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Saturn from his satellite Dione - Illustration

Saturn from his satellite Dione - Illustration

Miller, Ron (b.1947)

PIX4625645

Saturn and satellites seen by the Cassini probe on 30/01/2008 - Saturn and satellites seen by Cassini spacecraft Jan. 30 2008 - Saturn seen by the Cassini probe on 30 January 2008 at a distance of 1.3 million km from the planet. The Tethys satellite is visible under Saturn's rings and the Titan satellite appears at the top of the picture. Titan emerges from behind Saturn, while Tethys streaks into view, in this colorful scene. Saturn's shadow darkens the far arm of the rings near the planet's limb. Titan is 5,150 kilometers (3,200 miles) wide; Tethys is 1,071 kilometers (665 miles) wide. This view looks toward the unilluminated side of the rings from about 3 degrees above the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Jan. 30, 2008 at a distance of approximately 1.3 million kilometers (800,000 miles) from Saturn. Image scale is 77 kilomete

Saturn and satellites seen by the Cassini probe on 30/01/2008 - Saturn and satellites seen by Cassini spacecraft Jan. 30 2008 - Saturn seen by the Cassini probe on 30 January 2008 at a distance of 1.3 million km from the planet. The Tethys satellite is visible under Saturn's rings and the Titan satellite appears at the top of the picture. Titan emerges from behind Saturn, while Tethys streaks into view, in this colorful scene. Saturn's shadow darkens the far arm of the rings near the planet's limb. Titan is 5,150 kilometers (3,200 miles) wide; Tethys is 1,071 kilometers (665 miles) wide. This view looks toward the unilluminated side of the rings from about 3 degrees above the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Jan. 30, 2008 at a distance of approximately 1.3 million kilometers (800,000 miles) from Saturn. Image scale is 77 kilomete

PIX4625119

Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

PIX4634712

Space satellite

Space satellite

English School, (20th century)

LAL319159

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The Tethys satellite photographed by the Cassini probe on August 30, 2007 at a distance of 97,000 km. Tethys is about 1070 km in diameter. At the top left of the picture is the gigantic impact crater Odysseus, which measures 450 km in diameter. The vast expanse of the crater Odysseus spreads out below Cassini in this mosaic view of Saturn's moon Tethys. The crater (450 kilometers or 280 miles across) is a remarkably well - preserved example of an ancient multi - ringed impact basin: the outer ring is defined by steep, cliff - like walls that descend to generally broad internal terraces. The inner ring is formed by a prominent, crown - shaped, 140 - kilometer (88 - mile) diameter circular band of icy mountains. Multi - ring basins are seen on rocky bodies as well as icy ones. The complex internal structure and multi - ringed nature of these very large basins are believed to arise from

PIX4625574

E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the e.deorbit satellite (left) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon. In

E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the e.deorbit satellite (left) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon. In

D. Ducros

PIX4605500

SPUTNIK II, launched by Russia in 1957, with dog inside.

SPUTNIK II, launched by Russia in 1957, with dog inside.

EVB2955411

Satellite view of the Earth (north America) from space.

Satellite view of the Earth (north America) from space.

UIG529847

Sao Paulo, Brazil, 2002, 2002

Sao Paulo, Brazil, 2002, 2002

UIG1579995

Typhoon Faxai, 2001

Typhoon Faxai, 2001

UIG3508172

Sunrise seen from Triton - Artist view - Sunrise on Triton - Artist view - Sunrise seen from Triton, the largest satellite in Neptune. A diminutive sun rises over Triton's hard and glistening landscape of rock, frozen water, carbon dioxide, nitrogen, and methane. The little warmth that reaches Triton's surface induces a nitrogen and methane haze, forming a very tenuous atmosphere. It is very cold on Triton with temperatures falling as low as minus 391o F. While as much as 25% of Triton may be composed of water ice, it is very unlikely that there is any liquid water, or life, on this world

