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Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

D. Ducros

PIX4606055

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

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

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Miller, Ron (b.1947)

PIX4626037

Saturn view from his satellite Tethys - Artist view - Saturn from Tethys - Artist view - Artist view from Ithaca Chasma on the surface of the satellite Tethys. Ithaca Chasma is a large valley 100 km wide, 2000 km long and several km deep. Artist rendering of Ithaca Chasma, a large valley on Saturn's moon Tethys. Ithaca Chasma is 100 km wide, 3 to 5 km deep and 2,000 km long

Saturn view from his satellite Tethys - Artist view - Saturn from Tethys - Artist view - Artist view from Ithaca Chasma on the surface of the satellite Tethys. Ithaca Chasma is a large valley 100 km wide, 2000 km long and several km deep. Artist rendering of Ithaca Chasma, a large valley on Saturn's moon Tethys. Ithaca Chasma is 100 km wide, 3 to 5 km deep and 2,000 km long

Miller, Ron (b.1947)

PIX4626250

Saturn view from his satellite Tethys - Artist view - Saturn from Tethys - Artist view - Artist view from Ithaca Chasma on the surface of the satellite Tethys. Ithaca Chasma is a large valley 100 km wide, 2000 km long and several km deep. Artist rendering of Ithaca Chasma, a large valley on Saturn's moon Tethys. Ithaca Chasma is 100 km wide, 3 to 5 km deep and 2,000 km long

Saturn view from his satellite Tethys - Artist view - Saturn from Tethys - Artist view - Artist view from Ithaca Chasma on the surface of the satellite Tethys. Ithaca Chasma is a large valley 100 km wide, 2000 km long and several km deep. Artist rendering of Ithaca Chasma, a large valley on Saturn's moon Tethys. Ithaca Chasma is 100 km wide, 3 to 5 km deep and 2,000 km long

Miller, Ron (b.1947)

PIX4626263

Geyser on Titan - Artist view - Cryogeyser on Titan - Artist view - Artist view of geyser on the surface of Titan, Saturn's largest satellite

Geyser on Titan - Artist view - Cryogeyser on Titan - Artist view - Artist view of geyser on the surface of Titan, Saturn's largest satellite

Miller, Ron (b.1947)

PIX4974163

Planet Saturn, Saturn, 2018 (photo)

Planet Saturn, Saturn, 2018 (photo)

PIX5973642

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

D. Ducros

PIX4606082

In the rings of Saturn - Illustration - Saturn Ring Particles - Artist view - Artist view of the countless ice particles that make up Saturn's rings. A view from the interior of the rings of Saturn reveals some of the innumerable ice particles which make them up

In the rings of Saturn - Illustration - Saturn Ring Particles - Artist view - Artist view of the countless ice particles that make up Saturn's rings. A view from the interior of the rings of Saturn reveals some of the innumerable ice particles which make them up

PIX4625757

Saturn Planet - Hubble Space Telescope on June 20, 2019.

Saturn Planet - Hubble Space Telescope on June 20, 2019.

PIX5940218

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Steven Hobbs

PIX4626030

Ice volcano on Titan - Artist view - Titan Ice Volcano

Ice volcano on Titan - Artist view - Titan Ice Volcano

Miller, Ron (b.1947)

PIX4626243

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

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

PIX4625507

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

Astronauts explore the satellite Japet - Astronauts exploring Iapetus - Astronauts exploring Japet, one of Saturn's satellites. Astronauts are exploring Iapetus, one of Saturn's moons

Astronauts explore the satellite Japet - Astronauts exploring Iapetus - Astronauts exploring Japet, one of Saturn's satellites. Astronauts are exploring Iapetus, one of Saturn's moons

Miller, Ron (b.1947)

PIX4626315

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

Huygens probe en route to Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception of the Cassini orbiter shows the Huygens probe separating to enter Titan's atmosphere. After separation, the probe drifts for about three weeks until reaching its destination. Huygens landed on Titan surface on January 14, 2005

D. Ducros

PIX4606058

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

Occultation of Saturn by the Moon from 03/11/2001 - Moon is occulting Saturn. November 3 2001 - Sequence of images showing the passage of the Moon in front of Saturn

Occultation of Saturn by the Moon from 03/11/2001 - Moon is occulting Saturn. November 3 2001 - Sequence of images showing the passage of the Moon in front of Saturn

Sebastian Voltmer

PIX4588174

Occultation of Saturn by the Moon from 03/11/2001 - Moon is occulting Saturn. November 3 2001 - View with a C8 telescope and Televue-Barlow (2,5x

Occultation of Saturn by the Moon from 03/11/2001 - Moon is occulting Saturn. November 3 2001 - View with a C8 telescope and Televue-Barlow (2,5x

