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Images of 'NASA' found, 8,712

 
Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

PIX4619146

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

PIX4619146

 
Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

PIX4622792

Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

PIX4622792

 
Neptune seen by Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 20, 1989. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. In this photo, in the centre, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, on the left, a small cloud of irregular shape moving very quickly, nicknamed the scooter

PIX4622802

Neptune seen by Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 20, 1989. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. In this photo, in the centre, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, on the left, a small cloud of irregular shape moving very quickly, nicknamed the scooter

PIX4622802

 
Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

PIX4623115

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

PIX4623115

 
Ireland seen by satellite Terra - Ireland satellite view - Image obtained on 4 January 2003. True - color Moderate Resolution Imaging Spectroradiometer (MODIS) image of Ireland taken from Terra satellite on January 4, 2003. The rugged cliffs that mark the island's west coast are showing their red - brown rocky surface, but the low - lying interior region is still wearing the island's signature green. The highest elevation in Ireland is Carrantuohill, located in the rugged terrain of the southwest tip. The bowl - like shape creates the network of lakes scattered across the island, and over time has produced peat bogs, which provide a source of fuel on the island, which is covered mostly by pasture and meadows. Ireland's largest city, Dublin, makes a purplish - gray patch peeking out from the clouds about halfway down the east coast. Belfast is more clearly visible on the coast in the northeast, due east of large Lake Neagh. One Ireland's few other large cities, Cork, is located at the m

PIX4666158

Ireland seen by satellite Terra - Ireland satellite view - Image obtained on 4 January 2003. True - color Moderate Resolution Imaging Spectroradiometer (MODIS) image of Ireland taken from Terra satellite on January 4, 2003. The rugged cliffs that mark the island's west coast are showing their red - brown rocky surface, but the low - lying interior region is still wearing the island's signature green. The highest elevation in Ireland is Carrantuohill, located in the rugged terrain of the southwest tip. The bowl - like shape creates the network of lakes scattered across the island, and over time has produced peat bogs, which provide a source of fuel on the island, which is covered mostly by pasture and meadows. Ireland's largest city, Dublin, makes a purplish - gray patch peeking out from the clouds about halfway down the east coast. Belfast is more clearly visible on the coast in the northeast, due east of large Lake Neagh. One Ireland's few other large cities, Cork, is located at the m

PIX4666158

 
France seen by the Terra satellite - France as seen by the Terra satellit

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France seen by the Terra satellite - France as seen by the Terra satellit

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North pole by satellite - September 9, 2008 - Arctic sea ice - September 9, 2008 - Arctic ice coverage September 9, 2008. Image based on data obtained by the Aqua satellite. This image shows the sea ice that occurred on September 9, 2008. Sea ice is frozen seawater floating on the surface of the ocean. Some sea ice is semi-permanent, persisting from year to year, and some is seasonal, melting and refreezing from season to season. The sea ice cover reaches its minimum extent at the end of each summer and the remaining ice is called the perennial ice cover. Image made from Aqua satellite instrument

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North pole by satellite - September 9, 2008 - Arctic sea ice - September 9, 2008 - Arctic ice coverage September 9, 2008. Image based on data obtained by the Aqua satellite. This image shows the sea ice that occurred on September 9, 2008. Sea ice is frozen seawater floating on the surface of the ocean. Some sea ice is semi-permanent, persisting from year to year, and some is seasonal, melting and refreezing from season to season. The sea ice cover reaches its minimum extent at the end of each summer and the remaining ice is called the perennial ice cover. Image made from Aqua satellite instrument

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New York view from space - New York City seen from space - New York, with Manhattan Island in the center of the image, seen by Terra satellite on 8 September 2002. This image taken by satellite Terra shows New York City and the Island of Manhattan, bordered by the Hudson and East Rivers. Parts of Long Island and Staten Island are also visible. Two of New York's major airports (Newark and La Guardia) are within the image. In the middle of Manhattan, Central Park appears as a long green rectangle with a large lake in the middle. The image covers an area of 27 x 37 km, and was acquired September 8, 2002, and is located at 40.7 degrees north latitude and 74 degrees west longitude

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New York view from space - New York City seen from space - New York, with Manhattan Island in the center of the image, seen by Terra satellite on 8 September 2002. This image taken by satellite Terra shows New York City and the Island of Manhattan, bordered by the Hudson and East Rivers. Parts of Long Island and Staten Island are also visible. Two of New York's major airports (Newark and La Guardia) are within the image. In the middle of Manhattan, Central Park appears as a long green rectangle with a large lake in the middle. The image covers an area of 27 x 37 km, and was acquired September 8, 2002, and is located at 40.7 degrees north latitude and 74 degrees west longitude