Sunrise seen from Triton - Artist view - Sunrise on Triton - Artist view - Sunrise seen from Triton, the largest satellite in Neptune. A diminutive sun rises over Triton's hard and glistening landscape of rock, frozen water, carbon dioxide, nitrogen, and methane. The little warmth that reaches Triton's surface induces a nitrogen and methane haze, forming a very tenuous atmosphere. It is very cold on Triton with temperatures falling as low as minus 391o F. While as much as 25% of Triton may be composed of water ice, it is very unlikely that there is any liquid water, or life, on this world

Walter B Myers

PIX4624014

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Pluto vue de Charon - Vue d'artiste - Pluto seen from Charon - Artist view: Vue d'artiste de Pluto vue dans le ciel de son satellite Charon. Pluto seen from its moon Charon

Miller, Ron (b.1947)

PIX4624501

Astronauts on Titan - Illustration - Walking a dry gully on Titan - Astronauts explore Titan's surface. Earthlings explore a dry gully on Saturn's moon Titan. In early 2005 the European Space Agency's Huygens probe revealed a surface carved by numerous drainage channels similar to river deltas on Earth. While the exact nature of these channels is not yet known, one theory proposes that Titan's surface of hydrocarbon sediments has been washed from the highlands by methane rain

Astronauts on Titan - Illustration - Walking a dry gully on Titan - Astronauts explore Titan's surface. Earthlings explore a dry gully on Saturn's moon Titan. In early 2005 the European Space Agency's Huygens probe revealed a surface carved by numerous drainage channels similar to river deltas on Earth. While the exact nature of these channels is not yet known, one theory proposes that Titan's surface of hydrocarbon sediments has been washed from the highlands by methane rain

Walter B Myers

PIX4626139

Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft - Comparison of the two hemispheres of Japet, a satellite of Saturn of 1471 kilometres in diameter. Its main feature is the color difference between the two hemispheres. On the left, the dark region called Cassini Regio with to the east the largest crater of Japet, named Turgis (580 km in diameter). On the right, the bright side of the satellite with Roncevaux Terra (north) and Saragossa Terra (south) housing the large impact crater Engelier (504 km in diameter). Both images were obtained by the Cassini probe on 10 September 2007 (right) and 27 December 2004 (left). These two global images of Iapetus show the extreme brightness dichotomy on the surface of this peculiar Saturnian moon. The left - hand panel shows the moon's leading hemisphere and the right - hand panel shows the moon's trailing side. While low and mid latitudes of the leading side exhibit a surface almost as dark as charcoal,

Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft - Comparison of the two hemispheres of Japet, a satellite of Saturn of 1471 kilometres in diameter. Its main feature is the color difference between the two hemispheres. On the left, the dark region called Cassini Regio with to the east the largest crater of Japet, named Turgis (580 km in diameter). On the right, the bright side of the satellite with Roncevaux Terra (north) and Saragossa Terra (south) housing the large impact crater Engelier (504 km in diameter). Both images were obtained by the Cassini probe on 10 September 2007 (right) and 27 December 2004 (left). These two global images of Iapetus show the extreme brightness dichotomy on the surface of this peculiar Saturnian moon. The left - hand panel shows the moon's leading hemisphere and the right - hand panel shows the moon's trailing side. While low and mid latitudes of the leading side exhibit a surface almost as dark as charcoal,

PIX4625409

Oil Lake on Titan - Titan's ethane ocean - Artist's view of a hydrocarbon lake (methane - ethane) on the surface of Titan. Compared to the Earth, Titan is very far from the Sun's warming rays - - about ten times further - - and this leaves Titan a very cold world. Titan has an average surface temperature of minus 290o F. If there is any water on Titan it is frozen hard as steel, yet Titan may be the only body in the Solar System besides the Earth that harbors a liquid ocean. Titan's ocean would not be one of water, rather it would probably be composed of (very cold) liquid ethane. (On the Earth we know ethane as a colorless, odorless, nontoxic, flammable gas, a constituent of natural gas and petroleum.) If this werenn't exotic enough, immediately beneath this ocean may lie hundreds of feet of frozen acetylene (a common component of welder's torches)

