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Named after a Japanese paradise, NASA's Cassini spacecraft spies the Senkyo region of Titan), a bit less welcoming than its namesake with a very inhospitable average temperature of approximately 290 degrees below zero Fahrenheit (-180 degrees Celsius).
Named after a Japanese paradise, NASA's Cassini spacecraft spies the Senkyo region of Titan), a bit less welcoming than its namesake with a very inhospitable average temperature of approximately 290 degrees below zero Fahrenheit (-180 degrees Celsius).

Frozen Paradise

Named after a Japanese paradise, NASA's Cassini spacecraft spies the Senkyo region of Titan), a bit less welcoming than its namesake with a very inhospitable average temperature of approximately 290 degrees below zero Fahrenheit (-180 degrees Celsius).

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18309
Added: 2015-03-02

Views: 228

Frozen Paradise

Named after a Japanese paradise, NASA's Cassini spacecraft spies the Senkyo region of Titan), a bit less welcoming than its namesake with a very inhospitable average temperature of approximately 290 degrees below zero Fahrenheit (-180 degrees Celsius).

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Saturn's oblateness, the varying opacity of its rings and the shadows cast by those rings, sometimes creates elaborate and complicated patterns from NASA's Cassini's perspective.
Saturn's oblateness, the varying opacity of its rings and the shadows cast by those rings, sometimes creates elaborate and complicated patterns from NASA's Cassini's perspective.

Cubist Saturn

Saturn's oblateness, the varying opacity of its rings and the shadows cast by those rings, sometimes creates elaborate and complicated patterns from NASA's Cassini's perspective.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18303
Added: 2015-02-23

Views: 133

Cubist Saturn

Saturn's oblateness, the varying opacity of its rings and the shadows cast by those rings, sometimes creates elaborate and complicated patterns from NASA's Cassini's perspective.

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In reality, Janus and the rings both orbit Saturn and are only weakly connected to each other through their mutual gravitational tugs as seen by NASA's Cassini spacecraft.
In reality, Janus and the rings both orbit Saturn and are only weakly connected to each other through their mutual gravitational tugs as seen by NASA's Cassini spacecraft.

Janus the Jewel

In reality, Janus and the rings both orbit Saturn and are only weakly connected to each other through their mutual gravitational tugs as seen by NASA's Cassini spacecraft.

Target: Janus
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18304
Added: 2015-02-16

Views: 431

Janus the Jewel

In reality, Janus and the rings both orbit Saturn and are only weakly connected to each other through their mutual gravitational tugs as seen by NASA's Cassini spacecraft.

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Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view, at left, and one made using a new technique for handling electronic noise that results in clearer views of Titan's surface, at right.
Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view, at left, and one made using a new technique for handling electronic noise that results in clearer views of Titan's surface, at right.

Leilah Fluctus Despeckled

Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view, at left, and one made using a new technique for handling electronic noise that results in clearer views of Titan's surface, at right.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19054
Added: 2015-02-12

Views: 653

Leilah Fluctus Despeckled

Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view, at left, and one made using a new technique for handling electronic noise that results in clearer views of Titan's surface, at right.

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This montage from NASA's Cassini Synthetic Aperture Radar (SAR) images of the surface of Titan shows four examples of how a newly developed technique for handling noise results in clearer, easier to interpret views.
This montage from NASA's Cassini Synthetic Aperture Radar (SAR) images of the surface of Titan shows four examples of how a newly developed technique for handling noise results in clearer, easier to interpret views.

Titan Despeckled Montage

This montage from NASA's Cassini Synthetic Aperture Radar (SAR) images of the surface of Titan shows four examples of how a newly developed technique for handling noise results in clearer, easier to interpret views.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19053
Added: 2015-02-12

Views: 736

Titan Despeckled Montage

This montage from NASA's Cassini Synthetic Aperture Radar (SAR) images of the surface of Titan shows four examples of how a newly developed technique for handling noise results in clearer, easier to interpret views.

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These views from NASA's Cassini Synthetic Aperture Radar (SAR) present a side-by-side comparisons of a traditional view and one made using a new technique called despeckling for handling electronic noise that results in clearer views of Titan's surface.
These views from NASA's Cassini Synthetic Aperture Radar (SAR) present a side-by-side comparisons of a traditional view and one made using a new technique called despeckling for handling electronic noise that results in clearer views of Titan's surface.

