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Images of 'Enceladus' found, 89

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Ghost tendrils of Enceladus - Artist view - Enceladus icy tendrils - Artist view: Artist view of the particles and grains of ice ejects from the geysers of the satellite Enceladus - Tendril-like features from Saturn's moon Enceladus are the trajectories of tiny, icy grains ejected from Enceladus 'south polar geysers

Ghost tendrils of Enceladus - Artist view - Enceladus icy tendrils - Artist view: Artist view of the particles and grains of ice ejects from the geysers of the satellite Enceladus - Tendril-like features from Saturn's moon Enceladus are the trajectories of tiny, icy grains ejected from Enceladus 'south polar geysers

Miller, Ron (b.1947)

PIX4625913

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

PIX4625460

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn. Enceladus, one of Saturn's many icy moons, is now known to possess underground reservoirs of liquid water which sometimes erupt to the surface in the form of great jets or geysers. These keep the moon's surface sparkling white, and even add material to Saturn's rings

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn. Enceladus, one of Saturn's many icy moons, is now known to possess underground reservoirs of liquid water which sometimes erupt to the surface in the form of great jets or geysers. These keep the moon's surface sparkling white, and even add material to Saturn's rings

PIX4625859

The Cassini probe and the Enceladus geysers - Cassini spacecraft with Enceladus Geysers: Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. His mission ended on 15 September 2017. Cassini spacecraft is diving through the plume of Saturn's moon Enceladus

The Cassini probe and the Enceladus geysers - Cassini spacecraft with Enceladus Geysers: Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. His mission ended on 15 September 2017. Cassini spacecraft is diving through the plume of Saturn's moon Enceladus

PIX4606103

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Walter B Myers

PIX4625835

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn. A look at the water geysers of Saturn's moon Enceladus, which have been revealed to us so brilliantly by the Cassini Saturn orbiter. This digital illustration shows the water jets shooting out from vents in the bottom of one of the icy moon's multitude of folded, fractured valleys

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn. A look at the water geysers of Saturn's moon Enceladus, which have been revealed to us so brilliantly by the Cassini Saturn orbiter. This digital illustration shows the water jets shooting out from vents in the bottom of one of the icy moon's multitude of folded, fractured valleys

PIX4625857

Enceladus, Saturn's satellite, seen by the Cassini probe - Saturn's moon Enceladus seen by Cassini spacecraft - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 5 October 2008. The image shows a fractured region in the southern hemisphere of the satellite. On Oct. 5, 2008, just after coming within 25 kilometers (15.6 miles) of the surface of Enceladus, Nasa's Cassini captured this stunning mosaic as the spacecraft sped away from this geologically active moon of Saturn. Craters and cratered terrains are rare in this view of the southern region of the moon's Saturn - facing hemisphere. Instead, the surface is replete with fractures, folds, and ridges - - all hallmarks of remarkable tectonic activity for a relatively small world. In this enhanced - color view, regions that appear blue - green are thought to be coated with larger grains than those that appear white or gray. Portions of the tiger stripe fractures, or sulci, are visible a

Enceladus, Saturn's satellite, seen by the Cassini probe - Saturn's moon Enceladus seen by Cassini spacecraft - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 5 October 2008. The image shows a fractured region in the southern hemisphere of the satellite. On Oct. 5, 2008, just after coming within 25 kilometers (15.6 miles) of the surface of Enceladus, Nasa's Cassini captured this stunning mosaic as the spacecraft sped away from this geologically active moon of Saturn. Craters and cratered terrains are rare in this view of the southern region of the moon's Saturn - facing hemisphere. Instead, the surface is replete with fractures, folds, and ridges - - all hallmarks of remarkable tectonic activity for a relatively small world. In this enhanced - color view, regions that appear blue - green are thought to be coated with larger grains than those that appear white or gray. Portions of the tiger stripe fractures, or sulci, are visible a

PIX4625451

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of the ice jets on the surface of the Enceladus satellite observed by the Cassini probe. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Enceladus 'ice geysers - Saturn is in background. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of the ice jets on the surface of the Enceladus satellite observed by the Cassini probe. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Enceladus 'ice geysers - Saturn is in background. Artist view

M. Carroll

PIX4625793

Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite

Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite

Miller, Ron (b.1947)

