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Finding a Place
On Launch Complex 41 at Cape
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5/29/09
| Description |
On Launch Complex 41 at Cape Canaveral Air Force Station in Florida, the Lunar Reconnaissance Orbiter, or LRO, and NASA's Lunar Crater Observation and Sensing Satellite, known as LCROSS, are moved into the mobile service tower. The LRO will be mated to the Atlas V rocket for launch. May 28, 2009 Photo credit: NASA/Dimitri Gerondidakis |
| Date |
5/29/09 |
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In One Piece
On Launch Complex 41 at Cape
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5/29/09
| Description |
On Launch Complex 41 at Cape Canaveral Air Force Station in Florida, the Lunar Reconnaissance Orbiter, or LRO, and NASA's Lunar Crater Observation and Sensing Satellite, known as LCROSS, are mated with the Atlas V rocket inside the mobile service tower for launch. May 28, 2009 Photo credit: NASA/Dimitri Gerondidakis |
| Date |
5/29/09 |
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Connecting to Launch Vehicle
Workers prepare to connect L
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5/29/09
| Description |
Workers prepare to connect LRO and LCROSS inside the mobile service tower with the Atlas V rocket for launch. Photo credit: NASA/Dimitri Gerondidakis May 28, 2009 |
| Date |
5/29/09 |
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Atlas V Stands Tall
On Launch Complex 41 at Cape
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5/29/09
| Description |
On Launch Complex 41 at Cape Canaveral Air Force Station in Florida, NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite are connected with the Atlas V rocket inside the mobile service tower for launch. Photo credit: NASA/Dimitri Gerondidakis May 28, 2009 |
| Date |
5/29/09 |
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Fly Me to the Moon
At Launch Complex-41 on Cape
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6/18/09
| Description |
At Launch Complex-41 on Cape Canaveral Air Force Station in Florida, the Atlas V/Centaur rocket, with NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite on top, rolls out to the launch pad. The missions are the first in NASA's plan to return humans to the moon and begin establishing a lunar outpost by 2020. The orbiter spacecraft includes seven instruments that will help NASA characterize the moon's surface. Image credit: NASA/Jack Pfaller June 17, 2009 |
| Date |
6/18/09 |
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Ready to Roll
This photo reveals the paylo
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6/18/09
| Description |
This photo reveals the payload fairing carrying NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite ready to roll out to the launch pad atop the Atlas V/Centaur rocket. June 17, 2009 Photo credit: NASA/Jack Pfaller |
| Date |
6/18/09 |
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At the Launch Pad
On Launch Complex-41 on Cape
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6/18/09
| Description |
On Launch Complex-41 on Cape Canaveral Air Force Station in Florida, the Atlas V/Centaur rocket reaches the launch pad carrying NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite. Circling the pad are the protective lightning towers. June 17, 2009 Photo credit: NASA/Jack Pfaller |
| Date |
6/18/09 |
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Standing Tall
The Atlas V/Centaur rocket w
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6/18/09
| Description |
The Atlas V/Centaur rocket with NASA's Lunar Reconnaissance Orbiter, or LRO, and NASA's Lunar Crater Observation and Sensing Satellite, known as LCROSS, on top are on the pad at Launch Complex-41 on Cape Canaveral Air Force Station in Florida. June 17, 2009 Photo credit: NASA/Jack Pfaller |
| Date |
6/18/09 |
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Ignition and Liftoff!
