost encompass the orbit of Jupiter. But the larger envelope of circumstellar dust extends some 60 billion kilometers into space, equivalent to about 400 times the Earth-Sun distance.
The dust is likely formed as the swollen atmosphere of the supergiant sheds material into space, a final phase in the evolution of
a massive star. Mixing with the
interstellar medium, the dust could ultimately form
rocky terrestrial planets like
Earth. The central bright portion of the outer image has been masked to reveal fainter extended structures. The field of view is 5.63
arcseconds across.
Why is this cluster of galaxies so jumbled? Far from a smooth distribution,
Abell 2744 not only has knots of galaxies, but the
X-ray emitting hot gas (colored red) in the cluster appears distributed differently than the
dark matter. The dark matter, taking up over 75 percent of the
cluster mass and colored blue in the
above image, was inferred by that needed to create the distortion of background galaxies by
gravitational lensing. The
jumble appears to result from the
slow motion collision of at least four smaller galaxy clusters over the past few billion years. The above
picture combines optical images from the
Hubble Space Telescope and the
Very Large Telescope with X-ray images from the
Chandra X-Ray Observatory.
Abell 2744, dubbed
Pandora's cluster, spans over two million light years and can best be seen with a really large telescope toward the constellation of the
Sculptor.
Sculpted by stellar winds and radiation, the star factory known as
Messier 17 lies some 5,500 light-years away in the nebula-rich constellation
Sagittarius. At that distance,
this degree wide field of view spans almost 100 light-years, courtesy of ESO's
new VLT Survey Telescope and OmegaCAM. The sharp, false color image includes both optical and infrared data, following faint details of the region's gas and dust clouds against a backdrop of central
Milky Way stars. Stellar winds and energetic light from hot, massive stars formed from M17's stock of cosmic gas and dust have slowly carved away at the remaining interstellar material producing the cavernous appearance and
undulating shapes.
M17 is also known as the
Omega Nebula or the Swan Nebula.
In the 1920s, examining photographic plates from the
Mt. Wilson Observatory's 100 inch telescope,
Edwin Hubble determined the distance to the
Andromeda Nebula, decisively demonstrating the existence of other galaxies far beyond the Milky Way. His notations are evident on the historic plate image inset at the lower right, shown in context with ground based and Hubble Space Telescope images of the region made
nearly 90 years later. By intercomparing different plates, Hubble searched for novae, stars which underwent a sudden increase in brightness. He found several on this plate and marked them with an "N". Later, discovering that the one near the upper right corner (marked by lines) was actually a type of
variable star known as
a cepheid, he crossed out the "N" and wrote "VAR!". Thanks to the work of Harvard astronomer
Henrietta Leavitt, cepheids, regularly varying pulsating stars, could be used as standard candle
distance indicators. Identifying such a star allowed Hubble to show that Andromeda was not a small cluster of stars and gas within our own galaxy, but a large galaxy in its own right at a substantial distance from the Milky Way.
Hubble's discovery is responsible for establishing our modern concept of a
Universe filled with galaxies.
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.
<- 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 June 26-July 2, 2011.
(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=24273][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]
[c][url=http://apod.nasa.gov/apod/ap110627.html][size=150][b]Stars and Dust Across Corona Australis (2011 June 27)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1106/ngc6727_julio_900.jpg[/img2][/float]Cosmic dust clouds sprawl across a rich field of stars in this sweeping telescopic vista near the northern boundary of [url=http://www.botproductions.com/stellar/corona_australis.html]Corona Australis[/url], the Southern Crown. Probably less than 500 light-years away and effectively [url=http://apod.nasa.gov/apod/ap090425.html]blocking light[/url] from more distant, background stars in the [url=http://members.nova.org/~sol/chview/chv5.htm]Milky Way[/url], the densest part of the dust cloud is about 8 light-years long. [url=http://apod.nasa.gov/apod/image/0407/ngc6726_wide_tanlbl1.jpg]At its tip[/url] (upper right) is a group of lovely reflection nebulae cataloged as [url=http://www.aao.gov.au/images/captions/aat073.html]NGC 6726, 6727, 6729[/url], and IC 4812. A characteristic blue color is produced as light from hot stars is [url=http://apod.nasa.gov/apod/ap011228.html]reflected by[/url] the cosmic dust. The smaller yellowish nebula (NGC 6729) surrounds [url=http://apod.nasa.gov/apod/ap031226.html]young[/url] variable star [url=http://www.solstation.com/stars/r-coraus.htm]R Coronae Australis[/url]. Magnificent [url=http://apod.nasa.gov/apod/ap040511.html]globular star cluster[/url] NGC 6723 is toward the upper right corner of the view. While [url=http://www.seds.org/~spider/spider/MWGC/n6723.html]NGC 6723 appears[/url] to be part of the group, it actually lies nearly 30,000 [url=http://en.wikipedia.org/wiki/Light_years]light-years[/url] away, far beyond the [url=http://www.youtube.com/watch?v=G3rCrczjtm0]Corona Australis dust clouds[/url].
