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|
Reporting to the Launch Pad
The payload fairing carrying
…
2/16/09
| Description |
The payload fairing carrying NASA's Orbiting Carbon Observatory arrives at Space Launch Complex 576-E at Vandenberg Air Force Base in California. The spacecraft will launch aboard Orbital Sciences' Taurus XL rocket, being erected at left. Image credit: NASA/Randy Beaudoin, VAFB Feb. 10, 2009 |
| Date |
2/16/09 |
|
Taurus Stands Tall
NASA's Orbiting Carbon Obser
…
2/20/09
| Description |
NASA's Orbiting Carbon Observatory, OCO, upper stack is lowered onto the Stage 0 motor of Orbital Sciences' Taurus XL vehicle. The vehicle and spacecraft will launch from Launch Complex 576-E at Vandenberg Air Force Base in California. Image credit: NASA/Richard Nielsen Feb. 19, 2009 |
| Date |
2/20/09 |
|
Liftoff!
NASA's Orbiting Carbon Obser
…
2/25/09
| Description |
NASA's Orbiting Carbon Observatory and its Taurus booster lift off Feb. 24 from Vandenberg Air Force Base in California at 4:55 a.m. EST. The satellite ultimately did not reach orbit when the payload fairing failed to separate properly. Image courtesy of Orbital Sciences Corp. Feb. 24, 2009 |
| Date |
2/25/09 |
|
Star-Crossed Rings
| Description |
Star-Crossed Rings |
| Full Description |
This image is a false-color ultraviolet view of Saturn's B ring (center) and A ring (right), separated by a large gap known as the Cassini Division. It shows a bright horizontal streak, created by a series of time lapse images involving a star named 26 Taurus. The image was made over a nine-hour period as the star drifted behind the rings. The opacity of the outer A ring is most pronounced on its inner edge, indicating more ring debris is present there. The Encke Gap, much smaller than the Cassini Division, is visible near the outer edge of the A ring. The B ring is significantly more opaque than the A ring, indicating a greater density of ring material when imaged from above. The sky behind the rings glows red in the ultraviolet wavelengths from the hydrogen gas that fills the solar system. The images were processed from data taken by the ultraviolet imaging spectrograph aboard the Cassini spacecraft in May 2005. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The ultraviolet imaging spectrograph was built at, and the team is based at the University of Colorado, Boulder. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov. The ultraviolet imaging spectrograph team home page is at http://lasp.colorado.edu/cassini. Credit: NASA/JPL/University of Colorado |
| Date |
April 6, 2006 |
|
Long Leonid
| Title |
Long Leonid |
| Explanation |
Just last week this long lovely Leonid shower [ http://spacescience.com/headlines/y2000/ ast21nov_1.htm ] meteor arced through the night. Captured on [ http://www.comet-track.com/meteor/leonids00/ leonids00.html ] November 17/18 by photographer [ http://www.comet-track.com ] Bob Yen, the meteor trail spans about 70 times the apparent diameter of the full moon in the skies above Mt. Wilson, California, USA. The Leonid's path flashes from the outskirts of constellation Gemini [ http://www.seds.org/Maps/Stars_en/Fig/ gemini.html ] to the triangle-shaped head of Taurus [ http://www.astro.uiuc.edu/~kaler/sow/ taurus-p.html ] (lower right). Of course, the trail points back toward Leo, the shower's [ http://comets.amsmeteors.org/meteors/showers/ leonids.html ] eponymous radiant, while passing near such night sky notables as galactic star cluster M35 [ http://www.seds.org/messier/m/m035.html ] (upper left) and Taurus's brightest star, red giant Aldebaran [ http://www.astro.uiuc.edu/~kaler/sow/ aldebaran.html ]. Though the sky was ruled by a bright but waning Moon and brilliant Jupiter, the Leonid meteor shower [ http://www.spaceweather.com/meteors/gallery_18nov00.html ] still awed observers at dark sky locations with peak rates of hundreds of meteors per hour. |
|
Taurus Prepared to Carry Glo
…
glorymultimediagallery, nasa
The first, second and third
…
504065main_2010-10-16
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2010-12-07 |
| creator |
NASA |
| identifier |
504065main_2010-10-16 |
|
Taurus Prepared to Carry Glo
…
glorymultimediagallery, nasa
In Building 1555 at Vandenbe
…
504077main_2010-11-01
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2010-12-07 |
| creator |
NASA |
| identifier |
504077main_2010-11-01 |
|
Taurus Prepared to Carry Glo
…
glorymultimediagallery, nasa
At the Orbital Sciences payl
…
504002main_2008-11-13-3
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2010-12-07 |
| creator |
NASA |
| identifier |
504002main_2008-11-13-3 |
|
Present Day -- Taurus XL
nasa, nasarocketryimagegalle
…
A Taurus XL rocket prepares
…
481579main_rpd_Taurus
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2010-09-16 |
| creator |
NASA |
| identifier |
481579main_rpd_Taurus |
|
Taurus Prepared to Carry Glo
…
glorymultimediagallery, nasa
At Vandenberg Air Force Base
…
504089main_2010-11-16
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2010-12-07 |
| creator |
NASA |
| identifier |
