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Saturn seen by the Cassini probe - Saturn seen by Cassini - Saturn seen by the Cassini probe on 22 August 2008 at a distance of 1.2 million km from the planet. The Cassini spacecraft looks toward the sunlit face of Saturn's rings, whose shadows continue to slide southward on the planet toward their temporary disappearance during equinox in August 2009. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Aug. 22, 2008 at a distance of approximately 1.2 million kilometers (728,000 miles) from Saturn. Image scale is 66 kilometers (41 miles) per pixel

Saturn seen by the Cassini probe - Saturn seen by Cassini - Saturn seen by the Cassini probe on 22 August 2008 at a distance of 1.2 million km from the planet. The Cassini spacecraft looks toward the sunlit face of Saturn's rings, whose shadows continue to slide southward on the planet toward their temporary disappearance during equinox in August 2009. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide - angle camera on Aug. 22, 2008 at a distance of approximately 1.2 million kilometers (728,000 miles) from Saturn. Image scale is 66 kilometers (41 miles) per pixel

PIX4625173

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

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

PIX5940218

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 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

Saturn and Titan - Illustration - Saturn from Titan orbit - The planet Saturn seen from the orbit of its Titan satellite. This is how Saturn and Titan might look from a position in orbit around Titan. While in reality Saturn is vastly larger than Titan, it appears smaller here because Titan's orbit puts Saturn at a distance of about 700 thousand miles. Sunlight filtering through Titan's upper atmospheric haze - - extending over 300 miles above the surface - - gives a bluish cast to its limb

Saturn and Titan - Illustration - Saturn from Titan orbit - The planet Saturn seen from the orbit of its Titan satellite. This is how Saturn and Titan might look from a position in orbit around Titan. While in reality Saturn is vastly larger than Titan, it appears smaller here because Titan's orbit puts Saturn at a distance of about 700 thousand miles. Sunlight filtering through Titan's upper atmospheric haze - - extending over 300 miles above the surface - - gives a bluish cast to its limb

Walter B Myers

PIX4626066

Titan, Saturn satellite seen by Cassini - Titan near Saturn seen by Cassini spacecraft - Natural color image of Titan near Saturn blade taken by the Cassini probe on 29 January 2008 at a distance of about 2.3 million km from the satellite. Swathed in its thick blanket of atmosphere, frigid Titan approaches the brilliant limb of Saturn. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Jan. 29, 2008 at a distance of approximately 2.3 million kilometers (1.4 million miles) from Titan. Image scale is 14 kilometers (8 miles) per pixel

Titan, Saturn satellite seen by Cassini - Titan near Saturn seen by Cassini spacecraft - Natural color image of Titan near Saturn blade taken by the Cassini probe on 29 January 2008 at a distance of about 2.3 million km from the satellite. Swathed in its thick blanket of atmosphere, frigid Titan approaches the brilliant limb of Saturn. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Jan. 29, 2008 at a distance of approximately 2.3 million kilometers (1.4 million miles) from Titan. Image scale is 14 kilometers (8 miles) per pixel

PIX4625308

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 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

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

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

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 from the Atmosphere of Titan - Saturn from Titan - Illustration

Saturn seen from the Atmosphere of Titan - Saturn from Titan - Illustration

Steven Hobbs

PIX4626232

Saturn seen from a satellite Irregulier - Illustration: Irregular satellite of Saturn

Saturn seen from a satellite Irregulier - Illustration: Irregular satellite of Saturn

Miller, Ron (b.1947)

PIX4626441

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

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

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

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

PIX4625616

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

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

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 view of its satellite Hyperion - Artist view - Saturn from its moon Hyperion - Artist view

Saturn view of its satellite Hyperion - Artist view - Saturn from its moon Hyperion - Artist view

Miller, Ron (b.1947)

PIX4974168

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

Artist's view of the asteroid 2060 Chiron: (2060) Chiron, also designed as 95P/Chiron, is a centaur type cometary asteroid, an ice body of 166 kilometres of diameter orbiting around the Sun between Saturn and Uranus. 2060 Chiron, also known as 95P/Chiron, is a minor planet in the outer Solar System, orbiting the Sun between Saturn and Uranus. Discovered in 1977 it was the first-identified member of a new class of objects now known as centaurs - bodies orbiting between the asteroid belt and the Kuiper belt. Besides the four giant planets, Chiron and 10199 Chariklo, also a centaur, are the only other bodies in the Solar System known to have rings. Although it was initially called an asteroid and classified only as a minor planet with the designation “” 2060 Chiron””, it was later found to exhibit behavior typical of a comet. Today it is classified as both a minor planet and a comet, and is accordingly also known by the cometary designation “” 95P/Chiron””

Artist's view of the asteroid 2060 Chiron: (2060) Chiron, also designed as 95P/Chiron, is a centaur type cometary asteroid, an ice body of 166 kilometres of diameter orbiting around the Sun between Saturn and Uranus. 2060 Chiron, also known as 95P/Chiron, is a minor planet in the outer Solar System, orbiting the Sun between Saturn and Uranus. Discovered in 1977 it was the first-identified member of a new class of objects now known as centaurs - bodies orbiting between the asteroid belt and the Kuiper belt. Besides the four giant planets, Chiron and 10199 Chariklo, also a centaur, are the only other bodies in the Solar System known to have rings. Although it was initially called an asteroid and classified only as a minor planet with the designation “” 2060 Chiron””, it was later found to exhibit behavior typical of a comet. Today it is classified as both a minor planet and a comet, and is accordingly also known by the cometary designation “” 95P/Chiron””

Miller, Ron (b.1947)