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110628.html][size=150][b]Stardust and Betelgeuse (2011 June 28)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1106/BetelgeuseCircumstellar_eso900.jpg[/img2][/float][url=http://www.eso.org/public/news/eso1121/]An expansive nebula of dust[/url] is seen to surround red [url=http://apod.nasa.gov/apod/ap001222.html]supergiant[/url] star Betegeuse in this remarkable high resolution composite, an infrared [url=http://www.eso.org/public/teles-instr/vlt.html]VLT[/url] image from the European Southern Observatory. [url=http://apod.nasa.gov/apod/ap090805.html]Betelgeuse itself[/url] is outlined by the small, central red circle. If found in our own solar system [url=http://apod.nasa.gov/apod/ap100106.html]its diameter[/url] would almost encompass the orbit of Jupiter. But the larger envelope of circumstellar dust extends some 60 billion kilometers into space, equivalent to about 400 times the Earth-Sun distance. [url=http://arxiv.org/abs/1106.5041]The dust is[/url] likely formed as the swollen atmosphere of the supergiant sheds material into space, a final phase in the evolution of [url=http://hyperphysics.phy-astr.gsu.edu/hbase/astro/redsup.html#c1]a massive star[/url]. Mixing with the [url=http://espg.sr.unh.edu/ism/what1.html]interstellar medium[/url], the dust could ultimately form [url=http://apod.nasa.gov/apod/ap090923.html]rocky[/url] terrestrial planets like [url=http://arnett.us.com/psc/pbd.html]Earth[/url]. The central bright portion of the outer image has been masked to reveal fainter extended structures. The field of view is 5.63 [url=http://chandra.harvard.edu/photo/scale.html]arcseconds[/url] across.
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110629.html][size=150][b]Abell 2744: Pandora's Cluster of Galaxies (2011 June 29)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1106/abell2744_hst_900.jpg[/img2][/float]Why is this cluster of galaxies so jumbled? Far from a smooth distribution, [url=http://chandra.harvard.edu/photo/2011/a2744/]Abell 2744[/url] not only has knots of galaxies, but the [url=http://science.hq.nasa.gov/kids/imagers/ems/xrays.html]X-ray[/url] emitting hot gas (colored red) in the cluster appears distributed differently than the [url=http://en.wikipedia.org/wiki/Dark_matter]dark matter[/url]. The dark matter, taking up over 75 percent of the [url=http://en.wikipedia.org/wiki/Galaxy_groups_and_clusters]cluster[/url] mass and colored blue in the [url=http://hubblesite.org/newscenter/archive/releases/2011/17/image/a/]above image[/url], was inferred by that needed to create the distortion of background galaxies by [url=http://www.astrophysicsspectator.com/topics/generalrelativity/GravitationalLensPointSim.html]gravitational lensing[/url]. The [url=http://www.youtube.com/watch?v=qPE4ILbe4CM]jumble appears[/url] to result from the [url=http://www.youtube.com/watch?v=z6U_GFa76Ys]slow motion[/url] collision of at least four smaller galaxy clusters over the past few billion years. The above [url=http://imgsrc.hubblesite.org/hu/db/images/hs-2011-17-b-web_print.jpg]picture combines[/url] optical images from the [url=http://apod.nasa.gov/apod/ap010806.html]Hubble Space Telescope[/url] and the [url=http://apod.nasa.gov/apod/ap000707.html]Very Large Telescope[/url] with X-ray images from the [url=http://en.wikipedia.org/wiki/Chandra_X-ray_Observatory]Chandra[/url] X-Ray Observatory. [url=http://www.youtube.com/watch?v=WZ24B2qNhVQ]Abell 2744[/url], dubbed [url=http://en.wikipedia.org/wiki/Pandora%27s_box]Pandora[/url]'s cluster, spans over two million light years and can best be seen with a really large telescope toward the constellation of the [url=http://www.ianridpath.com/startales/sculptor.htm]Sculptor[/url].