504089main_2010-11-16 |
|
Star-Crossed Rings
PIA08036
Saturn
Ultraviolet Imaging Spectrog
…
| Title |
Star-Crossed Rings |
| Original Caption Released with Image |
This image is a false-color ultraviolet view of Saturn's B ring (center) and A ring (right), separated by a large gap known as the Cassini Division. It shows a bright horizontal streak, created by a series of time lapse images involving a star named 26 Taurus. The image was made over a nine-hour period as the star drifted behind the rings. The opacity of the outer A ring is most pronounced on its inner edge, indicating more ring debris is present there. The Encke Gap, much smaller than the Cassini Division, is visible near the outer edge of the A ring. The B ring is significantly more opaque than the A ring, indicating a greater density of ring material when imaged from above. The sky behind the rings glows red in the ultraviolet wavelengths from the hydrogen gas that fills the solar system. The images were processed from data taken by the ultraviolet imaging spectrograph aboard the Cassini spacecraft in May 2005. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The ultraviolet imaging spectrograph was built at, and the team is based at the University of Colorado, Boulder. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov/home/index.cfm [ http://saturn.jpl.nasa.gov ]. The ultraviolet imaging spectrograph team home page is at http://lasp.colorado.edu/cassini [ http://lasp.colorado.edu/cassini ]. |
|
Dead Star Creates Celestial
…
PIA01320
Infrared Array Camera (IRAC)
…
| Title |
Dead Star Creates Celestial Havoc |
| Original Caption Released with Image |
A star's spectacular death in the constellation Taurus was observed on Earth as the supernova of 1054 A.D. Now, almost a thousand years later, a superdense neutron star left behind by the stellar death is spewing out a blizzard of extremely high-energy particles into the expanding debris field known as the Crab Nebula. This composite image uses data from three of NASA's Great Observatories. The Chandra X-ray image is shown in light blue, the Hubble Space Telescope optical images are in green and dark blue, and the Spitzer Space Telescope's infrared image is in red. The size of the X-ray image is smaller than the others because ultrahigh-energy X-ray emitting electrons radiate away their energy more quickly than the lower-energy electrons emitting optical and infrared light. The neutron star, which has the mass equivalent to the sun crammed into a rapidly spinning ball of neutrons twelve miles across, is the bright white dot in the center of the image. |
|
The Seven Sisters
PIA08260
Unknown target/parent relati
…
Imaging Science Subsystem -
…
| Title |
The Seven Sisters |
| Original Caption Released with Image |
The stars of the Pleiades cluster, also known by the names "M45" and "the Seven Sisters," shine brightly in this view from the Cassini spacecraft. The cluster is comprised of hundreds of stars, a few of which are visible to the unaided eye on Earth as a brilliant grouping in the constellation Taurus. Some faint nebulous material is seen here. This reflection nebula is dust that reflects the light of the hot, blue stars in the cluster. The monochrome view was made by combining 49 clear filter images of the Pleiades taken with the Cassini spacecraft wide-angle camera on Aug. 1, 2006. The images were taken as a part of a sequence designed to help calibrate the camera electronics. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov/home/index.cfm [ http://saturn.jpl.nasa.gov ]. The Cassini imaging team homepage is at http://ciclops.org [ http://ciclops.org ]. |
|
The Seven Sisters Pose for S
…
PIA09263
Infrared Array Camera (IRAC)
…
| Title |
The Seven Sisters Pose for Spitzer |
| Original Caption Released with Image |
The Seven Sisters, also known as the Pleiades star cluster, seem to float on a bed of feathers in a new infrared image from NASA's Spitzer Space Telescope. Clouds of dust sweep around the stars, swaddling them in a cushiony veil. The Pleiades, located more than 400 light-years away in the Taurus constellation, are the subject of many legends and writings. Greek mythology holds that the flock of stars was transformed into celestial doves by Zeus to save them from a pursuant Orion. The 19th-century poet Alfred Lord Tennyson described them as "glittering like a swarm of fireflies tangled in a silver braid." The star cluster was born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5-billion-year-old sun. The brightest members of the cluster, also the highest-mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower-mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The new infrared image from Spitzer highlights the "tangled silver braid" mentioned in the poem by Tennyson. This spider-web-like network of filaments, colored yellow, green and red in this view, is made up of dust associated with the cloud through which the cluster is traveling. The densest portion of the cloud appears in yellow and red, and the more diffuse outskirts are shown in green