_______________________________________________________________
Please vote for the TWO best Astronomy Pictures of the Day (image and text) of May 22-28, 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
Why does the Crab Nebula flare? No one is sure. The unusual behavior,
discovered over the
past few years, seems only to
occur in very high energy light --
gamma rays. As recently as one month ago, gamma-ray observations of the
Crab Nebula by the
Fermi Gamma Ray Space Telescope showed an
unexpected increase in gamma-ray brightness,
becoming about five times the nebula's usual gamma-ray brightness, and
fading again in only a few days. Now usually the faster the variability, the smaller the region involved. This might indicate that the powerful pulsar at the
center of the Crab, a compact
neutron star rotating 30 times a second, is somehow involved. Specifically,
speculation is centered on the changing
magnetic field that surely surrounds the powerful
pulsar. Rapid changes in this field might lead to waves of rapidly accelerated electrons which emit
the flares, possibly in
ways similar to our
Sun. The
above image shows how the Crab Nebula normally
appears in gamma rays, as compared to the
Geminga pulsar, and how it then appeared during the recent brightening.
How many arches can you count in the above image? If you count both spans of the
Double Arch in the
Arches National Park in
Utah,
USA, then two. But since the
above image was taken during a clear dark night, it caught a photogenic third arch far in the distance -- that of the overreaching
Milky Way Galaxy. Because we are situated in the midst of the
spiral Milky Way Galaxy, the band of the
central disk appears all around us. The
sandstone arches of the
Double Arch were formed from the erosion of falling water. The larger arch rises over 30 meters above the
surrounding salt bed and spans close to 50 meters across. The
dark silhouettes across the image bottom are sandstone monoliths left over from silt-filled crevices in an evaporated 300 million year old salty sea. A dim flow created by light pollution from
Moab, Utah can also be seen in the distance.
What's that rising from the clouds? The space shuttle. If you looked out the window of an airplane at just the right place and time last week, you could have seen something very unusual -- the space shuttle Endeavour launching to orbit.
Images of the rising shuttle and its plume became widely circulated over the web shortly after
Endeavour's final launch. The
above image was taken from a shuttle training aircraft and is not
copyrighted. Taken well above the clouds, the image can be matched with similar images of the same shuttle plume taken
below the clouds. Hot glowing gasses expelled by the engines are visible near the
rising shuttle, as well as a long smoke plume. A
shadow of the plume appears on the cloud deck, indicating the direction of the Sun. The shuttle
Endeavour remains docked with the
International Space Station and is currently scheduled to return to Earth next week.
To create a sonata from supernovae, first you have to
find the supernovae. To do that composers Alex Parker and Melissa Graham relied on the
Canada France Hawaii Telescope (CFHT) Legacy Survey data of four deep fields on the sky monitored from April 2003 through August 2006, adopting 241 Type Ia supernovae.
Enchanting to
cosmologists,
Type Ia supernovae are thermonuclear explosions that destroy white dwarf stars. Then, they gave each supernova a note to play, the volume of the note determined by the distance to the supernova. Fainter, more distant supernovae play quieter notes.
Each note's pitch was based on a
stretch factor measured by how fast the supernova brightens and fades over time relative to an adopted standard time history. Higher stretch factors play higher notes in pitches drawn from the illustrated
Phrygian dominant scale. Of course, each supernova note is played on an instrument. Supernovae in massive galaxies were assigned to a stand-up bass, while supernovae in less massive galaxies played their note on a grand piano. Click on the image or follow these links (
Vimeo,
YouTube) to watch a time compressed animation of the CFHT Legacy Survey data while
listening to the Supernova Sonata.
In this action scene, red night vision lights, green laser pointers, tripods and telescopes in faint silhouette surround intrepid sky gazers embarked on the 10th annual Iran
Messier Marathon. Completing the marathon requires viewing all 110 objects in 18th century French astronomer
Charles Messier's catalog in one glorious dusk-to-dawn observing run. As daunting as it sounds, there are often favorable weekend dates for northern hemisphere marathoners to complete the task that fall on nearly moonless nights near the spring equinox. With the Milky Way as a backdrop, this
group of about 150 astronomy enthusiasts conducted their 2011 marathon on
such a night in April from the desert area of
Seh Qaleh, in eastern Iran. Placing your cursor over the image will map the stunning night sky above their remote and very dark observing site. Follow the green laser pointer toward the Messier catalog objects (for example,
M8) near the galactic center. Astronomer and former Messier Marathon organizer Babak Tafreshi also composed
Sky Gazers, a time-lapse movie of this year's event.