T. Edelmann

PIX4588186

Saturn Clouds - Clouds of Saturn - Artwork - Saturn rings seen through Saturn clouds. A view of the rings as seen from a point just above the main cloud deck of Saturn

Saturn Clouds - Clouds of Saturn - Artwork - Saturn rings seen through Saturn clouds. A view of the rings as seen from a point just above the main cloud deck of Saturn

PIX4625759

Saturn seen from his satellite Mimas - Illustration - Saturn as seen from Mimas - Illustration - Artist's view of the Herschel crater on the surface of the satellite Mimas. In the background, the planet Saturn. Artist's impression of crater Herschel on Mimas surface with planet Saturn in background

Saturn seen from his satellite Mimas - Illustration - Saturn as seen from Mimas - Illustration - Artist's view of the Herschel crater on the surface of the satellite Mimas. In the background, the planet Saturn. Artist's impression of crater Herschel on Mimas surface with planet Saturn in background

Miller, Ron (b.1947)

PIX4626337

Huygens probe enters the atmosphere of Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception shows the Huygens probe close to enter Titan's atmosphere. The probe Huygens landed on Titan surface on January 14, 2005

Huygens probe enters the atmosphere of Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception shows the Huygens probe close to enter Titan's atmosphere. The probe Huygens landed on Titan surface on January 14, 2005

D. Ducros

PIX4606081

The Cassini probe and the rings of Saturn - Cassini spacecraft with Saturn's rings - Artist's view of the Cassini probe near the rings of Saturn. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini-Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004.

The Cassini probe and the rings of Saturn - Cassini spacecraft with Saturn's rings - Artist's view of the Cassini probe near the rings of Saturn. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini-Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004.

Steven Hobbs

PIX4643503

The Huygens probe is on Titan - Artist view - Huygens Titan descent - Artist view - Artist view of the descent of the European probe Huygens on Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's impression shows the Probe Huygens suspended from the stabilizer parachute passing through the clouds that are expected at around 20 km altitude. The descent will occur during daylight to provide the best illumination conditions for imaging the clouds and surface

The Huygens probe is on Titan - Artist view - Huygens Titan descent - Artist view - Artist view of the descent of the European probe Huygens on Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's impression shows the Probe Huygens suspended from the stabilizer parachute passing through the clouds that are expected at around 20 km altitude. The descent will occur during daylight to provide the best illumination conditions for imaging the clouds and surface

PIX4606129

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

Dish depicting 'Saturn devouring one of his children' by Urbino

Dish depicting 'Saturn devouring one of his children' by Urbino

UIG3520186

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The planet Saturn seen through its rings. Image obtained by the Voyager 1 probe on November 14, 1980. Saturn's limb seen through the veil of its rings by Voyager 1 on November 14, 1980

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The planet Saturn seen through its rings. Image obtained by the Voyager 1 probe on November 14, 1980. Saturn's limb seen through the veil of its rings by Voyager 1 on November 14, 1980

Steven Hobbs

PIX4624899

Huygens probe enters the atmosphere of Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception shows the Huygens probe entering Titan's atmosphere. The probe Huygens landed on Titan surface on January 14, 2005

Huygens probe enters the atmosphere of Titan - The Huygens probe entering Titan's atmosphere - Artist's view of the European Huygens probe above the atmosphere of Titan. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. This artist's conception shows the Huygens probe entering Titan's atmosphere. The probe Huygens landed on Titan surface on January 14, 2005

Steven Hobbs

PIX4606111

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

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of Saturn's rings is projected on the planet. Image obtained by the Voyager 1 probe on November 12, 1980. Ring's shadow casted on Saturn photographed by Voyager 1 on November 12, 1980

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of Saturn's rings is projected on the planet. Image obtained by the Voyager 1 probe on November 12, 1980. Ring's shadow casted on Saturn photographed by Voyager 1 on November 12, 1980

Steven Hobbs

PIX4624910

Saturn seen by the Cassini probe - Saturn northern hemisphere seen by Cassini spacecraft: Saturn seen by the Cassini probe on 25 April 2016. Cassini scanned across the planet and its rings on April 25, 2016, capturing three sets of red, green and blue images to cover this entire scene showing the planet and the main rings. The images were obtained using Cassini's wide-angle camera at a distance of approximately 1.9 million miles (3 million kilometers) from Saturn and at an elevation of about 30 degrees above the ring plane. The view looks toward the sunlit side of the rings from a Sun-saturn-spacecraft angle, or phase angle, of 55 degrees.