Oil Lake on Titan - Titan's ethane ocean - Artist's view of a hydrocarbon lake (methane - ethane) on the surface of Titan. Compared to the Earth, Titan is very far from the Sun's warming rays - - about ten times further - - and this leaves Titan a very cold world. Titan has an average surface temperature of minus 290o F. If there is any water on Titan it is frozen hard as steel, yet Titan may be the only body in the Solar System besides the Earth that harbors a liquid ocean. Titan's ocean would not be one of water, rather it would probably be composed of (very cold) liquid ethane. (On the Earth we know ethane as a colorless, odorless, nontoxic, flammable gas, a constituent of natural gas and petroleum.) If this werenn't exotic enough, immediately beneath this ocean may lie hundreds of feet of frozen acetylene (a common component of welder's torches)

Walter B Myers

PIX4626096

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

D. Ducros

PIX4604558

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

Fusees Ariane 5 ES ATV and ECA - Illustration - The Ariane 5 ES ATV and ECA rockets - Illustration - Artist view of the Ariane 5 ES ATV rocket, on the left, compare to the Ariane 5 ECA rocket, on the right. Artist's impression of the Ariane 5 ES ATV (left) with the Ariane 5 ECA (right)

D. Ducros

PIX4604560

Relief map of Iran (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

Relief map of Iran (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

UIG5422657

Satellite view of Iran with Bump Effect (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Iran with Bump Effect (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422676

Relief map of Iraq (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data

Relief map of Iraq (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data

UIG5422680

Relief map of Israel (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data

Relief map of Israel (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data

UIG5422689

Relief map of Israel (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

Relief map of Israel (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

UIG5422692

Satellite view of Jordan (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Jordan (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422703

Relief map of Kuwait (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

Relief map of Kuwait (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

UIG5422735

Satellite view of Lebanon (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Lebanon (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422761

War Games in Space

War Games in Space

Wood, Gerry (b.1938)

LAL295432

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, during summer solstice at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, during summer solstice at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5421995

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole with cloud coverage, at the equinox at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole with cloud coverage, at the equinox at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422002

Dubai, United Arab Emirates, In 1976, True Colour Satellite Image. True colour satellite image of Dubai, United Arab Emirates. Image size A4, taken on 8 June 1976, using LANDSAT data ©Planet Observer/UIG/Leemage

Dubai, United Arab Emirates, In 1976, True Colour Satellite Image. True colour satellite image of Dubai, United Arab Emirates. Image size A4, taken on 8 June 1976, using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5422064

Satellite view of Yemen (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Yemen (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5423135

Satellite view of Cyprus with Bump Effect. This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Cyprus with Bump Effect. This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422505

Satellite view of New Zealand. This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of New Zealand. This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422864

Relief map of New Zealand. This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

Relief map of New Zealand. This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data

UIG5422867

Relief map of Syria (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

Relief map of Syria (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

UIG5423061

Relief map of Tonga. This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

Relief map of Tonga. This image was compiled from data acquired by LANDSAT 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

UIG5423078

Relief map of The United Arab Emirates (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

Relief map of The United Arab Emirates (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

UIG5423109

Satellite view of Vanuatu. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Vanuatu. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5423133

Satellite view of Oman (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Oman (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422894

Satellite view of Palau with Bump Effect. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Palau with Bump Effect. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422904

Relief map of Portugal (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

Relief map of Portugal (with border and mask). This image was compiled from data acquired by landsat 5 & 7 satellites combined with elevation data ©Planet Observer/UIG/Leemage

UIG5422936

Satellite view of Portugal (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Portugal (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422942

Satellite view of Qatar (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Qatar (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422946

Satellite view of Qatar (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Satellite view of Qatar (with border). This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422947

Torres Detroit And Banks Islands, Australia, True Colour Satellite Image. The Torres detroit separates Australia (the Australian Cap York is down below on the image) from Papouasia-New Guinea ©Planet Observer/UIG/Leemage

Torres Detroit And Banks Islands, Australia, True Colour Satellite Image. The Torres detroit separates Australia (the Australian Cap York is down below on the image) from Papouasia-New Guinea ©Planet Observer/UIG/Leemage