If you're driving down a dark road on a starry night, you might want to check the odometer. Earlier this month, when traveling astronomer Dennis Mammana did he was greeted with the significant mileage reading of 186,282 miles. That's the number of miles
light travels in one second. Or, if you prefer kilometers, the number you are looking for is 299,792. Mammana muses that in driving to countless
observatories,
star parties, and
night sky photo shoots it has taken his 1998 vintage sport utility vehicle over 13 years to cover that distance. Of course, he considers his next important mileage milestone to be the distance
to the Moon.
<- 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 May 22-28, 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=23735][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]
[c][url=http://apod.nasa.gov/apod/ap110523.html][size=150][b]An Unexpected Flare from the Crab Nebula (2011 May 23)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1105/crabflare_fermi_900.jpg[/img2][/float]Why does the Crab Nebula flare? No one is sure. The unusual behavior, [url=http://www.astronomerstelegram.org/?read=2855]discovered[/url] over the [url=http://adsabs.harvard.edu/abs/2011Sci...331..739A]past[/url] few years, seems only to [url=http://adsabs.harvard.edu/abs/2010ATel.2861....1B]occur[/url] in very high energy light -- [url=http://en.wikipedia.org/wiki/Gamma_ray]gamma rays[/url]. As recently as one month ago, gamma-ray observations of the [url=http://apod.nasa.gov/apod/ap091025.html]Crab Nebula[/url] by the [url=http://en.wikipedia.org/wiki/Fermi_Space_Telescope]Fermi Gamma Ray Space Telescope[/url] showed an [url=http://www.nasa.gov/mission_pages/GLAST/news/crab-nebula-surprise.html]unexpected increase[/url] in gamma-ray brightness, [url=http://heasarc.gsfc.nasa.gov/docs/objects/heapow/archive/transients/crabflare_fermi.html]becoming about[/url] five times the nebula's usual gamma-ray brightness, and [url=http://www.nasa.gov/home/hqnews/2011/may/HQ_11-146_Crab_Nebula_Flare.html]fading again[/url] in only a few days. Now usually the faster the variability, the smaller the region involved. This might indicate that the powerful pulsar at the [url=http://www.youtube.com/watch?v=FYEprFXTdDQ]center of the Crab[/url], a compact [url=http://en.wikipedia.org/wiki/Neutron_star]neutron star[/url] rotating 30 times a second, is somehow involved. Specifically, [url=http://asterisk.apod.com/viewtopic.php?f=31&t=21399]speculation[/url] is centered on the changing [url=http://www.youtube.com/watch?v=fxC-AEC0ROk]magnetic field[/url] that surely surrounds the powerful [url=http://www.youtube.com/watch?v=duh2srW8j3U]pulsar[/url]. Rapid changes in this field might lead to waves of rapidly accelerated electrons which emit [url=http://www.youtube.com/watch?v=JsOqBxyHsYs]the flares[/url], possibly in [url=http://apod.nasa.gov/apod/ap031029.html]ways[/url] similar to our [url=http://apod.nasa.gov/apod/ap110307.html]Sun[/url]. The [url=http://www.nasa.gov/mission_pages/GLAST/news/crab-flare.html]above image[/url] shows how the Crab Nebula normally [url=http://apod.nasa.gov/apod/ap950624.html]appears[/url] in gamma rays, as compared to the [url=http://en.wikipedia.org/wiki/Geminga]Geminga[/url] pulsar, and how it then appeared during the recent brightening.
