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Apollo17 - On the Shoulders
…
APOLLO 17: ON THE SHOULDERS
…
1973
| Title |
Apollo17 - On the Shoulders of_Giants |
| Description |
APOLLO 17: ON THE SHOULDERS OF GIANTS JSC 603 - (1973) - 28 1/2 Minutes Astronauts: Eugene A. Cernan, Ronald E. Evans, and Harrison H. Schmitt Launch date: December 7, 1972 A documentary view of the Apollo 17 journey to Taurus-Littrow, the final lunar landing mission in the Apollo Program. The film depicts the highlights of the mission and relates the Apollo Program to Skylab, the Apollo-Soyuz linkup, and the Space Shuttle. AWARDS: Chris Bronze Plaque Award, 21st Annual Columbus Film Festival, 1983 * Trophy of the Italian Department of Defense * 1st International Review of Cinema and TV Films on Flight, Milan, Italy, 1974 * Special Prize, 11th International Review of Technical, Scientific, and Educational Films, Pardubice, Czechoslovakia, 1973 |
| Date |
1973 |
|
Reporting to the Launch Pad
The payload fairing carrying
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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 |
|
The Upper Stack
Just before dawn on Launch C
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2/19/09
| Description |
Just before dawn on Launch Complex 576-E at Vandenberg Air Force Base in California, a crane lifts the tent covering (at left) NASA's Orbiting Carbon Observatory, or OCO, the Taurus XL upper stack and the umbilical tower. The tent removal will allow OCO to be hoisted into place atop the Taurus rocket's Stage 0. Image credit: NASA/Randy Beaudoin Feb. 18, 2009 |
| Date |
2/19/09 |
|
All Stacked Up
On Launch Complex 576-E at V
…
2/19/09
| Description |
On Launch Complex 576-E at Vandenberg Air Force Base in California, NASA's Orbiting Carbon Observatory, OCO, upper stack is lowered toward the Stage 0 motor of the Taurus XL vehicle. The upper stack consists of Stages 1, 2 and 3 of the Taurus. Image credit: NASA/Randy Beaudoin Feb. 18, 2009 |
| Date |
2/19/09 |
|
Waiting for a Lift
Workers prepare NASA's Orbit
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2/19/09
| Description |
Workers prepare NASA's Orbiting Carbon Observatory upper stack for attachment to the umbilical tower above. The umbilical tower will be erected on the pad. The upper stack consists of Stages 1, 2 and 3 of the Taurus. Image credit: NASA/Randy Beaudoin Feb. 18, 2009 |
| Date |
2/19/09 |
|
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 |
|
At the Ready
On Launch Complex 576-E at V
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2/20/09
| Description |
On Launch Complex 576-E at Vandenberg Air Force Base in California, NASA's Orbiting Carbon Observatory, or OCO, has been erected atop Orbital Sciences' Taurus XL rocket for launch. Image credit: NASA/Randy Beaudoin Feb. 19, 2009 |
| Date |
2/20/09 |
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Sunset Silhouette
A sunset silhouette of the T
…
2/24/09
| Description |
A sunset silhouette of the Taurus XL rocket with NASA's OCO satellite aboard sits poised for launch on Launch Complex 576-E at Vandenberg Air Force Base in California.</br></br> Image credit: NASA/Analex Randy Beaudoin</br> Feb. 23, 2009 |
| Date |
2/24/09 |
|
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 |
|
Apollo17 - On the Shoulders
…
APOLLO 17: ON THE SHOULDERS
…
1973
| Description |
APOLLO 17: ON THE SHOULDERS OF GIANTS JSC 603 - (1973) - 28 1/2 Minutes Astronauts: Eugene A. Cernan, Ronald E. Evans, and Harrison H. Schmitt Launch date: December 7, 1972 A documentary view of the Apollo 17 journey to Taurus-Littrow, the final lunar landing mission in the Apollo Program. The film depicts the highlights of the mission and relates the Apollo Program to Skylab, the Apollo-Soyuz linkup, and the Space Shuttle. AWARDS: Chris Bronze Plaque Award, 21st Annual Columbus Film Festival, 1983 * Trophy of the Italian Department of Defense * 1st International Review of Cinema and TV Films on Flight, Milan, Italy, 1974 * Special Prize, 11th International Review of Technical, Scientific, and Educational Films, Pardubice, Czechoslovakia, 1973 |
| Date |
1973 |
|
Apollo -- December 1972
Scientist-astronaut Harrison
…
7/16/08
| Description |
Scientist-astronaut Harrison H. Schmitt, Apollo 17 lunar module pilot, collects lunar rake samples at Station 1 during the mission's first spacewalk at the Taurus-Littrow landing site. This picture was taken by astronaut Eugene A. Cernan, commander. The lunar rake, an Apollo lunar geology hand tool, is used to collect discrete samples of rocks and rock chips ranging in size from one-half inch (1.3 centimeters) to 1 inch (2.5 centimeters). |