PIX4625909

Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite

Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite

Miller, Ron (b.1947)

PIX4625936

Hydrothermal springs on Enceladus - Artist view - Enceladus Smokers - Artist view: Artist view of hydrothermal chiminees in the ocean of Enceladus. Illustration of hydrothermal activity in Enceladus subsurface ocean

Hydrothermal springs on Enceladus - Artist view - Enceladus Smokers - Artist view: Artist view of hydrothermal chiminees in the ocean of Enceladus. Illustration of hydrothermal activity in Enceladus subsurface ocean

Miller, Ron (b.1947)

PIX4625933

Size comparison: Enceladus, Earth and Moon satellite - Enceladus, Earth, and Earth's Moon Compared - Saturn Enceladus satellite (500 km in diameter) compares with Earth and Moon. Enceladus is considered one of Saturn's major satellites, however it is quite diminutive when compared with the Earth and Earth's Moon. With a radius of only 160 miles, Enceladus could rest in the Gulf of Mexico with plenty of room to spare. Enceladus is one of the brightest objects in the Solar System. Where Earth's Moon has a surface reflectively about the same as charcoal, Enceladus is covered in water ice that reflects sunlight like freshly fallen snow

Size comparison: Enceladus, Earth and Moon satellite - Enceladus, Earth, and Earth's Moon Compared - Saturn Enceladus satellite (500 km in diameter) compares with Earth and Moon. Enceladus is considered one of Saturn's major satellites, however it is quite diminutive when compared with the Earth and Earth's Moon. With a radius of only 160 miles, Enceladus could rest in the Gulf of Mexico with plenty of room to spare. Enceladus is one of the brightest objects in the Solar System. Where Earth's Moon has a surface reflectively about the same as charcoal, Enceladus is covered in water ice that reflects sunlight like freshly fallen snow

Walter B Myers

PIX4629983

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Walter B Myers

PIX4625896

Saturn seen from Enceladus - Illustration - Saturn from the surface of Enceladus: The planet Saturn seen from the icy surface of its satellite Enceladus

Saturn seen from Enceladus - Illustration - Saturn from the surface of Enceladus: The planet Saturn seen from the icy surface of its satellite Enceladus

Miller, Ron (b.1947)

PIX4625874

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view: Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn - Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view: Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn - Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole

Miller, Ron (b.1947)

PIX4625876

Cassini spacecraft with Enceladus Geysers - Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini deliberately flies through the enigmatic geysurs of Encaledus, as the slim cresent of Saturn rises above the horizon

Cassini spacecraft with Enceladus Geysers - Artist's view of the Cassini probe observing geysers on the surface of Enceladus, one of Saturn's satellites. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini deliberately flies through the enigmatic geysurs of Encaledus, as the slim cresent of Saturn rises above the horizon

Steven Hobbs

PIX4643515

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. The largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Titan's left, just above the rings, on its left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. Several of Saturn's moons transiting the face of the gas giant planet. This is a rare event because the rings are tilted edge on to Earth every 15 years. This frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow are below, at left, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. The largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Titan's left, just above the rings, on its left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. Several of Saturn's moons transiting the face of the gas giant planet. This is a rare event because the rings are tilted edge on to Earth every 15 years. This frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow are below, at left, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the

PIX4624886

Planet Saturn, Saturn, 2018 (photo)

Planet Saturn, Saturn, 2018 (photo)

PIX5973642

Artist's view of ice geysers on the surface of the Enceladus satellite. In the sky, the Sun and the Planet Saturn.

Artist's view of ice geysers on the surface of the Enceladus satellite. In the sky, the Sun and the Planet Saturn.

Miller, Ron (b.1947)

PIX4626439

Surface d'Enceladus - Artist view - Enceladus Panorama - Artist view - Artist view of ice geysers on the surface of the Enceladus satellite. In the sky, the Sun and the Planet Saturn. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky.

Surface d'Enceladus - Artist view - Enceladus Panorama - Artist view - Artist view of ice geysers on the surface of the Enceladus satellite. In the sky, the Sun and the Planet Saturn. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky.