hues. One of the parent stars, Atlas, can be seen at the bottom, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue. The Spitzer data also reveal never-before-seen brown dwarfs, or "failed stars," and disks of planetary debris (not pictured). John Stauffer of NASA's Spitzer Space Telescope mission says Spitzer's infrared vision allows astronomers to better study the cooler, lower-mass stars in the region, which are much fainter when viewed in optical light. Stauffer, who admits to being biased because the Pleiades is his favorite astronomical object, says the cluster is the perfect laboratory for understanding the evolution of stars. This image is made up of data taken by Spitzer's multiband imaging photometer and its infrared array camera. Light with a wavelength of 4.5 microns is blue, light of 8 microns is green, and light of 24 microns is red. Venus and Pleiades Mingle in the Sky The sky chart in figure 1, illustrates the Venus-Pleiades encounter that reached its closest approach on April 11, 2007. The Pleiades are a tight gem-like cluster of stars that resemble a tiny dipper (but should not be confused with the Little Dipper constellation). If you look west shortly after sunset, Venus will be the brightest object in the sky. If the skies are clear and dark, you'll also see the Pleiades twinkling above Venus. On April 19, the moon will join the party, sliding between Venus and the Pleiades. Viewers in the northern and southern hemispheres will be able to witness the event. |
|
The Seven Sisters Pose for S
…
PIA09263
Infrared Array Camera (IRAC)
…
| Title |
The Seven Sisters Pose for Spitzer |
| Original Caption Released with Image |
The Seven Sisters, also known as the Pleiades star cluster, seem to float on a bed of feathers in a new infrared image from NASA's Spitzer Space Telescope. Clouds of dust sweep around the stars, swaddling them in a cushiony veil. The Pleiades, located more than 400 light-years away in the Taurus constellation, are the subject of many legends and writings. Greek mythology holds that the flock of stars was transformed into celestial doves by Zeus to save them from a pursuant Orion. The 19th-century poet Alfred Lord Tennyson described them as "glittering like a swarm of fireflies tangled in a silver braid." The star cluster was born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5-billion-year-old sun. The brightest members of the cluster, also the highest-mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower-mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The new infrared image from Spitzer highlights the "tangled silver braid" mentioned in the poem by Tennyson. This spider-web-like network of filaments, colored yellow, green and red in this view, is made up of dust associated with the cloud through which the cluster is traveling. The densest portion of the cloud appears in yellow and red, and the more diffuse outskirts are shown in green hues. One of the parent stars, Atlas, can be seen at the bottom, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue. The Spitzer data also reveal never-before-seen brown dwarfs, or "failed stars," and disks of planetary debris (not pictured). John Stauffer of NASA's Spitzer Space Telescope mission says Spitzer's infrared vision allows astronomers to better study the cooler, lower-mass stars in the region, which are much fainter when viewed in optical light. Stauffer, who admits to being biased because the Pleiades is his favorite astronomical object, says the cluster is the perfect laboratory for understanding the evolution of stars. This image is made up of data taken by Spitzer's multiband imaging photometer and its infrared array camera. Light with a wavelength of 4.5 microns is blue, light of 8 microns is green, and light of 24 microns is red. Venus and Pleiades Mingle in the Sky The sky chart in figure 1, illustrates the Venus-Pleiades encounter that reached its closest approach on April 11, 2007. The Pleiades are a tight gem-like cluster of stars that resemble a tiny dipper (but should not be confused with the Little Dipper constellation). If you look west shortly after sunset, Venus will be the brightest object in the sky. If the skies are clear and dark, you'll also see the Pleiades twinkling above Venus. On April 19, the moon will join the party, sliding between Venus and the Pleiades. Viewers in the northern and southern hemispheres will be able to witness the event. |
|
The Seven Sisters Pose for S
…
PIA09263
Infrared Array Camera (IRAC)
…
| Title |
The Seven Sisters Pose for Spitzer |
| Original Caption Released with Image |