Rising on a column of fire,
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6/18/09
| Description |
Rising on a column of fire, the Atlas V/Centaur rocket roars into space carrying NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite. June 18, 2009 Photo Credit: United Launch Alliance/Pat Corkery |
| Date |
6/18/09 |
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...And the Atlas V Clears th
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The Atlas V/Centaur rocket c
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6/18/09
| Description |
The Atlas V/Centaur rocket climbs up and away from Launch Complex 41 at Cape Canaveral Air Force Station in Florida. Safely tucked inside the protective payload fairing are NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite. June 18, 2009 Photo Credit: NASA/Bill Ingalls |
| Date |
6/18/09 |
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Up and Away
After a flawless liftoff, th
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6/18/09
| Description |
After a flawless liftoff, the Atlas V/Centaur rocket speeds toward space carrying NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite. LRO and LCROSS are the first missions in NASA's plan to return humans to the moon and begin establishing a lunar outpost by 2020. June 18, 2009 Photo Credit: NASA/Bill Ingalls |
| Date |
6/18/09 |
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To the Moon
Fire and smoke signal the li
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6/19/09
| Description |
Fire and smoke signal the liftoff of the Atlas V/Centaur carrying NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite on their missions to the moon. Launch from Launch Complex 41 at Cape Canaveral Air Force Station in Florida was on-time at 5:32 p.m. EDT. June 18, 2009 Image credit: NASA/Tom Farrar, Kevin O'Connell |
| Date |
6/19/09 |
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Two Spacecraft Head to the M
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The Atlas V/Centaur rocket c
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6/19/09
| Description |
The Atlas V/Centaur rocket carrying NASA's Lunar Reconnaissance Orbiter and NASA's Lunar Crater Observation and Sensing Satellite lifts off from Launch Complex 41 at Cape Canaveral Air Force Station in Florida. Image credit: NASA/Jeffery Marino June 18, 2009 |
| Date |
6/19/09 |
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The Road to Apollo
Project Fire explored the in
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3/9/09
| Description |
Project Fire explored the intense heat of atmospheric reentry and its effects on would-be spacecraft materials. Although the ultimate tests involved Atlas rockets carrying recoverable reentry packages, the flight tests from Cape Canaveral were preceded by a series of important wind-tunnel tests at Langley. Here technicians ready materials for a high-temperature wind tunnel test. Credit: NASA |
| Date |
3/9/09 |
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Mercury -- February 1962
Astronaut John H. Glenn Jr.,
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7/16/08
| Description |
Astronaut John H. Glenn Jr., NASA flight surgeon William Douglas and equipment specialist Joseph W. Schmidt leave crew quarters prior to the Mercury-Atlas 6 mission. Glenn is in his pressure suit and is carrying the portable ventilation unit. |
| Date |
7/16/08 |
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Mercury -- September 1962
Astronaut Walter M. "Wally"
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7/16/08
| Description |
Astronaut Walter M. "Wally" Schirra Jr., pilot of the Mercury-Atlas 8 Earth-orbital spaceflight, goes through a suiting-up exercise at Cape Canaveral several weeks prior to his scheduled Oct. 3, 1962 flight. |
| Date |
7/16/08 |
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Mercury -- May 1963
Mercury astronaut L. Gordon
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7/16/08
| Description |
Mercury astronaut L. Gordon Cooper Jr. is wearing a spacesuit during Mercury-Atlas 9 prelaunch activities. |
| Date |
7/16/08 |
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Atlas V for Next NASA Moon M
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The Atlas V first stage for
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4/27/09
| Description |
The Atlas V first stage for the Lunar Reconnaissance Orbiter (LRO) and the Lunar Crater Observation and Sensing Satellite (LCROSS) mission was moved on April 27 from its hangar to the Vertical Integration Facility at Launch Complex 41 at Cape Canaveral Air Force Station, Fla. The Centaur upper stage followed on April 30 for stacking atop the Atlas rocket. Launch preparations now will begin for a liftoff targeted for no earlier than June 2. The Lunar Reconnaissance Orbiter will orbit the poles of the moon for up to five years surveying and mapping its surface. The Centaur stage of this Atlas V has a unique role of continuing to the moon with LCROSS to impact the lunar surface shortly after arrival. Scientists will observe the subsurface material that is ejected, particularly looking for ice and minerals. |
| Date |
4/27/09 |
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Walter Schirra
Pictured is astronaut Walter
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11/19/07
| Description |
Pictured is astronaut Walter M. Schirra, one of the original seven astronauts for Mercury Project selected by NASA on April 27, 1959. Schirra's Mercury-Atlas 8 mission, during which he piloted his Sigma 7 spacecraft, was the third manned orbital flight by the United States. Image credit: NASA |
| Date |
11/19/07 |
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Mercury-Atlas 9
Technicians were performing
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4/10/09
| Description |
Technicians were performing pre-launch testing of the Mercury-Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral when this photo was taken on May 14, 1963.... |
| Date |
4/10/09 |
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Mercury-Atlas 9