Miller, Ron (b.1947)

PIX4945527

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid wate

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid wate

Walter B Myers

PIX4625850

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

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

PIX4624944

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of ice jets on the surface of the Enceladus satellite. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Geysers erupt from the so called Tiger Stripes of Encaledus, one of Saturn's moons. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of ice jets on the surface of the Enceladus satellite. It would appear that these particles feed the E-ring of Saturn, the origin of which was previously unknown. Geysers erupt from the so called Tiger Stripes of Encaledus, one of Saturn's moons. Artist view

Steven Hobbs

PIX4625825

images of Saturn's moon Enceladus

images of Saturn's moon Enceladus

UIG3524589

Size comparison: Enceladus and Spain - Planetary-size comparison: Enceladus with Spain - Saturn Enceladus satellite (500 km in diameter) compares with Spain. A moon of Saturn, Enceladus (500 km in diameter), compared to the Earth

Size comparison: Enceladus and Spain - Planetary-size comparison: Enceladus with Spain - Saturn Enceladus satellite (500 km in diameter) compares with Spain. A moon of Saturn, Enceladus (500 km in diameter), compared to the Earth

M. Carroll

PIX4629938

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Miller, Ron (b.1947)

PIX4625828

Astronaut and Geyser on Enceladus - Artist view - Astronaut and Water geyser on Enceladus - Artist view: An astronaut contemplates the eruption of an ice geyser accompanied by a parhely on the surface of the Enceladus satellite

Astronaut and Geyser on Enceladus - Artist view - Astronaut and Water geyser on Enceladus - Artist view: An astronaut contemplates the eruption of an ice geyser accompanied by a parhely on the surface of the Enceladus satellite

Miller, Ron (b.1947)

PIX4625922

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

PIX4625315

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. On the top image, the largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Saturn's left blade, on the left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. The image in the center shows the satellites Enceladus and Dione that cast their shadow on the west (left) side of Saturn, Titan in the upper right, and Mimas on the eastern edge of Saturn. In the image below, Dione and his shadow pass to the center of Saturn, above Enceladus and its shadow. Titan is on Saturn's eastern blade, Mimas is right above the rings. This sequence of images captures the parade of several of Saturn's moons trans

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. On the top image, the largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Saturn's left blade, on the left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. The image in the center shows the satellites Enceladus and Dione that cast their shadow on the west (left) side of Saturn, Titan in the upper right, and Mimas on the eastern edge of Saturn. In the image below, Dione and his shadow pass to the center of Saturn, above Enceladus and its shadow. Titan is on Saturn's eastern blade, Mimas is right above the rings. This sequence of images captures the parade of several of Saturn's moons trans

PIX4624877

images of Saturn's moon Enceladus

images of Saturn's moon Enceladus

UIG3524407

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of a space probe sent to observe ice jets on the surface of the Enceladus satellite. A spacecraft sent to study geysers of Enceladus, one of Saturn's moons. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of a space probe sent to observe ice jets on the surface of the Enceladus satellite. A spacecraft sent to study geysers of Enceladus, one of Saturn's moons. Artist view

Miller, Ron (b.1947)

PIX4625843

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Miller, Ron (b.1947)

PIX4625820

Size comparison: Enceladus satellite and Japan - Planetary-size comparison: Enceladus with Japan - Saturn Enceladus satellite (500 km in diameter) compares to Japan. A moon of Saturn, Enceladus (500 km in diameter), compared to the Earth

Size comparison: Enceladus satellite and Japan - Planetary-size comparison: Enceladus with Japan - Saturn Enceladus satellite (500 km in diameter) compares to Japan. A moon of Saturn, Enceladus (500 km in diameter), compared to the Earth

M. Carroll

PIX4629933

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Geysers sur Enceladus - Artist view - Enceladus' ice geysers - Artist view - Artist view of astronauts who came to observe the ice jets on the surface of the Enceladus satellite. Astronauts observing geysers of Enceladus, one of Saturn's moons. Artist view

Miller, Ron (b.1947)

PIX4625872

Enceladus the sixth-largest moon of Saturn.

Enceladus the sixth-largest moon of Saturn.

UIG3524516

Photograph of Enceladus

Photograph of Enceladus

UIG3524411

The cracks in Saturns moon, Enceladus

The cracks in Saturns moon, Enceladus

UIG2911243

The Cassini spacecraft observes three of Saturn's moons set against the darkened night side of the planet. Rhea, Enceladus and Dione.