Saturn seen by the Cassini probe - Saturn northern hemisphere seen by Cassini spacecraft: Saturn seen by the Cassini probe on 25 April 2016. Cassini scanned across the planet and its rings on April 25, 2016, capturing three sets of red, green and blue images to cover this entire scene showing the planet and the main rings. The images were obtained using Cassini's wide-angle camera at a distance of approximately 1.9 million miles (3 million kilometers) from Saturn and at an elevation of about 30 degrees above the ring plane. The view looks toward the sunlit side of the rings from a Sun-saturn-spacecraft angle, or phase angle, of 55 degrees.

PIX4625257

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 seen at equinox - Saturn during Equinox - Saturn seen by the Cassini probe on August 12, 2009, 1.25 days after the exact date of Saturn equinox. The images that make up this mosaic were obtained at a distance of 847,000 km from the planet. Several satellites are visible in this image: Janus (lower left), Epimethee (lower middle), Pandora (on the right of the image, outside the rings) and Atlas (on the right, inside the F ring). Seen from our planet, the view of Saturn's rings during equinox is extremely foreshortened and limited. But in orbit around Saturn, Cassini spacecraft had no such problems. From 20 degrees above the ring plane, Cassini's wide angle camera shot 75 exposures in succession for this mosaic showing Saturn, its rings, and a few of its moons a day and a half after exact Saturn equinox, when the sun's disk was exactly overhead at the planet's equator. The novel illumination geometry that accompanies equinox lowers the sun's angle to the ring plane, significantly

Saturn seen at equinox - Saturn during Equinox - Saturn seen by the Cassini probe on August 12, 2009, 1.25 days after the exact date of Saturn equinox. The images that make up this mosaic were obtained at a distance of 847,000 km from the planet. Several satellites are visible in this image: Janus (lower left), Epimethee (lower middle), Pandora (on the right of the image, outside the rings) and Atlas (on the right, inside the F ring). Seen from our planet, the view of Saturn's rings during equinox is extremely foreshortened and limited. But in orbit around Saturn, Cassini spacecraft had no such problems. From 20 degrees above the ring plane, Cassini's wide angle camera shot 75 exposures in succession for this mosaic showing Saturn, its rings, and a few of its moons a day and a half after exact Saturn equinox, when the sun's disk was exactly overhead at the planet's equator. The novel illumination geometry that accompanies equinox lowers the sun's angle to the ring plane, significantly

PIX4625283

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of the planet Saturn is projected on its rings. Image obtained by the Voyager 1 probe on November 14, 1980. The shadow of Saturn casted on the rings was photographed by Voyager 1 on November 14, 1980

Saturn seen by Voyager 1 - Saturn seen by Voyager 1 - The shadow of the planet Saturn is projected on its rings. Image obtained by the Voyager 1 probe on November 14, 1980. The shadow of Saturn casted on the rings was photographed by Voyager 1 on November 14, 1980

Steven Hobbs

PIX4624898

The Moon and Saturn - Moon with Saturn. November 3 2001 - The Moon and Planet Saturn. End of the blackout on 3 November 2001. Moon with Saturn. End of the occultation of november 3rd 2001

The Moon and Saturn - Moon with Saturn. November 3 2001 - The Moon and Planet Saturn. End of the blackout on 3 November 2001. Moon with Saturn. End of the occultation of november 3rd 2001

Sebastian Voltmer

PIX4588258

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

PIX4624969

The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

PIX4624799

Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope

Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope

Walter B Myers

PIX4625712

Occultation of Saturn by the Moon - The Moon and Planet Saturn. End of the blackout on 22 May 2007. Moon with Saturn. End of the occultation of may 22 2007

Occultation of Saturn by the Moon - The Moon and Planet Saturn. End of the blackout on 22 May 2007. Moon with Saturn. End of the occultation of may 22 2007

Alex Conu

PIX4569523

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

PIX4643494

La prode Cassini et Saturn - Cassini spacecraft at Saturn - This illustration shows Nasa's Cassini spacecraft about to make one of its dives between Saturn and its innermost rings as part of the mission's Grand Finale. Cassini will make 22 orbits that swoop between the rings and the planet before ending its mission on Sept 15, 2017, with a final plunge into Saturn

La prode Cassini et Saturn - Cassini spacecraft at Saturn - This illustration shows Nasa's Cassini spacecraft about to make one of its dives between Saturn and its innermost rings as part of the mission's Grand Finale. Cassini will make 22 orbits that swoop between the rings and the planet before ending its mission on Sept 15, 2017, with a final plunge into Saturn

PIX4643507

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe during its final dip into the atmosphere of Saturn on September 15, 2017. As depicted in this illustration, Cassini will plunge into Saturn's atmosphere on Sept 15, 2017. Using its attitude control thrusters, the spacecraft will work to keep its antenna pointed at Earth while it sends its final data, including the composition of Saturn's upper atmosphere. The atmospheric torque will quickly become stronger than what the thrusters can compensate for, and after that point, Cassini will begin to tumble. When this happens, its radio connection to Earth will be severed, ending the mission. Following loss of signal, the spacecraft will burn up like a meteor in Saturn's upper atmosphere.