UIG5421274

Lake Yamma, Queensland, Australia, True Colour Satellite Image. The Lake Yamma is a salted lake located in a semi-arid area. The lake evaporates totally during the dry season. During austral winter, the ochre soil of the desert is covered by rivers filled with sand, clay and salt that render that blue colour. Image taken on 18 July 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

Lake Yamma, Queensland, Australia, True Colour Satellite Image. The Lake Yamma is a salted lake located in a semi-arid area. The lake evaporates totally during the dry season. During austral winter, the ochre soil of the desert is covered by rivers filled with sand, clay and salt that render that blue colour. Image taken on 18 July 1990 using LANDSAT data ©Planet Observer/UIG/Leemage

UIG5421283

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, during summer solstice at 12 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, during summer solstice at 12 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5421991

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, at the equinox at 6 p.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Globe Centred On The South Pole, True Colour Satellite Image. True colour satellite image of the Earth centred on the South Pole, at the equinox at 6 p.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5422016

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - Astronauts John Grunsfeld (on the robotic arm of the shuttle) and Andrew Feustel (foreground) during the fifth and last extravehicular exit to maintain the Hubble space telescope (HST). 18 May 2009. Astronaut John Grunsfeld, STS - 125 mission specialist, positioned on a foot restraint on the end of Atlantis' remote manipulator system (RMS), and astronaut Andrew Feustel (foreground), mission specialist, participate in the mission's fifth and final session of extravehicular activity (EVA) as work continues to refurbish and upgrade the Hubble Space Telescope. During the seven - hour and two - minute spacewalk, Grunsfeld and Feustel installed a battery group replacement, removed and replaced a Fine Guidance Sensor and three thermal blankets (NOBL) protecting Hubble's electronics. 18 May 2009

Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - Astronauts John Grunsfeld (on the robotic arm of the shuttle) and Andrew Feustel (foreground) during the fifth and last extravehicular exit to maintain the Hubble space telescope (HST). 18 May 2009. Astronaut John Grunsfeld, STS - 125 mission specialist, positioned on a foot restraint on the end of Atlantis' remote manipulator system (RMS), and astronaut Andrew Feustel (foreground), mission specialist, participate in the mission's fifth and final session of extravehicular activity (EVA) as work continues to refurbish and upgrade the Hubble Space Telescope. During the seven - hour and two - minute spacewalk, Grunsfeld and Feustel installed a battery group replacement, removed and replaced a Fine Guidance Sensor and three thermal blankets (NOBL) protecting Hubble's electronics. 18 May 2009

PIX4645407

Mission habitee vers Mars-View d'artiste - Manned mission to Mars - Artist vie

Mission habitee vers Mars-View d'artiste - Manned mission to Mars - Artist vie

S. Numazawa

PIX4639464

Terraformation de Mars-Illustration - Terraforming of Mars - Illustration - In 1000 years, the inhabitants of the cites under the dome of Phobos will be able to contemplate the Martian oceans from their balconies. The terraforming of a planet, moon or other body, is the hypothetical process of deliberately modifying its atmosphere, temperature, or ecology to be similar to those of Earth in order to make it habitable by humans. Inhabitants of Phobos would gaze martian oceans in the next thousand years

Terraformation de Mars-Illustration - Terraforming of Mars - Illustration - In 1000 years, the inhabitants of the cites under the dome of Phobos will be able to contemplate the Martian oceans from their balconies. The terraforming of a planet, moon or other body, is the hypothetical process of deliberately modifying its atmosphere, temperature, or ecology to be similar to those of Earth in order to make it habitable by humans. Inhabitants of Phobos would gaze martian oceans in the next thousand years