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110524.html][size=150][b]Three Arches Above Utah (2011 May 24)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1105/doublearch_goldpaint_900.jpg[/img2][/float]How many arches can you count in the above image? If you count both spans of the [url=http://www.360cities.net/image/inside-double-arch]Double Arch[/url] in the [url=http://en.wikipedia.org/wiki/Arches_National_Park]Arches National Park[/url] in [url=http://en.wikipedia.org/wiki/Utah]Utah[/url], [url=http://en.wikipedia.org/wiki/United_States]USA[/url], then two. But since the [url=http://www.flickr.com/photos/goldpaint/5707263924/in/set-72157622614976024/]above image[/url] was taken during a clear dark night, it caught a photogenic third arch far in the distance -- that of the overreaching [url=http://apod.nasa.gov/apod/ap080713.html]Milky Way Galaxy[/url]. Because we are situated in the midst of the [url=http://www.windows2universe.org/the_universe/Spirals.html]spiral[/url] Milky Way Galaxy, the band of the [url=http://apod.nasa.gov/apod/ap070930.html]central disk[/url] appears all around us. The [url=http://www.youtube.com/watch?v=YB_p3jjER6c]sandstone arches[/url] of the [url=http://en.wikipedia.org/wiki/Double_Arch]Double Arch were[/url] formed from the erosion of falling water. The larger arch rises over 30 meters above the [url=http://en.wikipedia.org/wiki/Paradox_Basin]surrounding salt bed[/url] and spans close to 50 meters across. The [url=http://apod.nasa.gov/apod/ap090516.html]dark silhouettes[/url] across the image bottom are sandstone monoliths left over from silt-filled crevices in an evaporated 300 million year old salty sea. A dim flow created by light pollution from [url=http://en.wikipedia.org/wiki/Moab,_Utah]Moab, Utah[/url] can also be seen in the distance.
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110525.html][size=150][b]Space Shuttle Rising (2011 May 25)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1105/shuttleplume_sts134_900.jpg[/img2][/float]What's that rising from the clouds? The space shuttle. If you looked out the window of an airplane at just the right place and time last week, you could have seen something very unusual -- the space shuttle Endeavour launching to orbit. [url=http://twitpic.com/4yg4ur]Images[/url] of the rising shuttle and its plume became widely circulated over the web shortly after [url=http://apod.nasa.gov/apod/ap110518.html]Endeavour's final launch[/url]. The [url=http://spaceflight.nasa.gov/gallery/images/shuttle/sts-134/html/sts134-s-061.html]above image[/url] was taken from a shuttle training aircraft and is not [url=http://redtape.msnbc.msn.com/_news/2011/05/23/6703177-that-famous-space-shuttle-photo-when-is-sharing-stealing]copyrighted[/url]. Taken well above the clouds, the image can be matched with similar images of the same shuttle plume taken [url=http://spaceflight.nasa.gov/gallery/images/shuttle/sts-134/html/sts134-s-013.html]below the clouds[/url]. Hot glowing gasses expelled by the engines are visible near the [url=http://www.youtube.com/watch?v=X47raRdRSBA]rising shuttle[/url], as well as a long smoke plume. A [url=http://apod.nasa.gov/apod/ap070603.html]shadow of the plume[/url] appears on the cloud deck, indicating the direction of the Sun. The shuttle [url=http://en.wikipedia.org/wiki/STS-134]Endeavour remains docked[/url] with the [url=http://www.nasa.gov/mission_pages/station/main/index.html]International Space Station[/url] and is currently scheduled to return to Earth next week.
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110526.html][size=150][b]Supernova Sonata (2011 May 26)[/b][/size][/url][/c]
[float=left][url=http://www.astro.uvic.ca/~alexhp/new/supernova_sonata.html][img]http://apod.nasa.gov/apod/image/1105/SupernovaSonata_parker900.jpg[/img][/url][/float]To create a sonata from supernovae, first you have to [url=http://arxiv.org/abs/1104.1443]find the supernovae[/url]. To do that composers Alex Parker and Melissa Graham relied on the [url=http://www.cfht.hawaii.edu/Science/CFHLS/]Canada France Hawaii Telescope (CFHT) Legacy Survey[/url] data of four deep fields on the sky monitored from April 2003 through August 2006, adopting 241 Type Ia supernovae. [url=http://apod.nasa.gov/apod/ap110430.html]Enchanting[/url] to [url=http://apod.nasa.gov/apod/ap110330.html]cosmologists[/url], [url=http://en.wikipedia.org/wiki/Type_Ia_supernova]Type Ia supernovae[/url] are thermonuclear explosions that destroy white dwarf stars. Then, they gave each supernova a note to play, the volume of the note determined by the distance to the supernova. Fainter, more distant supernovae play quieter notes. [url=http://hyperphysics.phy-astr.gsu.edu/hbase/sound/pitch.html]Each note's pitch[/url] was based on a [url=http://arxiv.org/abs/astro-ph/0104382]stretch factor[/url] measured by how fast the supernova brightens and fades over time relative to an adopted standard time history. Higher stretch factors play higher notes in pitches drawn from the illustrated [url=http://en.wikipedia.org/wiki/Phrygian_dominant_scale]Phrygian dominant scale[/url]. Of course, each supernova note is played on an instrument. Supernovae in massive galaxies were assigned to a stand-up bass, while supernovae in less massive galaxies played their note on a grand piano. Click on the image or follow these links ([url=http://vimeo.com/23927216]Vimeo[/url], [url=http://www.youtube.com/watch?v=9h_ZrD7axi4]YouTube[/url]) to watch a time compressed animation of the CFHT Legacy Survey data while [url=http://www.astro.uvic.ca/~alexhp/new/supernova_sonata.html]listening to the Supernova Sonata[/url].