| Date |
7/16/08 |
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The Versatile Taurus
The four-stage Taurus rocket
…
2/18/09
| Title |
The Versatile Taurus |
| Date |
2/18/09 |
| Description |
The four-stage Taurus rocket is designed to be cost-effective, adaptable and dependable. |
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Taurus is OCO's Ride to Spac
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The four-stage Taurus rocket
…
2/23/09
| Title |
Taurus is OCO's Ride to Space |
| Date |
2/23/09 |
| Description |
The four-stage Taurus rocket is set to launch. |
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Crab Nebula Supernova Remnan
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| Title |
Crab Nebula Supernova Remnant (IRAC-MIPS Image) |
| Description |
The Crab Nebula is the shattered remnant of a massive star that ended its life in a massive supernova explosion. Nearly a thousand years old, the supernova was noted in the constellation of Taurus by Chinese astronomers in the year 1054 AD. This view of the supernova remnant obtained by the Spitzer Space Telescope shows the infrared view of this complex object. The blue region traces the cloud of energetic electrons trapped within the star's magnetic field, emitting so-called "synchrotron" radiation. The yellow-red features follow the well-known filamentary structures that permeate this nebula. Though they are known to contain hot gasses, their exact nature is still a mystery that astronomers are examining. The energetic cloud of electrons are driven by a rapidly rotating neutron star, or pulsar, at its core. The nebula is about 6,500 light-years away from the Earth, and is 5 light-years across. This false-color image presents images from Spitzer's Infrared Array Camera (IRAC) and Multiband Imaging Photometer (MIPS) at 3.6 (blue), 8.0 (green), 24 (red) microns. |
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Crab Nebula Supernova Remnan
…
| Title |
Crab Nebula Supernova Remnant (IRAC Image) |
| Description |
The Crab Nebula is the shattered remnant of a massive star that ended its life in a massive supernova explosion. Nearly a thousand years old, the supernova was noted in the constellation of Taurus by Chinese astronomers in the year 1054 AD. This view of the supernova remnant obtained by the Spitzer Space Telescope shows the infrared view of this complex object. The blue-white region traces the cloud of energetic electrons trapped within the star's magnetic field, emitting so-called "synchrotron" radiation. The red features follow the well-known filamentary structures that permeate this nebula. Though they are known to contain hot gasses, their exact nature is still a mystery that astronomers are examining. The energetic cloud of electrons are driven by a rapidly rotating neutron star, or pulsar, at its core. The nebula is about 6,500 light-years away from the Earth, and is 5 light-years across. This false-color image presents images from Spitzer's Infrared Array Camera (IRAC) at 3.6 (blue), 4.5 (green), and 8.0 (red) microns. |
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The Spirit of Halloween Live
…
| Title |
The Spirit of Halloween Lives On as a Dead Star Creates Celestial Havoc |
| Description |
According to the folklore of the Celts and other ancient cultures, Halloween marked the midpoint between the autumnal equinox and the winter solstice on the astronomical calendar, a spooky night when spirits of the dead spread havoc upon their return to Earth. Nowadays, Halloween is primarily a time for children to dress in costume and demand treats, but the original spirit of Halloween lives on in the sky in the guise of the Crab Nebula. 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. |
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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. |
|
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. |
|
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. |
|
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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Forming a Planetary Gap
| Title |
Forming a Planetary Gap |
| Description |