Technicians were performing
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4/10/09
| Description |
Technicians were performing pre-launch testing of the Mercury-Atlas 9 (MA9) on Launch Pad 14 at Cape Canaveral when this photo was taken on May 14, 1963. A day later on May 15, Gordon Cooper successfully piloted this his 'Faith 7' spacecraft for more than 34 hours and 22 orbits. Cooper's flight stretched the capabilities of the Mercury capsule to the limits. His 34-hour flight lasted more than three times the longest U.S. human space flight until that time, and far exceeded the initial design capability of the capsule. Image Credit: NASA |
| Date |
4/10/09 |
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Building an Original
Platforms surround the Ares
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10/23/09
| Description |
Platforms surround the Ares I-X in High Bay 3 of the Vehicle Assembly Building before it was moved to the launch pad on Oct. 20, 2009. Closer in height to the hulking Saturn V moon rockets than the space shuttle, Ares I-X looks unlike any rocket that's ever stood at Launch Complex 39. But it blends familiar hardware from existing programs with newly developed components. Four first-stage, solid-fuel booster segments are derived from the Space Shuttle Program. A simulated fifth booster segment contains Atlas-V-based avionics, and the rocket's roll control system comes from the Peacekeeper missile. The launch abort system, simulated crew and service modules, upper stage, and various connecting structures all are original. Image Credit: NASA/Jack Pfaller |
| Date |
10/23/09 |
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Glenn and STS-95 Go to Space
The seven crew members in tr
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10/29/09
| Description |
The seven crew members in training for the STS-95 mission aboard Discovery pose for photographers prior to participating in a training session at NASA's Johnson Space Center. Pictured, from the left, are Pedro Duque, Curtis Brown, Chiaki Nauto-Mukai, then-U.S. Sen. John H. Glenn Jr. (D.-Ohio), Stephen Robinson, Steven Lindsey and Scott Parazynski. Sen. Glenn, who served as a payload specialist for the mission, launched with the Discovery crew on Oct. 29, 1998. On Feb. 20, 1962, Glenn piloted the Mercury-Atlas 6 Friendship 7 spacecraft on America's first manned orbital mission. Image Credit: NASA |
| Date |
10/29/09 |
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Eastern Morocco
This spaceborne radar image
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5/22/97
| Date |
5/22/97 |
| Description |
This spaceborne radar image shows how the Atlas Mountains in northwestern Africa dominate the geography of Morocco. The image shows a part of the eastern flank of these mountains near the town of Rissani, approximately 50 kilometers (31 miles) from its border with Algeria. The striking bright patterns are the complex folds in the layered rocks of this region. Careful examination of the image shows areas where the folded structures have been disrupted due to fault movement and earthquakes. Dark areas between the rock outcrops are covered in sand and serve as channels for seasonal streams in this arid region. Scientists can use images like this one to map the geology and drainage patterns in arid regions. The area shown is 44 kilometers by 34 kilometers (27 miles by 21 miles) centered at 31 degrees north latitude, 4.4 degrees west longitude, north is toward the upper right. Colors are assigned to different radar frequencies and polarizations as follows: red is L-band horizontally transmitted, horizontally received, green is C-band horizontally transmitted, horizontally received, blue is C-band horizontally transmitted, vertically received. The image was acquired by the Spaceborne Imaging Radar-C/X-band Synthetic Aperture (SIR-C/X- SAR) imaging radar when it flew aboard the space shuttle Endeavour on April 15, 1994. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth program. ##### |
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This picture of Venus was ca
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| Description |
This picture of Venus was captured by the Mariner 10 spacecraft during its approach to the planet in early 1974. Taken with the spacecraft's imaging system using an ultraviolet filter, the picture has been color enhanced to simulate Venus's natural color as the human eye would see it. Although the planet closest to the Earth in size and distance from the Sun, Venus is perpetually blanketed by a thick veil of clouds high in carbon dioxide, its surface temperature approaches 900 degrees Fahrenheit. Launched on November 3, 1973 atop an Atlas Centaur rocket, Mariner 10 flew by Venus on February 5, 1974. It then went on to an encounter with Mercury, thus becoming the first spacecraft ever to fly by more than one planet. Mariner 10 was designed, built and managed by the Jet Propulsion Laboratory for NASA's Office of Space Science and Applications. |
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The Seven Sisters Pose for S
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| Title |
The Seven Sisters Pose for Spitzer |
| Description |
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. |
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The Seven Sisters Pose for S
…
| Title |
The Seven Sisters Pose for Spitzer |
| Description |
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. |
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Pink Pleiades
| Title |
Pink Pleiades |
| Description |
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. |
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Pink Pleiades
| Title |
Pink Pleiades |
| Description |
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. |
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NASA TV's This Week @NASA, F
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* President Obama spoke with
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02/19/10
| Description |