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110527.html][size=150][b]Messier Marathon (2011 May 27)[/b][/size][/url][/c]
[float=left][imghover=http://apod.nasa.gov/apod/image/1105/MilkyWayObservers_tafreshi1100.jpg]http://apod.nasa.gov/apod/image/1105/MilkyWayObserversLabels3_tafreshi1100.jpg[/imghover][/float] [url=http://www.twanight.org/newtwan/photos.asp?ID=3003233&Sort=Site]In this action scene[/url], red night vision lights, green laser pointers, tripods and telescopes in faint silhouette surround intrepid sky gazers embarked on the 10th annual Iran [url=http://www.seds.org/messier/xtra/marathon/marathon.html]Messier Marathon[/url]. Completing the marathon requires viewing all 110 objects in 18th century French astronomer [url=http://www.seds.org/messier/xtra/history/m-cat.html]Charles Messier's catalog[/url] in one glorious dusk-to-dawn observing run. As daunting as it sounds, there are often favorable weekend dates for northern hemisphere marathoners to complete the task that fall on nearly moonless nights near the spring equinox. With the Milky Way as a backdrop, this [url=http://dreamview.net/dv/new/photos.asp?id=102254]group of about 150 astronomy enthusiasts[/url] conducted their 2011 marathon on [url=http://apod.nasa.gov/apod/ap080419.html]such a night[/url] in April from the desert area of [url=http://www.twanight.org/newtwan/galleries.asp?Sort=Site&Value=Seh%20Qaleh&page=1]Seh Qaleh[/url], in eastern Iran. Placing your cursor over the image will map the stunning night sky above their remote and very dark observing site. Follow the green laser pointer toward the Messier catalog objects (for example, [url=http://apod.nasa.gov/apod/ap070804.html]M8[/url]) near the galactic center. Astronomer and former Messier Marathon organizer Babak Tafreshi also composed [url=http://www.twanight.org/newTWAN/photos.asp?ID=3003232&Background=dark]Sky Gazers, a time-lapse movie[/url] of this year's event.
[clear][/clear]
[c][url=http://apod.nasa.gov/apod/ap110528.html][size=150][b]The Mileage of Light (2011 May 28)[/b][/size][/url][/c]
[float=left][img2]http://apod.nasa.gov/apod/image/1105/OdometerC_Mammana900.jpg[/img2][/float][url=http://apod.nasa.gov/apod/ap981212.html]If you're driving[/url] down a dark road on a starry night, you might want to check the odometer. Earlier this month, when traveling astronomer Dennis Mammana did he was greeted with the significant mileage reading of 186,282 miles. That's the number of miles [url=http://en.wikipedia.org/wiki/Speed_of_light]light travels in one second[/url]. Or, if you prefer kilometers, the number you are looking for is 299,792. Mammana muses that in driving to countless [url=http://apod.nasa.gov/apod/ap101216.html]observatories[/url], [url=http://apod.nasa.gov/apod/ap081011.html]star parties[/url], and [url=http://www.dennismammana.com/gallery/night.htm]night sky photo shoots[/url] it has taken his 1998 vintage sport utility vehicle over 13 years to cover that distance. Of course, he considers his next important mileage milestone to be the distance [url=http://solarsystem.nasa.gov/planets/profile.cfm?Display=Facts&Object=Moon]to the Moon[/url].
[clear][/clear]
[size=110][url=http://asterisk.apod.com/viewtopic.php?f=29&t=23735][color=#4040FF][b]<- Previous week's poll[/b][/color][/url][/size]