The Cassini spacecraft observes three of Saturn's moons set against the darkened night side of the planet. Rhea, Enceladus and Dione.

UIG866395

A pair of Saturn's moons appears as if hung below the planet's rings in this Cassini spacecraft view. Enceladus and Tethys.

A pair of Saturn's moons appears as if hung below the planet's rings in this Cassini spacecraft view. Enceladus and Tethys.

UIG866406

The Cassini spacecraft looks at a brightly illuminated Enceladus and examines the surface of the leading hemisphere of this Saturnian moon.

The Cassini spacecraft looks at a brightly illuminated Enceladus and examines the surface of the leading hemisphere of this Saturnian moon.

UIG866410

The Enceladus Basin (or The Fountain of Enceladus) at Versailles, France 18th Century

The Enceladus Basin (or The Fountain of Enceladus) at Versailles, France 18th Century

DGA509919

Exploring Enceladus - Illustration

Exploring Enceladus - Illustration

Miller, Ron (b.1947)

PIX7223436

Geyser on Enceladus - Artist view

Geyser on Enceladus - Artist view

Miller, Ron (b.1947)

PIX7223435

Exploring Enceladus - Illustration

Exploring Enceladus - Illustration

Miller, Ron (b.1947)

PIX7223438

Geyser on Enceladus - Artist view

Geyser on Enceladus - Artist view

Miller, Ron (b.1947)

PIX7223434

Exploring Enceladus - Illustration

Exploring Enceladus - Illustration

Miller, Ron (b.1947)

PIX7223431

Exploring Enceladus - Illustration

Exploring Enceladus - Illustration

Miller, Ron (b.1947)

PIX7223432

Exploring Enceladus - Illustration

Exploring Enceladus - Illustration

Miller, Ron (b.1947)

PIX7223433

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia

PIX4625492

Enceladus (Moon Of Saturn), 2018 (digital illustration)

Enceladus (Moon Of Saturn), 2018 (digital illustration)

Roetsch, Tobias

KBS7232267

Enceladus Buried Underneath Mount Etna, 1731 (engraving)

Enceladus Buried Underneath Mount Etna, 1731 (engraving)

Picart, Bernard (1673-1733)

STC134101

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 25 images obtained by the Cassini probe during the flight over this satellite on March 9, 2005. The image shows the side of Enceladus opposite Saturn. Many cracks and impact crateres are visible

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 25 images obtained by the Cassini probe during the flight over this satellite on March 9, 2005. The image shows the side of Enceladus opposite Saturn. Many cracks and impact crateres are visible

PIX4625488

The Groves of the Versailles. View of the Fountain of Enceladus with the Feast of Lycaon (oil on canvas)

The Groves of the Versailles. View of the Fountain of Enceladus with the Feast of Lycaon (oil on canvas)

Cotelle, Jean the Younger (1642-1708)

XIR288987

The Basin of Enceladus at Versailles, early eighteenth century (oil on canvas)

The Basin of Enceladus at Versailles, early eighteenth century (oil on canvas)

French School, (18th century)

XIR375742

Enceladus, one of the moons of Saturn, photographed by Voyager 2, 1981

Enceladus, one of the moons of Saturn, photographed by Voyager 2, 1981

UIS5071148

Magna graecia: metope with Enceladus and Athena (Gigantomachy), stone relief, 5th century BC

Magna graecia: metope with Enceladus and Athena (Gigantomachy), stone relief, 5th century BC

Greek school, (5th century BC)

Luisa Ricciarini

LRI4592142

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water.

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water.

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Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 11 images obtained by the Cassini probe during the flight over this satellite on 9 March 2005. Image shows a region in the middle of the hemisphere opposite Saturn, where many flaws are visible

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 11 images obtained by the Cassini probe during the flight over this satellite on 9 March 2005. Image shows a region in the middle of the hemisphere opposite Saturn, where many flaws are visible

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The brightly reflective moon Enceladus appears before Saturn's rings while the larger moon Titan looms in the distance.

The brightly reflective moon Enceladus appears before Saturn's rings while the larger moon Titan looms in the distance.

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