The Seven Sisters, also known as the Pleiades star cluster, seem to float on a bed of feathers in a new infrared image from NASA's Spitzer Space Telescope. Clouds of dust sweep around the stars, swaddling them in a cushiony veil. The Pleiades, located more than 400 light-years away in the Taurus constellation, are the subject of many legends and writings. Greek mythology holds that the flock of stars was transformed into celestial doves by Zeus to save them from a pursuant Orion. The 19th-century poet Alfred Lord Tennyson described them as "glittering like a swarm of fireflies tangled in a silver braid." The star cluster was born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5-billion-year-old sun. The brightest members of the cluster, also the highest-mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower-mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The new infrared image from Spitzer highlights the "tangled silver braid" mentioned in the poem by Tennyson. This spider-web-like network of filaments, colored yellow, green and red in this view, is made up of dust associated with the cloud through which the cluster is traveling. The densest portion of the cloud appears in yellow and red, and the more diffuse outskirts are shown in green hues. One of the parent stars, Atlas, can be seen at the bottom, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue. The Spitzer data also reveal never-before-seen brown dwarfs, or "failed stars," and disks of planetary debris (not pictured). John Stauffer of NASA's Spitzer Space Telescope mission says Spitzer's infrared vision allows astronomers to better study the cooler, lower-mass stars in the region, which are much fainter when viewed in optical light. Stauffer, who admits to being biased because the Pleiades is his favorite astronomical object, says the cluster is the perfect laboratory for understanding the evolution of stars. This image is made up of data taken by Spitzer's multiband imaging photometer and its infrared array camera. Light with a wavelength of 4.5 microns is blue, light of 8 microns is green, and light of 24 microns is red. Venus and Pleiades Mingle in the Sky The sky chart in figure 1, illustrates the Venus-Pleiades encounter that reached its closest approach on April 11, 2007. The Pleiades are a tight gem-like cluster of stars that resemble a tiny dipper (but should not be confused with the Little Dipper constellation). If you look west shortly after sunset, Venus will be the brightest object in the sky. If the skies are clear and dark, you'll also see the Pleiades twinkling above Venus. On April 19, the moon will join the party, sliding between Venus and the Pleiades. Viewers in the northern and southern hemispheres will be able to witness the event. |
|
Pink Pleiades
PIA09262
Infrared Array Camera (IRAC)
| Title |
Pink Pleiades |
| Original Caption Released with Image |
Venus and Pleiades Mingle in the Sky Diagram The Seven Sisters, also known as the Pleiades star cluster, seem to float on a bed of feathers in a new infrared image from NASA's Spitzer Space Telescope. Clouds of dust sweep around the stars, swaddling them in a cushiony veil. The Pleiades, located more than 400 light-years away in the Taurus constellation, are the subject of many legends and writings. Greek mythology holds that the flock of stars was transformed into celestial doves by Zeus to save them from a pursuant Orion. The 19th-century poet Alfred Lord Tennyson described them as "glittering like a swarm of fireflies tangled in a silver braid." The star cluster was born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5-billion-year-old sun. The brightest members of the cluster, also the highest-mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower-mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The new infrared image from Spitzer highlights the "tangled silver braid" mentioned in the poem by Tennyson. This spider-web-like network of filaments, colored red in this view, is made up of dust associated with the cloud through which the cluster is traveling. One of the parent stars, Atlas, can be seen at the bottom, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue. The Spitzer data also reveal never-before-seen brown dwarfs, or "failed stars," and disks of planetary debris (not pictured). John Stauffer of NASA's Spitzer Space Telescope mission says Spitzer's infrared vision allows astronomers to better study the cooler, lower-mass stars in the region, which are much fainter when viewed in optical light. Stauffer, who admits to being biased because the Pleiades is his favorite astronomical object, says the cluster is the perfect laboratory for understanding the evolution of stars. This image shows infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange, light of 4.5 microns is green, and light of 3.6 microns is blue. Venus and Pleiades Mingle in the Sky The sky chart in figure 1, illustrates the Venus-Pleiades encounter that reached its closest approach on April 11, 2007. The Pleiades are a tight gem-like cluster of stars that resemble a tiny dipper (but should not be confused with the Little Dipper constellation). If you look west shortly after sunset, Venus will be the brightest object in the sky. If the skies are clear and dark, you'll also see the Pleiades twinkling above Venus. On April 19, the moon will join the party, sliding between Venus and the Pleiades. Viewers in the northern and southern hemispheres will be able to witness the event. |
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