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'Nasa's Dawn' images and/or videos results

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Images of 'Nasa's Dawn' found, 22

 
This image, taken by the framing camera instrument aboard NASA's Dawn spacecraft, shows the south polar region of this object, which has a diameter of 330 miles (530 kilometers). The image was taken through the clear filter on July 9, 2011, as part of a rotation characterization sequence, and it has a scale of about 2.2 miles (3.5 kilometers) per pixel. To enhance details, the resolution was enlarged to .6 miles (1 kilometer) per pixel. This region is characterized by rough topography, a large mountain, impact craters, grooves and steep scarps. The original image was map-projected, centered at 55 degrees southern latitude and 210 degrees eastern longitude.

UIG866225

This image, taken by the framing camera instrument aboard NASA's Dawn spacecraft, shows the south polar region of this object, which has a diameter of 330 miles (530 kilometers). The image was taken through the clear filter on July 9, 2011, as part of a rotation characterization sequence, and it has a scale of about 2.2 miles (3.5 kilometers) per pixel. To enhance details, the resolution was enlarged to .6 miles (1 kilometer) per pixel. This region is characterized by rough topography, a large mountain, impact craters, grooves and steep scarps. The original image was map-projected, centered at 55 degrees southern latitude and 210 degrees eastern longitude.

UIG866225

 
This image from NASA's Dawn mission reveals the creeping dawn over the north pole of the giant asteroid Vesta now that sunlight is shining over that area. The mosaic is composed of 5 images obtained by Dawn's framing camera on Aug.26, 2012, while Dawn was at an altitude of about 4,000 miles (6,000 kilometers). Dawn's north pole is centered in this image and still in the dark. The mosaic shows two large impact craters, one relatively fresh with no smaller impacts on its floor and a second larger and older one with many smaller impacts on its floor.

UIG866673

This image from NASA's Dawn mission reveals the creeping dawn over the north pole of the giant asteroid Vesta now that sunlight is shining over that area. The mosaic is composed of 5 images obtained by Dawn's framing camera on Aug.26, 2012, while Dawn was at an altitude of about 4,000 miles (6,000 kilometers). Dawn's north pole is centered in this image and still in the dark. The mosaic shows two large impact craters, one relatively fresh with no smaller impacts on its floor and a second larger and older one with many smaller impacts on its floor.

UIG866673

 
This Dawn framing camera (FC) image of the Asteroid Vesta, shows the Arruntia crater, which is the large crater offset to the top right of the center of the image. Slightly over half of Arruntia crater is covered in a large shadow. But, the non-shadowed part of Arruntia shows impressive details. There is bright material cropping out slightly below the left rim and just below the top and bottom rims there are distinct ridges of material, which are probably formed by material from the rim cascading down towards the center of Arruntia. This image is located in Vesta's Bellicia quadrangle, in Vesta's northern hemisphere. NASA's Dawn spacecraft obtained this image with its framing camera on Oct. 24, 2011.

UIG866402

This Dawn framing camera (FC) image of the Asteroid Vesta, shows the Arruntia crater, which is the large crater offset to the top right of the center of the image. Slightly over half of Arruntia crater is covered in a large shadow. But, the non-shadowed part of Arruntia shows impressive details. There is bright material cropping out slightly below the left rim and just below the top and bottom rims there are distinct ridges of material, which are probably formed by material from the rim cascading down towards the center of Arruntia. This image is located in Vesta's Bellicia quadrangle, in Vesta's northern hemisphere. NASA's Dawn spacecraft obtained this image with its framing camera on Oct. 24, 2011.

UIG866402

 
This Dawn framing camera (FC) image of steroid Vesta shows Fabia crater, which is the large crater offset to the bottom right of the center of the image. Fabia crater is very distinctive because the two sides of its rim have very different states of freshness. In this image the bottom part of the rim is distinct and fresh but the top part of the rim is much more rounded and degraded. This image is located in Vesta's Numisia quadrangle, in Vesta's northern hemisphere. NASA's Dawn spacecraft obtained this image with its framing camera on Oct. 19, 2011.

UIG866487

This Dawn framing camera (FC) image of steroid Vesta shows Fabia crater, which is the large crater offset to the bottom right of the center of the image. Fabia crater is very distinctive because the two sides of its rim have very different states of freshness. In this image the bottom part of the rim is distinct and fresh but the top part of the rim is much more rounded and degraded. This image is located in Vesta's Numisia quadrangle, in Vesta's northern hemisphere. NASA's Dawn spacecraft obtained this image with its framing camera on Oct. 19, 2011.