P. Carril

PIX4639658

Typhoon Damrey, 2000

Typhoon Damrey, 2000

UIG3508173

Rhea, satellite of Saturn, seen by Cassini - Saturn's moon Rhea seen by Cassini - Mosaic of images obtained by the Cassini probe in March 2015. Rhea is the second largest satellite in Saturn (1528 km in diameter). After a couple of years in high - inclination orbits that limited its ability to encounter Saturn's moons, Nasa's Cassini spacecraft returned to Saturn's equatorial plane in March 2015.Image taken using clear, green, infrared and ultraviolet spectral filters were combined to create these enhanced color views, which offer an expanded range of the colors visible to human eyes in order to highlight subtle color differences across Rhea's surface. The moon's surface is fairly uniform in natural color.This view at right is centered at 9 degrees north latitude, 254 degrees west longitude. Resolution in this mosaic is 300 meters (984 feet) per pixel. The image was acquired at a distance that ranged from about 36,000 to 32.100 miles (57,900 to 51,700 kilometers) from Rhea

Rhea, satellite of Saturn, seen by Cassini - Saturn's moon Rhea seen by Cassini - Mosaic of images obtained by the Cassini probe in March 2015. Rhea is the second largest satellite in Saturn (1528 km in diameter). After a couple of years in high - inclination orbits that limited its ability to encounter Saturn's moons, Nasa's Cassini spacecraft returned to Saturn's equatorial plane in March 2015.Image taken using clear, green, infrared and ultraviolet spectral filters were combined to create these enhanced color views, which offer an expanded range of the colors visible to human eyes in order to highlight subtle color differences across Rhea's surface. The moon's surface is fairly uniform in natural color.This view at right is centered at 9 degrees north latitude, 254 degrees west longitude. Resolution in this mosaic is 300 meters (984 feet) per pixel. The image was acquired at a distance that ranged from about 36,000 to 32.100 miles (57,900 to 51,700 kilometers) from Rhea

PIX4625591

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

PIX4625625

Saturn seen from his satellite Japet - Saturn as seen from Iapetus

Saturn seen from his satellite Japet - Saturn as seen from Iapetus

Miller, Ron (b.1947)

PIX4974169

Mars - Phobos Satellite - Martian moon Phobos - View of the Phobos satellite obtained by the Mars Express probe on March 7, 2010. The resolution is 4.4 meters per pixel. Mars Express took this image of the surface of the moon Phobos on 7 March 2010. The resolution is about 4.4 m/pixel

Mars - Phobos Satellite - Martian moon Phobos - View of the Phobos satellite obtained by the Mars Express probe on March 7, 2010. The resolution is 4.4 meters per pixel. Mars Express took this image of the surface of the moon Phobos on 7 March 2010. The resolution is about 4.4 m/pixel

PIX4616280

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

PIX4625583

Pluto and Charon - Artist view - Pluto and Charon - Artist view - Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Pluto and Charon - Artist view - Pluto and Charon - Artist view - Pluto's icy surface with its Charon satellite in the sky. Icy surface of Pluto with in the sky its moon Charon

Miller, Ron (b.1947)

PIX4624499

Satellite view of Georgia with Bump Effect (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

Satellite view of Georgia with Bump Effect (with border and mask). This image was compiled from data acquired by LANDSAT 5 & 7 satellites

UIG5422608

Lake Baikal, Siberia, Russia, True Colour Satellite Image. True colour satellite image of Lake Baikal, located in the south of the Russian region of Siberia. Composite image using LANDSAT 5 data ©Planet Observer/UIG/Leemage

Lake Baikal, Siberia, Russia, True Colour Satellite Image. True colour satellite image of Lake Baikal, located in the south of the Russian region of Siberia. Composite image using LANDSAT 5 data ©Planet Observer/UIG/Leemage

UIG5422142

Kuwait, True Colour Satellite Image With Mask. Kuwait, true colour satellite image with mask. North of the image, the Shatt al Arab river flows into the Persian Gulf. Kuwait City (center) is the capital city of Kuwait. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

Kuwait, True Colour Satellite Image With Mask. Kuwait, true colour satellite image with mask. North of the image, the Shatt al Arab river flows into the Persian Gulf. Kuwait City (center) is the capital city of Kuwait. This image was compiled from data acquired by LANDSAT 5 & 7 satellites ©Planet Observer/UIG/Leemage

UIG5421051

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