Astronomers are using NASA's Spitzer Space Telescope to probe the structures of circumstellar discs, the dusty discs that surround young stars, to look for the earliest signs of the formation of planetary systems. Examining young stars in the constellation of Taurus known to have such discs, Spitzer's ultra-sensitive infrared spectrograph instrument has detected the clearest evidence to date that an inner gap has formed in the disc surrounding the star CoKu Tau 4. Such a gap could indicate the presence of a new planet that has formed from the missing material. This animation illustrates one possible scenario for the formation of an inner gap. Initially we see the circumstellar disc around a young star, made of the dust, ices and gases from which planets might form. As we move in to view the inner disc, an unstable ripple forms in the inner part of the disc. The force of gravity acts upon this ripple, allowing the material to rapidly condense into a new planet. The innermost portions of the disc that did not condense onto the planet rapidly spiral in and accrete onto the star, adding a little more to its final mass. |
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Icy Organics in Planet-Formi
…
| Title |
Icy Organics in Planet-Forming Discs |
| Description |
Using the Spitzer Space Telescope, astronomers are probing the chemistry of circumstellar discs, the dusty discs that surround stars, to understand the first moments in planetary life. Spitzer has turned its ultra-sensitive infrared spectrograph instrument toward five young stars in the constellation Taurus. These stars are still surrounded by thick, dusty discs -- relics of the gravitational collapse that formed them only a few million years ago. The five discs have similar chemistry, indicating dusty material rich in silicates and organic compounds, as well as both water and carbon dioxide ices. Despite their similarities, there are also intriguing differences between the discs that may hold important clues about the evolution of stars and their young planetary systems. In this animation, we focus on the disc of a young star. Light from the star is almost completely blocked by the thick dust and is seen only when it scatters off dust and gas above the disc plane. Delving in closer, we observe that the disc is composed of countless tiny grains of dust, some of which, according to Spitzer observations, have crystal structures. These dust grains may serve as the first building blocks of new planets, accreting into larger and larger bodies, as time progresses. As a few of these crystals fill our view, a strange metamorphosis takes place. Ice, already known to be present in these discs, begins to condense onto the surface of the crystals. Over time, the grains become larger, icier and more spherical. These chemical and physical changes in the dust grains may explain the differing spectral characteristics of the discs, and may also serve as a marker of the age and evolutionary stage of protoplanetary, or planet-forming, discs. |
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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 |
|
Luna 21/Lunokhod 2
| title |
Luna 21/Lunokhod 2 |
| date |
01.08.1973 |
| description |
Luna 21 carried the second successful Soviet "8YeL" lunar rover, Lunokhod 2, and was launched less than a month after the last Apollo lunar landing. After a midcourse correction the day after launch, Luna 21 entered orbit around the Moon on 12 January 1973. Parameters were 100 x 90 kilometers at 60° inclination. On 15 January, the spacecraft deorbited and, after multiple engine firings, landed on the Moon at 22:35 UT the same day, inside the LeMonnier crater at 25°51' north latitude and 30°27' east longitude, between Mare Serenitatis and the Taurus Mountains. Less than 3 hours later, at 01:14 UT on 16 January, the rover disembarked onto the lunar surface. The 840-kilogram Lunokhod 2 was an improved version of its predecessor and was equipped with a third TV camera, an improved eight-wheel traction system, and additional scientific instrumentation. By the end of its first lunar day, Lunokhod 2 had already traveled further than Lunokhod 1 in its entire operational life. On 9 May, the rover inadvertently rolled into a crater and dust covered its solar panels, disrupting temperatures in the vehicle. Attempts to save the rover failed, and on 3 June, the Soviet news agency announced that its mission was over. Before last contact, the rover took 80,000 TV pictures and 86 panoramic photos and had performed hundreds of mechanical and chemical surveys of the soil. The Soviets later revealed that during a conference on planetary exploration in Moscow, 29 January to 2 February 1973 (that is, after the landing of Luna 21), an American scientist had given photos of the lunar surface around the Luna 21 landing site to a Soviet engineer in charge of the Lunokhod 2 mission. These photos, taken prior to the Apollo 17 landing, were later used by the "driver team" to navigate the new rover on its mission on the Moon. |