* President Obama spoke with the crews of space shuttle Endeavour and the International Space Station from the Roosevelt Room of the White House. * New findings by NASA's Chandra X-ray Observatory in the Andromeda galaxy have provided a major advance in understanding a type of supernova believed critical to studying dark energy. * The telescope aboard NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, was successfully activated during a January 15 test flight of almost six hours. * A new NASA Web site can help our future explorers and leaders better understand the how's and why's of climate change and what they can do to make our planet more habitable. * Scott Carpenter: ''Godspeed John Glenn'' Forty-eight years ago, Mercury astronaut John Glenn became the first American to orbit the Earth when an Atlas rocket successfully carried his Friendship 7 capsule into space. |
| Date |
02/19/10 |
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Watching Atlas's Waistline
| Description |
Watching Atlas's Waistline |
| Full Description |
The Cassini spacecraft finds oddly-shaped Atlas gliding along the edge of the A ring. The moon has a prominent equatorial bulge, which is accentuated here by the grazing viewing angle of Cassini, making Atlas appear pointy. Cassini images revealed in 2004 that a faint ring of material coincides with the orbit of Atlas (32 kilometers, or 20 miles across). See The Atlas Ring for more information. This view looks upward, toward the lit side of Saturn's rings. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on June 30, 2006 at a distance of approximately 283,000 kilometers (176,000 miles) from Atlas. Image scale is 2 kilometers (1 mile) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
August 1, 2006 |
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Down Under on Pan
| Description |
Down Under on Pan |
| Full Description |
Hiding within the Encke gap is the small moon Pan, partly in shadow and party cut off by the outer A ring in this view. Similar to Atlas, Pan appears to have a slight ridge around its middle, and like Atlas, Pan's orbit also coincides with a faint ringlet. (See Cruising with Pan for a movie featuring Pan). Pan is 26 kilometers (16 miles) across. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on June 30, 2006 at a distance of approximately 269,000 kilometers (167,000 miles) from Pan. Image scale is 2 kilometers (5,259 feet) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
July 27, 2006 |
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Saturn Shine
| Description |
Saturn Shine |
| Full Description |
This view looks down onto the unlit side of Saturn's ringplane. It nicely shows a near-arm/far-arm brightness asymmetry in the B ring: The near arm of the B ring (in the lower half of the image) is notably darker from this viewing geometry than is the far arm (above). Imaging scientists believe this to be a manifestation of the reflection of light from the disk of Saturn falling predominantly on the far arm of the rings. (At the time this image was taken, Cassini was more or less on the dark side of the planet.) As the B ring is the thickest part of Saturn's rings, it scatters less sunlight from below, and reflects more Saturn shine from above, than either the A or C rings, making the effect look more dramatic in the B ring. Two small moons appear in this scene as well: Atlas (32 kilometers, or 20 miles across) is visible above and left of center and outside the A ring, Pandora (84 kilometers, or 52 miles across) can be seen near upper right beyond the F ring. Between the two moons lie multiple clumps of material in the F ring. The image was taken in visible light with the Cassini spacecraft wide-angle camera on July 25, 2006 at a distance of approximately 1 million kilometers (600,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 128 degrees. Image scale is 58 kilometers (36 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
August 28, 2006 |
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Janus Hides in Plain Sight
| Description |
Janus Hides in Plain Sight |
| Full Description |
Tiny, dust-sized particles in Saturn's rings become much easier to see at high phase angle -- the angle formed by the Sun, the rings and the spacecraft. The brightest ring at the right is the F ring, the next feature to the left is the outer edge of the A ring. Inward of that, and very bright, are the ringlets in the Encke gap. Epimetheus (116 kilometers, or 72 miles across) is easy to spot just right of the outer F ring edge. Janus (181 kilometers, or 113 miles across), however, is quite a bit harder to make out, it is the dark spot located directly to the left of Epimetheus, above the gap between the A and F rings. Within the space between the A and F rings there are two faint rings seen previously by the Cassini spacecraft. The inner faint ring (called R/2004 S1) coincides with the orbit of Atlas. The outer one forms the inner boundary of the orbit of Prometheus. The narrow G ring is visible above and below the bright F ring. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on July 15, 2006 at a distance of approximately 2.7 million kilometers (1.7 million miles) from Epimetheus and 2.8 million kilometers (1.7 million miles) from Janus. The view was acquired at a Sun-Epimetheus-spacecraft, or phase, angle of 164 degrees. Image scale is 16 kilometers (10 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
August 16, 2006 |
|
Toward the Shadow
| Description |
This strikingly crisp view shows Atlas heading into Saturn's shadow at upper left. The moon's basic, elongated shape is easy to detect here. |
| Full Description |
This strikingly crisp view shows Atlas heading into Saturn's shadow at upper left. The moon's basic, elongated shape is easy to detect here. (See Watching Atlas's Waistline for a different perspective on Atlas.) Above Atlas (32 kilometers, or 20 miles across) in the image, a bright clump in the F ring also heads toward the darkness. This view looks toward the unlit side of the rings from about 30 degrees above the ringplane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Jan. 19, 2007 at a distance of approximately 1.2 million kilometers (700,000 miles) from Atlas. Image scale is 7 kilometers (4 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