PIX4584210

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

Saturn 3 by Stanley Donen, 1980

Saturn 3 by Stanley Donen, 1980

DIL1637623

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

Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice

Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice

Walter B Myers

PIX4626289

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

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

Saturn and Mimas seen by the Cassini probe on 04/09/2007 - Saturn and Mimas seen by Cassini spacecraft Sept. 4 2007 - Saturn seen by the Cassini probe on 4/09/2007 at a distance of 2.7 million km from the planet. The Mimas ice satellite is visible under Saturn's rings. The Cassini spacecraft looks beyond Saturn's limb towards the icy face of Mimas, the innermost of the planet's major moons. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Mimas is 396 kilometers (246 miles) across. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Sept. 4, 2007 at a distance of approximately 2.7 million kilometers (1.7 million miles) from Saturn and 2.8 million kilometers (1.8 million miles) from Mimas. Image scale is 16 kilometers (10 miles) per pixel on Saturn and 17 kilometers (11 miles) per pixel on Mimas

Saturn and Mimas seen by the Cassini probe on 04/09/2007 - Saturn and Mimas seen by Cassini spacecraft Sept. 4 2007 - Saturn seen by the Cassini probe on 4/09/2007 at a distance of 2.7 million km from the planet. The Mimas ice satellite is visible under Saturn's rings. The Cassini spacecraft looks beyond Saturn's limb towards the icy face of Mimas, the innermost of the planet's major moons. This view looks toward the sunlit side of the rings from about 3 degrees below the ringplane. Mimas is 396 kilometers (246 miles) across. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft narrow - angle camera on Sept. 4, 2007 at a distance of approximately 2.7 million kilometers (1.7 million miles) from Saturn and 2.8 million kilometers (1.8 million miles) from Mimas. Image scale is 16 kilometers (10 miles) per pixel on Saturn and 17 kilometers (11 miles) per pixel on Mimas

PIX4625115

Saturn view from its satellite Rhea - Artist view - Saturn from Rhea - Artist view: Artist view of the surface of the satellite Rhea and the planet Saturn - Saturn rises above its moon Rhea

Saturn view from its satellite Rhea - Artist view - Saturn from Rhea - Artist view: Artist view of the surface of the satellite Rhea and the planet Saturn - Saturn rises above its moon Rhea

Miller, Ron (b.1947)

PIX4626388

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

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

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

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

PIX4625625

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

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

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

The formation of Saturn's rings - Artist's view - The origin of Saturn's rings

The formation of Saturn's rings - Artist's view - The origin of Saturn's rings

Miller, Ron (b.1947)

PIX4625779

The Moon, Venus and Saturn (Plate XXX), from 'A Celestial Atlas' by Alexander Jamieson, pub. London 1822 (hand coloured engraving)

The Moon, Venus and Saturn (Plate XXX), from 'A Celestial Atlas' by Alexander Jamieson, pub. London 1822 (hand coloured engraving)

Jamieson, Alexander (fl.1820)

STC956782

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

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

Saturn view from its satellite Rhea - Artist view - Saturn from Rhea - Artist view: Artist view of the surface of the satellite Rhea and the planet Saturn - Saturn rises above its moon Rhea

Saturn view from its satellite Rhea - Artist view - Saturn from Rhea - Artist view: Artist view of the surface of the satellite Rhea and the planet Saturn - Saturn rises above its moon Rhea

Miller, Ron (b.1947)

PIX4626379

Saturn 3 by Stanley Donen, 1980

Saturn 3 by Stanley Donen, 1980

DIL1637622

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

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

PIX4625591

Saturn from his satellite Dione - Illustration

Saturn from his satellite Dione - Illustration

Miller, Ron (b.1947)

PIX4625645

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

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

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The formation of Saturn's rings - Artist's view - Saturn moon break up - A satellite of Saturn breaks giving birth to the rings of Saturn and has small satellites

The formation of Saturn's rings - Artist's view - Saturn moon break up - A satellite of Saturn breaks giving birth to the rings of Saturn and has small satellites

Miller, Ron (b.1947)

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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

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

the planet Saturn

UIG529113

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

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Saturn and satellites shepherds - Artist view - Saturn and Shepherd Moons - Artist view - Artist view of Saturn's F ring accompanies small satellites shepherds Promethee and Pandora. The weirdly braided F - ring of Saturn is confined by two tiny “” shepherd”” moons, named Prometheus and Pandora, which orbit just on either side of it

Saturn and satellites shepherds - Artist view - Saturn and Shepherd Moons - Artist view - Artist view of Saturn's F ring accompanies small satellites shepherds Promethee and Pandora. The weirdly braided F - ring of Saturn is confined by two tiny “” shepherd”” moons, named Prometheus and Pandora, which orbit just on either side of it

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A satellite of Saturn breaks into the rings of Saturn and has small satellites.

A satellite of Saturn breaks into the rings of Saturn and has small satellites.

Miller, Ron (b.1947)

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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.

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

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

Miller, Ron (b.1947)

PIX4974169

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

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

PIX4625583

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

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The Cassini - Huygens probe crosses the rings of Saturn - Cassini - Huygens spacecraft crossing Saturn's rings - Artist's view of the Cassini probe as he crossed the rings of 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 Cassini/Huygens spacecraft makes a dangerous journey through Saturn's debris filled ring plane before entering orbit around the planet

The Cassini - Huygens probe crosses the rings of Saturn - Cassini - Huygens spacecraft crossing Saturn's rings - Artist's view of the Cassini probe as he crossed the rings of 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 Cassini/Huygens spacecraft makes a dangerous journey through Saturn's debris filled ring plane before entering orbit around the planet

Steven Hobbs

PIX4606024

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

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

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

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