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Crab Nebula
| Name |
Crab Nebula |
| Category |
Supernovas & Supernova Remnants, Neutron Stars/X-ray Binaries |
| Release Date |
September 28, 1999 |
|
Supernova SN1999em:
| Name |
Supernova SN1999em: |
| Category |
Supernovas & Supernova Remnants |
| Release Date |
December 14, 1999 |
|
Crab Nebula Movie: Space Mov
…
| Name |
Crab Nebula Movie: Space Movie Reveals Shocking Secrets of the Crab Pulsar |
| Category |
Supernovas & Supernova Remnants |
| Release Date |
September 19, 2002 |
|
V471 Tauri: Star Shows It Ha
…
| Name |
V471 Tauri: Star Shows It Has the Right Stuff |
| Category |
Normal Stars & White Dwarf Stars |
| Release Date |
January 30, 2004 |
|
Crab Nebula: The Spirit of H
…
| Name |
Crab Nebula: The Spirit of Halloween Lives on as a Dead Star Creates Celestial Havoc |
| Category |
Supernovas & Supernova Remnants, Neutron Stars/X-ray Binaries |
| Release Date |
October 24, 2006 |
|
Lunarama
| Title |
Lunarama |
| Full Description |
An extraordinary lunar panorama at Station 4 (Shorty Crater) showing Geologist-Astronaut Harrison H. Schmitt working at the Lunar Roving Vehicle (LRV) during the second Apollo 17 extravehicular activity (EVA-2) at the Taurus-Littrow landing site. This is the area where Schmitt first spotted the orange soil. Shorty Crater is to the right. The peak in the center background is Family Mountain. A portion of South Massif is on the horizon at the left edge. |
| Date |
12/12/1972 |
| NASA Center |
Johnson Space Center |
|
Apollo 17 Prime Crew
| Title |
Apollo 17 Prime Crew |
| Full Description |
The prime crew for the Apollo 17 lunar landing mission are: Commander, Eugene A. Cernan (seated), Command Module pilot Ronald E. Evans (standing on right), and Lunar Module pilot, Harrison H. Schmitt. They are photographed with a Lunar Roving Vehicle (LRV) trainer. Cernan and Schmitt will use an LRV during their exploration of the Taurus-Littrow landing site. The Apollo 17 Saturn V Moon rocket is in the background. This picture was taken at Pad A, Launch Complex 39, Kennedy Space Center (KSC), Florida, The Apollo 17 emblem is in the photo insert at upper left. |
| Date |
09/30/1971 |
| NASA Center |
Johnson Space Center |
|
Orange Soil Discovery
| Title |
Orange Soil Discovery |
| Full Description |
A view of the area at Station 4 (Shorty Crater) showing the highly- publicized orange soil which the Apollo 17 crewmen found on the Moon during the second Apollo 17 extravehicular activity (EVA-2) at the Taurus-Littrow landing site. The tripod-like object is the gnomon and photometric chart assembly which is used as a photographic reference to establish local vertical Sun angle, scale and lunar color. The Gnomon is one of the Apollo lunar geology hand tools. |
| Date |
12/12/1972 |
| NASA Center |
Johnson Space Center |
|
Cernan Driving the Rover
| Title |
Cernan Driving the Rover |
| Full Description |
Astronaut Eugene A. Cernan, Apollo 17 mission commander, makes a short checkout of the Lunar Roving Vehicle during the early part of the first Apollo 17 extravehicular activity (EVA-1) at the Taurus-Littrow landing site. This view of the "stripped down" Rover is prior to loadup. This photograph was taken by Geologist-Astronaut Harrison H. Schmitt, Lunar Module pilot. The mountain in the right background is the East end of South Massif. |
| Date |
12/10/1972 |
| NASA Center |
Johnson Space Center |
|
Cernan Jump Salutes Flag
| Title |
Cernan Jump Salutes Flag |
| Full Description |
Eugene A. Cernan, Commander, Apollo 17 salutes the flag on the lunar surface during extravehicular activity (EVA) on NASA's final lunar landing mission. The Lunar Module "Challenger" is in the left background behind the flag and the Lunar Roving Vehicle (LRV) also in background behind him. While astronauts Cernan and Schmitt descended in the Challenger to explore the Taurus-Littrow region of the Moon, astronaut Ronald E. Evans, Command Module pilot, remained with the Command/Service Module (CSM) "America" in lunar-orbit. |
| Date |
12/13/1972 |
| NASA Center |
Johnson Space Center |
|
Replica of Plaque Left on Mo
…
| Title |
Replica of Plaque Left on Moon by Apollo 17 Astronauts |
| Full Description |