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Urangan Irene - August 26, 2011 - Hurricane Irene - August 26, 2011 - Hurricane Irene on the eastern coast of the United States seen by the GOES-13 meteorological satellite on August 26, 2011. Irene, the first hurricane of the 2011 Atlantic season, was poised on August 26 to be the first to make landfall in the United States since 2008. More than 50 million people were estimated to lie within the path of the storm as it headed towards the major U.S. population centers of Norfolk, Washington, Baltimore, Philadelphia, New York, and Boston

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Urangan Irene - August 26, 2011 - Hurricane Irene - August 26, 2011 - Hurricane Irene on the eastern coast of the United States seen by the GOES-13 meteorological satellite on August 26, 2011. Irene, the first hurricane of the 2011 Atlantic season, was poised on August 26 to be the first to make landfall in the United States since 2008. More than 50 million people were estimated to lie within the path of the storm as it headed towards the major U.S. population centers of Norfolk, Washington, Baltimore, Philadelphia, New York, and Boston

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Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

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Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

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Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

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Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

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Saturn and satellites seen by Voyager - Saturn system montage - Mounting made from the photos obtained by the Voyager 1 and 2 probes showing Saturn accompanied by its satellites. Enceladus is the largest satellite on the image, then clockwise we find Dione, Rhea, Titan (top right), Japet, Tethys, and Mimas. This montage of images of the Saturnian system was prepared from an assemblage of images taken by the Voyager 1 and 2 spacecrafts during their Saturn encounter. The large satellite at left is Enceladus, followed in clockwise order by Dione, Rhea, Titan (in top right corner), Iapetus, Tethys, & Mimas

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Saturn and satellites seen by Voyager - Saturn system montage - Mounting made from the photos obtained by the Voyager 1 and 2 probes showing Saturn accompanied by its satellites. Enceladus is the largest satellite on the image, then clockwise we find Dione, Rhea, Titan (top right), Japet, Tethys, and Mimas. This montage of images of the Saturnian system was prepared from an assemblage of images taken by the Voyager 1 and 2 spacecrafts during their Saturn encounter. The large satellite at left is Enceladus, followed in clockwise order by Dione, Rhea, Titan (in top right corner), Iapetus, Tethys, & Mimas

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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Syvach Lagoons (Sivash Lagoons), Crimea (photo)

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Syvach Lagoons (Sivash Lagoons), Crimea (photo)

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Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

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Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

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Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

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Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

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Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

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Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

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Active galaxy NGC 1068 in the Whale - Composite X - visible - Active galaxy NGC 1068 seen in visible and X - ray - This visible X composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068. This active galaxy houses a massive black hole and is the object of intense star formation in its spiral arms. NGC 1068 stands at about 50 million years - light. Image obtained by the Chandra satellite in December 2000. This composite X - ray (blue and green) and optical (red) image of the active galaxy, NGC 1068, shows gas blowing away in a high - speed wind from the vicinity of a central supermassive black hole. Regions of intense star formation in the inner spiral arms of the galaxy are highlighted by both optical and X - ray emission

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Active galaxy NGC 1068 in the Whale - Composite X - visible - Active galaxy NGC 1068 seen in visible and X - ray - This visible X composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068. This active galaxy houses a massive black hole and is the object of intense star formation in its spiral arms. NGC 1068 stands at about 50 million years - light. Image obtained by the Chandra satellite in December 2000. This composite X - ray (blue and green) and optical (red) image of the active galaxy, NGC 1068, shows gas blowing away in a high - speed wind from the vicinity of a central supermassive black hole. Regions of intense star formation in the inner spiral arms of the galaxy are highlighted by both optical and X - ray emission

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Elliptical Galaxy M60 in Virgo - Elliptical galaxy M60 in Virgo - M60 (NGC 4649) is an elliptical galaxy of type E2 located about 51 million years ago - light from Earth in the Virgin's cluster. This image is a composite of X-ray images (purple) obtained by the Chandra Space Telescope, and visible (blue) by the Hubble Space Telescope. This galaxy houses a supermassive black hole. Elliptical galaxy M60 (NGC 4649) located about 51 million light - years away in the Virgo cluster of galaxies. This image is a composite of X - ray image (in purple) taken by Chandra space telescope and optical image (blue) taken by Hubble space telescope. NGC 4649 contains one of the biggest black hole of our local universe

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Elliptical Galaxy M60 in Virgo - Elliptical galaxy M60 in Virgo - M60 (NGC 4649) is an elliptical galaxy of type E2 located about 51 million years ago - light from Earth in the Virgin's cluster. This image is a composite of X-ray images (purple) obtained by the Chandra Space Telescope, and visible (blue) by the Hubble Space Telescope. This galaxy houses a supermassive black hole. Elliptical galaxy M60 (NGC 4649) located about 51 million light - years away in the Virgo cluster of galaxies. This image is a composite of X - ray image (in purple) taken by Chandra space telescope and optical image (blue) taken by Hubble space telescope. NGC 4649 contains one of the biggest black hole of our local universe

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Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

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Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

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Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

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Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

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Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

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Manicouagan impact crater seen by Landsat satellite

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Manicouagan impact crater seen by Landsat satellite

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