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110630.html][size=150][b]Star Factory Messier 17 (2011 June 30)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1106/esoM17c900.jpg[/img2][/float][url=http://apod.nasa.gov/apod/ap030821.html]Sculpted by[/url] stellar winds and radiation, the star factory known as [url=http://seds.org/messier/m/m017.html]Messier 17[/url] lies some 5,500 light-years away in the nebula-rich constellation [url=http://www.hawastsoc.org/deepsky/sgr/index.html]Sagittarius[/url]. At that distance, [url=http://www.eso.org/public/images/eso1119a/]this degree wide field of view[/url] spans almost 100 light-years, courtesy of ESO's [url=http://www.eso.org/public/news/eso1119/]new VLT Survey Telescope and OmegaCAM[/url]. The sharp, false color image includes both optical and infrared data, following faint details of the region's gas and dust clouds against a backdrop of central [url=http://apod.nasa.gov/apod/ap110520.html]Milky Way[/url] stars. Stellar winds and energetic light from hot, massive stars formed from M17's stock of cosmic gas and dust have slowly carved away at the remaining interstellar material producing the cavernous appearance and [url=http://apod.nasa.gov/apod/ap040828.html]undulating[/url] shapes. [url=http://coolcosmos.ipac.caltech.edu/cosmic_classroom/multiwavelength_astronomy/multiwavelength_museum/m17.html]M17 is also[/url] known as the [url=http://apod.nasa.gov/apod/ap040208.html]Omega Nebula[/url] or the Swan Nebula.
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[c][url=http://apod.nasa.gov/apod/ap110701.html][size=150][b]VAR! (2011 July 01)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1107/varHubblepanel_hst800.jpg[/img2][/float]In the 1920s, examining photographic plates from the [url=http://www.mtwilson.edu/vir/100/]Mt. Wilson Observatory's[/url] 100 inch telescope, [url=http://www.spacetelescope.org/about/history/the_man_behind_the_name/]Edwin Hubble[/url] determined the distance to the [url=http://apod.nasa.gov/apod/ap100109.html]Andromeda Nebula[/url], decisively demonstrating the existence of other galaxies far beyond the Milky Way. His notations are evident on the historic plate image inset at the lower right, shown in context with ground based and Hubble Space Telescope images of the region made [url=http://hubblesite.org/newscenter/archive/releases/2011/15/]nearly 90 years later[/url]. By intercomparing different plates, Hubble searched for novae, stars which underwent a sudden increase in brightness. He found several on this plate and marked them with an "N". Later, discovering that the one near the upper right corner (marked by lines) was actually a type of [url=http://hubblesite.org/newscenter/archive/releases/2011/15/fastfacts/]variable star known[/url] as [url=http://apod.nasa.gov/apod/ap080212.html]a cepheid[/url], he crossed out the "N" and wrote "VAR!". Thanks to the work of Harvard astronomer [url=http://apod.nasa.gov/apod/ap000903.html]Henrietta Leavitt[/url], cepheids, regularly varying pulsating stars, could be used as standard candle [url=http://www.aavso.org/cosmic-distance-ladder]distance indicators[/url]. Identifying such a star allowed Hubble to show that Andromeda was not a small cluster of stars and gas within our own galaxy, but a large galaxy in its own right at a substantial distance from the Milky Way. [url=http://heritage.stsci.edu/2011/15/caption.html]Hubble's discovery[/url] is responsible for establishing our modern concept of a [url=http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1995PASP..107.1133T]Universe filled with galaxies[/url].
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[c][url=http://apod.nasa.gov/apod/ap110702.html][size=150][b]Moon and Venus at Dawn (2011 July 02)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1107/mv2011Jun30_tezel900c.jpg[/img2][/float]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 [url=http://www.twanight.org/newTWAN/index.asp]skyview[/url] overlooking a reservoir near Izmir, Turkey. [url=http://transit.savage-garden.org/en/occultations/?which=13&longitude=29.57143&latitude=36.85714&elevation=0&temperature=0&pressure=870&explain=on]For some[/url], the close conjunction could be viewed as a [url=http://apod.nasa.gov/apod/ap070620.html]daylight occultation[/url]. While Venus is nearing the end of its latest performance as planet Earth's [url=http://www.glyphweb.com/esky/planets/venus.html]morning star[/url], the old lunar cresent, about 24 hours from its New Moon phase, was also [url=http://www.poets.org/viewmedia.php/prmMID/5873]bidding farewell[/url] for now to the dawn. In fact, for the next two nights a [url=http://apod.nasa.gov/apod/ap050513.html]young Moon[/url] can be spotted just after sunset. [url=http://www.skyandtelescope.com/observing/ataglance]Look for[/url] a thin sunlit sliver close to the western horizon, not far from bright planet Mercury.
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[size=110][url=http://asterisk.apod.com/viewtopic.php?f=29&t=24273][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]