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe during its final dip into the atmosphere of Saturn on September 15, 2017. As depicted in this illustration, Cassini will plunge into Saturn's atmosphere on Sept 15, 2017. Using its attitude control thrusters, the spacecraft will work to keep its antenna pointed at Earth while it sends its final data, including the composition of Saturn's upper atmosphere. The atmospheric torque will quickly become stronger than what the thrusters can compensate for, and after that point, Cassini will begin to tumble. When this happens, its radio connection to Earth will be severed, ending the mission. Following loss of signal, the spacecraft will burn up like a meteor in Saturn's upper atmosphere.

PIX4643513

Saturn seen by the Cassini probe - Saturn seen by Cassini spacecraft: Saturn seen by the Cassini probe on 28 October 2016. Images taken on Oct. 28, 2016 with the wide angle camera using red, green and blue spectral filters were combined to create this color view. This view looks toward the sunlit side of the rings from about 25 degrees above the ringplane. The view was acquired at a distance of approximately 870,000 miles (1.4 million kilometers) from Saturn. Image scale is 50 miles (80 kilometers) per pixel

Saturn seen by the Cassini probe - Saturn seen by Cassini spacecraft: Saturn seen by the Cassini probe on 28 October 2016. Images taken on Oct. 28, 2016 with the wide angle camera using red, green and blue spectral filters were combined to create this color view. This view looks toward the sunlit side of the rings from about 25 degrees above the ringplane. The view was acquired at a distance of approximately 870,000 miles (1.4 million kilometers) from Saturn. Image scale is 50 miles (80 kilometers) per pixel

PIX4582280

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

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

The Cassini and Saturn probe - Cassini spacecraft at Saturn: Artist's view of the Cassini probe around Saturn. - Artist's concept of Cassini orbiter crossing Saturn's ring plane

The Cassini and Saturn probe - Cassini spacecraft at Saturn: Artist's view of the Cassini probe around Saturn. - Artist's concept of Cassini orbiter crossing Saturn's ring plane

PIX4643481

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

PIX4606016

Occultation of Saturn by the Moon - Saturn occultation by the moon Artwork - Artist view

Occultation of Saturn by the Moon - Saturn occultation by the moon Artwork - Artist view

S. Numazawa

PIX4588586

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

PIX4624826

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

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

PIX4606029

Giant planets of our solar system - From top to bottom the planets Jupiter, Neptune and Saturn. Illustration. Illustration showing from top to bottom planets Jupiter, Neptune and Saturn

Giant planets of our solar system - From top to bottom the planets Jupiter, Neptune and Saturn. Illustration. Illustration showing from top to bottom planets Jupiter, Neptune and Saturn

D. Ducros

PIX4629732

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

PIX4625303

The planet Saturn observed with the Hubble space telescope in October 1997. Saturn is 120,000 km in diameter -: The planet Saturn seen by the Hubble space telescope in 1997 - Saturn seen from the Hubble space telescope in october 1997

The planet Saturn observed with the Hubble space telescope in October 1997. Saturn is 120,000 km in diameter -: The planet Saturn seen by the Hubble space telescope in 1997 - Saturn seen from the Hubble space telescope in october 1997

PIX4624811

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

PIX4625231

Size comparison: Earth and Saturn - Saturn and the Earth compared - Saturn, the second largest planet in the solar system compared to Earth. Saturn's diameter is about nine times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh only 165 pounds at Saturn's cloud tops (despite Saturn's enormous mass, its density is so low that if you were able to stand atop Saturn's clouds, you would feel a pull of gravity slightly less than what you feel on the Earth's surface). Saturn is ten times further from the Sun than the Earth. Saturn has the honor of being the second-largest planet in the Solar System, though it has only 30% the mass of its jovian better Jupiter. Like Jupiter, Saturn is blanketed by thick clouds and is believed to have no solid surface except for a relatively small, Earth-size core of rock and metals

Size comparison: Earth and Saturn - Saturn and the Earth compared - Saturn, the second largest planet in the solar system compared to Earth. Saturn's diameter is about nine times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh only 165 pounds at Saturn's cloud tops (despite Saturn's enormous mass, its density is so low that if you were able to stand atop Saturn's clouds, you would feel a pull of gravity slightly less than what you feel on the Earth's surface). Saturn is ten times further from the Sun than the Earth. Saturn has the honor of being the second-largest planet in the Solar System, though it has only 30% the mass of its jovian better Jupiter. Like Jupiter, Saturn is blanketed by thick clouds and is believed to have no solid surface except for a relatively small, Earth-size core of rock and metals

Walter B Myers

PIX4629905

The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996

The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996

PIX4624800

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

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