March 1, 2007 |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098665.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 1,790,834 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098666.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 1,790,832 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098680.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 2,049,337 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
W00040047.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 2,048,571 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
W00040039.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 1,790,832 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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Atlas and the F Ring
| Description |
The Cassini spacecraft gazes toward the multiple strands of the ever-changing F ring, also sighting Atlas at its station just beyond the A ring edge. |
| Full Description |
The Cassini spacecraft gazes toward the multiple strands of the ever-changing F ring, also sighting Atlas at its station just beyond the A ring edge. A few faint background stars are visible in the image. Atlas, which appears left of center, is 32 kilometers (20 miles across). This view looks toward the unlit side of the rings from about 58 degrees above the ringplane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Feb. 10, 2007 at a distance of approximately 1.7 million kilometers (1.1 million miles) from Atlas and at a Sun-Atlas-spacecraft, or phase, angle of 128 degrees. Image scale is 10 kilometers (6 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
March 29, 2007 |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098681.jpg was taken on December 07, 2007 and received on Earth December 08, 2007. The camera was pointing toward ATLAS at approximately 2,048,571 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098682.jpg was taken on December 08, 2007 and received on Earth December 09, 2007. The camera was pointing toward ATLAS at approximately 2,203,740 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
W00040082.jpg was taken on December 08, 2007 and received on Earth December 09, 2007. The camera was pointing toward ATLAS at approximately 2,203,863 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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Emergent Moons
| Description |
Emergent Moons |
| Full Description |
Atlas and Pan emerge from the far side of Saturn. Light passing through the upper reaches of the planet''s atmosphere is refracted, or bent, distorting the image of the rings beyond. Pan (26 kilometers, or 16 miles across) is seen within the Encke Gap. Atlas (32 kilometers, or 20 miles across) orbits just beyond the outer edge of Saturn''s A ring. This view looks toward the unilluminated side of the rings from about 12 degrees above the ringplane. Shadows cast by the rings arc across the planet toward the Cassini spacecraft. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 12, 2007 at a distance of approximately 1.6 million kilometers (1 million miles) from Saturn. Image scale is 10 kilometers (6 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
May 23, 2007 |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098683.jpg was taken on December 08, 2007 and received on Earth December 09, 2007. The camera was pointing toward ATLAS at approximately 2,203,863 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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Ring Moon Rendezvous
| Description |
Ring Moon Rendezvous |
| Full Description |
Across the expanse of Saturn's rings, the Cassini spacecraft spies two small moons in consort. Atlas (32 kilometers, or 20 miles across) is seen exterior to the bright outer edge of the A ring. Daphnis (7 kilometers, or 4.3 miles across), below Atlas in this view, orbits Saturn within the narrow Keeler Gap. The presence of Daphnis is revealed by the waves it raises in the ring material surrounding it on the edges of the gap. Daphnis and its waves moved between exposures taken to create this color view, resulting in their slight displacement in each color. This view looks toward the unilluminated side of the rings from about 18 degrees above the ringplane. Bright clumps are visible in the narrow F ring. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow-angle camera on April 13, 2007 at a distance of approximately 1.8 million kilometers (1.1 million miles) from Atlas. Image scale is 11 kilometers (7 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
May 16, 2007 |
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In-between Moon
| Description |
In-between Moon |
| Full Description |
A small icy world plies the space between Saturn's A and F rings. Atlas (32 kilometers, or 20 miles across) is seen here, along with clumps of material in the F ring. This view looks toward the unilluminated side of the rings from about 13 degrees above the ringplane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 29, 2007 at a distance of approximately 1.8 million kilometers (1.1 million miles) from Atlas. Image scale is 11 kilometers (7 miles) per pixel. 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 . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
June 7, 2007 |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098733.jpg was taken on December 12, 2007 and received on Earth December 13, 2007. The camera was pointing toward ATLAS at approximately 2,312,080 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
N00098732.jpg was taken on December 12, 2007 and received on Earth December 13, 2007. The camera was pointing toward ATLAS at approximately 2,312,083 kilometers away, and the image was taken using the CL1 and CL2 filters. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2008. For more information on raw images check out our frequently asked questions section. Image Credit: NASA/JPL/Space Science Institute |
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