UIG866487

 
This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

UIG866227

This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

UIG866227

 
This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

UIG866228

This image from NASA's Dawn mission shows the topography of the northern and southern hemispheres of the giant asteroid Vesta, updated with pictures obtained during Dawn's last look back. Around the time of Dawn's departure from Vesta in the late summer of 2012, dawn was beginning to creep over the high northern latitudes, which were dark when Dawn arrived in the summer of 2011. The three craters that make up Dawn's "snowman" feature can be seen at the top of the northern hemisphere map on the left. A mountain more than twice the height of Mount Everest, inside the largest impact basin on Vesta, can be seen near the center of the southern hemisphere map on the right.

UIG866228

 
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The Dawn probe near Vesta - Artist's view: Artist's view of the Dawn probe near the Vesta asteroid. On 16 July 2011 the probe went into orbit around Vesta and collected data that significantly improved our knowledge of asteroid. After studying Vesta for more than a year, the probe left on 5 September 2012 to reach the dwarf planet Ceres. Artist's concept of the Dawn spacecraft with asteroid Vesta. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta (2011-2012) and the dwarf planet Ceres (2015).

Miller, Ron (b.1947)

PIX4643719

The Dawn probe near Vesta - Artist's view: Artist's view of the Dawn probe near the Vesta asteroid. On 16 July 2011 the probe went into orbit around Vesta and collected data that significantly improved our knowledge of asteroid. After studying Vesta for more than a year, the probe left on 5 September 2012 to reach the dwarf planet Ceres. Artist's concept of the Dawn spacecraft with asteroid Vesta. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta (2011-2012) and the dwarf planet Ceres (2015).

Miller, Ron (b.1947)

PIX4643719

 
The Dwarf Planet Ceres seen by the Dawn probe - Dwarf Planet Ceres: Image reconstructed in very high resolution from observations made by the Dawn probe, showing the dwarf planet Ceres with the occator crater in the center. This orthographic projection shows dwarf planet Ceres as seen by Nasa's Dawn spacecraft. The projection is centered on Occator Crater, home to the brightest area on Ceres. Occator is centered at 20 degrees north latitude, 239 degrees east longitude. This image was made from views Dawn took during its low-altitude mapping orbit, at about 240 miles (385 kilometers) above the surface. The image resolution is about 120 feet (35 meters) per pixel

PIX4583550

The Dwarf Planet Ceres seen by the Dawn probe - Dwarf Planet Ceres: Image reconstructed in very high resolution from observations made by the Dawn probe, showing the dwarf planet Ceres with the occator crater in the center. This orthographic projection shows dwarf planet Ceres as seen by Nasa's Dawn spacecraft. The projection is centered on Occator Crater, home to the brightest area on Ceres. Occator is centered at 20 degrees north latitude, 239 degrees east longitude. This image was made from views Dawn took during its low-altitude mapping orbit, at about 240 miles (385 kilometers) above the surface. The image resolution is about 120 feet (35 meters) per pixel

PIX4583550

 
Dawn and Vesta and Ceres - Artist's concept of the Dawn spacecraft with Vesta and Ceres - Artist's view of the Dawn probe near the Vesta asteroid and the dwarf planet Ceres Artist's concept of the Dawn spacecraft with Vesta and Ceres. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta and the dwarf planet Ceres. The two bodies have very different properties from each other. By observing them both with the same set of instruments, Dawn will probe the early solar system and specify the properties of each body

PIX4607287

Dawn and Vesta and Ceres - Artist's concept of the Dawn spacecraft with Vesta and Ceres - Artist's view of the Dawn probe near the Vesta asteroid and the dwarf planet Ceres Artist's concept of the Dawn spacecraft with Vesta and Ceres. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta and the dwarf planet Ceres. The two bodies have very different properties from each other. By observing them both with the same set of instruments, Dawn will probe the early solar system and specify the properties of each body

PIX4607287

 
Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

PIX4625211

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

PIX4625211

 
Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605150

Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605150

 
Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft rises from the smoke and fire on the launch pad to begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605145

Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft rises from the smoke and fire on the launch pad to begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605145

 
Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft rises from the smoke and fire on the launch pad to begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605138

Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft rises from the smoke and fire on the launch pad to begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605138

 
Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649404

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649404

 
Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649419

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649419

 
Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649416

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649416

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