This image is a photographic replica of the plaque that the Apollo 17 astronauts left on the Moon at the Taurus-Littrow landing site. Apollo 17 was the final lunar landing mission in NASA's Apollo program. The commemorative plaque was unveiled at the close of the third extravehicular activity (EVA-3). The plaque was made of stainless steel measuring nine by seven and five-eighths inches, and one-sixteenth inch thick. It was attached to the ladder on the landing gear strut on the descent stage of Apollo 17 Lunar Module "Challenger. |
| Date |
12/12/1972 |
| NASA Center |
Johnson Space Center |
|
Schmitt Covered with Lunar D
…
| Title |
Schmitt Covered with Lunar Dirt |
| Full Description |
Geologist-Astronaut Harrison Schmitt, Apollo 17 lunar module pilot, uses an adjustable sampling scoop to retrieve lunar samples during the second extravehicular activity (EVA-2), at Station 5 at the Taurus- Littrow landing site. The cohesive nature of the lunar soil is born out by the "dirty" appearance of Schmitt's space suit. A gnomon is atop the large rock in the foreground. The gnomon is a stadia rod mounted on a tripod, and serves as an indicator of the gravitational vector and provides accurate vertical reference and calibrated length for determining size and position of objects in near-field photographs. The color scale of blue, orange and green is used to accurately determine color for photography. The rod of it is 18 inches long. The scoop Dr. Schmitt is using is 11 3/4 inches long and is attached to a tool extension which adds a potential 30 inches of length to the scoop. The pan portion, blocked in this view, has a flat bottom, flanged on both sides with a partial cover on the top. It is used to retrieve sand, dust and lunar samples too small for the tongs. The pan and the adjusting mechanism are made of stainless steel and the handle is made of aluminum. |
| Date |
12/12/1972 |
| NASA Center |
Johnson Space Center |
|
Schmitt Next to Big Boulder
| Title |
Schmitt Next to Big Boulder |
| Full Description |
Geologist-Astronaut Harrison H. Schmitt is photographed standing next to a huge, split boulder at Station 6 on the sloping base of North Massif during the third Apollo 17 extravehicular activity (EVA-3) at the Taurus-Littrow landing site. The "Rover" Lunar Roving Vehicle (LRV) is in the left foreground. Schmitt is the Apollo 17 Lunar Module pilot. This picture was taken by Commander Eugene A. Cernan. |
| Date |
12/13/1972 |
| NASA Center |
Johnson Space Center |
|
Schmitt with Flag and Earth
…
| Title |
Schmitt with Flag and Earth Above |
| Full Description |
Geologist-Astronaut Harrison Schmitt, Apollo 17 Lunar Module pilot, is photographed next to the American Flag during extravehicular activity (EVA) of NASA's final lunar landing mission in the Apollo series. The photo was taken at the Taurus-Littrow landing site. The highest part of the flag appears to point toward our planet earth in the distant background. |
| Date |
12/13/1972 |
| NASA Center |
Johnson Space Center |
|
Shepard and Schmitt Enjoying
…
| Title |
Shepard and Schmitt Enjoying a Light Hearted Moment |
| Full Description |
Apollo 17 Lunar Module Pilot Harrison H. Schmitt shares a moment of relaxation with astronaut Alan Shepard during prelaunch suiting operations. Schmitt will explore the Moon's Taurus-Littrow region with Mission Commander Eugene A. Cernan during NASA's sixth and last manned lunar landing mission. The third crewman, Ronald E. Evans, will pilot the command module alone in lunar orbit during his crewmates' surface exploration. |
| Date |
12/6/1972 |
| NASA Center |
Kennedy Space Center |
|
Spiro Agnew Congratulates La
…
| Title |
Spiro Agnew Congratulates Launch Control After Launch of Apollo 17 |
| Full Description |
Vice President Spiro T. Agnew congratulates launch team personnel, in firing room #1 of launch control minutes after the successful launch of Apollo 17 from Complex 39-A at 12:33 am EST, December 7, 1972, with astronauts Eugene A. Cernan, Ronald E. Evans, and Harrison H. Schmitt aboard. Apollo 17, NASA's sixth and final manned lunar landing mission in the Apollo program, landed within 200 feet of the targeted point in the Taurus-Littrow landing site on the lunar surface at 2:55 pm EST on December 11, 1972. |
| Date |
12/13/1972 |
| NASA Center |
Kennedy Space Center |
|
Hubble Observes the Fire and
…
| Title |
Hubble Observes the Fire and Fury of a Stellar Birth |
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Astronomers Track Down Aster
…
| Title |
Astronomers Track Down Asteroids in Hubble Archive |
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Hubble Takes First Image of
…
| Title |
Hubble Takes First Image of a Possible Planet around Another Star and Finds a Runaway World |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope has given astronomers their first direct look at what is possibly a planet outside our solar system —, one apparently that has been ejected into deep space by its parent stars. The discovery further challenges conventional theories about the birth and evolution of planets, and offers new insights into the formation of our own solar system. Located within a star-forming region in the constellation Taurus, the object, called TMR-1C, appears to lie at the end of a strange filament of light, suggesting it has apparently been flung away from the vicinity of a newly forming pair of binary stars. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/19/text/ ] |
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Hubble Takes First Image of
…
| Title |
Hubble Takes First Image of a Possible Planet around Another Star and Finds a Runaway World |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope has given astronomers their first direct look at what is possibly a planet outside our solar system —, one apparently that has been ejected into deep space by its parent stars. The discovery further challenges conventional theories about the birth and evolution of planets, and offers new insights into the formation of our own solar system. Located within a star-forming region in the constellation Taurus, the object, called TMR-1C, appears to lie at the end of a strange filament of light, suggesting it has apparently been flung away from the vicinity of a newly forming pair of binary stars. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/19/text/ ] |
|
Hubble Takes First Image of
…
| Title |
Hubble Takes First Image of a Possible Planet around Another Star and Finds a Runaway World |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope has given astronomers their first direct look at what is possibly a planet outside our solar system —, one apparently that has been ejected into deep space by its parent stars. The discovery further challenges conventional theories about the birth and evolution of planets, and offers new insights into the formation of our own solar system. Located within a star-forming region in the constellation Taurus, the object, called TMR-1C, appears to lie at the end of a strange filament of light, suggesting it has apparently been flung away from the vicinity of a newly forming pair of binary stars. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/19/text/ ] |
|
Hubble Takes First Image of
…
| Title |
Hubble Takes First Image of a Possible Planet around Another Star and Finds a Runaway World |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope has given astronomers their first direct look at what is possibly a planet outside our solar system —, one apparently that has been ejected into deep space by its parent stars. The discovery further challenges conventional theories about the birth and evolution of planets, and offers new insights into the formation of our own solar system. Located within a star-forming region in the constellation Taurus, the object, called TMR-1C, appears to lie at the end of a strange filament of light, suggesting it has apparently been flung away from the vicinity of a newly forming pair of binary stars. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/19/text/ ] |
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Far-Flung Galaxy Clusters Ma
…
| Title |
Far-Flung Galaxy Clusters May Reveal Fate of Universe |
|
Astronomers Track Down Aster
…
| Title |
Astronomers Track Down Asteroids in Hubble Archive |
|
Hubble Takes First Image of
…
| Title |
Hubble Takes First Image of a Possible Planet around Another Star and Finds a Runaway World |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope has given astronomers their first direct look at what is possibly a planet outside our solar system —, one apparently that has been ejected into deep space by its parent stars. The discovery further challenges conventional theories about the birth and evolution of planets, and offers new insights into the formation of our own solar system. Located within a star-forming region in the constellation Taurus, the object, called TMR-1C, appears to lie at the end of a strange filament of light, suggesting it has apparently been flung away from the vicinity of a newly forming pair of binary stars. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/19/text/ ] |
|
Peering into the Heart of th
…
| Title |
Peering into the Heart of the Crab Nebula |
| General Information |
What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Back to top [ #top ] |
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