Despeckling Ligea Mare

These views from NASA's Cassini Synthetic Aperture Radar (SAR) present a side-by-side comparisons of a traditional view and one made using a new technique called despeckling for handling electronic noise that results in clearer views of Titan's surface.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19052
Added: 2015-02-12

Views: 4550

Despeckling Ligea Mare

These views from NASA's Cassini Synthetic Aperture Radar (SAR) present a side-by-side comparisons of a traditional view and one made using a new technique called despeckling for handling electronic noise that results in clearer views of Titan's surface.

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NASA's Cassini Synthetic Aperture Radar (SAR) image is presented as a perspective view and shows a landscape near the eastern shoreline of Kraken Mare, a hydrocarbon sea in Titan's north polar region.
NASA's Cassini Synthetic Aperture Radar (SAR) image is presented as a perspective view and shows a landscape near the eastern shoreline of Kraken Mare, a hydrocarbon sea in Titan's north polar region.

Perspective on Kraken Mare Shores

NASA's Cassini Synthetic Aperture Radar (SAR) image is presented as a perspective view and shows a landscape near the eastern shoreline of Kraken Mare, a hydrocarbon sea in Titan's north polar region.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19051
Added: 2015-02-12

Views: 1290

Perspective on Kraken Mare Shores

NASA's Cassini Synthetic Aperture Radar (SAR) image is presented as a perspective view and shows a landscape near the eastern shoreline of Kraken Mare, a hydrocarbon sea in Titan's north polar region.

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Many color images are taken by NASA's Cassini spacecraft in red light so scientists can study the often subtle color variations of Saturn's rings. These variations may reveal clues about the chemical composition and physical nature of the rings.
Many color images are taken by NASA's Cassini spacecraft in red light so scientists can study the often subtle color variations of Saturn's rings. These variations may reveal clues about the chemical composition and physical nature of the rings.

Study in Scarlet

Many color images are taken by NASA's Cassini spacecraft in red light so scientists can study the often subtle color variations of Saturn's rings. These variations may reveal clues about the chemical composition and physical nature of the rings.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18301
Added: 2015-02-09

Views: 188

Study in Scarlet

Many color images are taken by NASA's Cassini spacecraft in red light so scientists can study the often subtle color variations of Saturn's rings. These variations may reveal clues about the chemical composition and physical nature of the rings.

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Tiny Epimetheus is dwarfed by adjacent slivers of the A and F rings in this image from NASA's Cassini spacecraft.
Tiny Epimetheus is dwarfed by adjacent slivers of the A and F rings in this image from NASA's Cassini spacecraft.

Deceptively Small

Tiny Epimetheus is dwarfed by adjacent slivers of the A and F rings in this image from NASA's Cassini spacecraft.

Target: Epimetheus
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18302
Added: 2015-02-02

Views: 973

Deceptively Small

Tiny Epimetheus is dwarfed by adjacent slivers of the A and F rings in this image from NASA's Cassini spacecraft.

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Two masters of their craft are caught at work shaping Saturn's rings captured by NASA's Cassini spacecraft. Pandora (upper right) sculpts the F ring. Meanwhile, Daphnis is busy holding open the Keeler gap (bottom center).
Two masters of their craft are caught at work shaping Saturn's rings captured by NASA's Cassini spacecraft. Pandora (upper right) sculpts the F ring. Meanwhile, Daphnis is busy holding open the Keeler gap (bottom center).

The Shapers

Two masters of their craft are caught at work shaping Saturn's rings captured by NASA's Cassini spacecraft. Pandora (upper right) sculpts the F ring. Meanwhile, Daphnis is busy holding open the Keeler gap (bottom center).

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18298
Added: 2015-01-26

Views: 249

The Shapers

Two masters of their craft are caught at work shaping Saturn's rings captured by NASA's Cassini spacecraft. Pandora (upper right) sculpts the F ring. Meanwhile, Daphnis is busy holding open the Keeler gap (bottom center).

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Janus seems to almost stare off into the distance, contemplating deep, moonish thoughts as the F ring stands by at the bottom of this image from NASA's Cassini spacecraft.
Janus seems to almost stare off into the distance, contemplating deep, moonish thoughts as the F ring stands by at the bottom of this image from NASA's Cassini spacecraft.

Contemplative Janus

Janus seems to almost stare off into the distance, contemplating deep, moonish thoughts as the F ring stands by at the bottom of this image from NASA's Cassini spacecraft.

Target: Janus
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18299
Added: 2015-01-19

Views: 322

Contemplative Janus

Janus seems to almost stare off into the distance, contemplating deep, moonish thoughts as the F ring stands by at the bottom of this image from NASA's Cassini spacecraft.

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A bright spot can be seen on the left side of Rhea in this image from NASA's Cassini spacecraft. The spot is the crater Inktomi, named for a Lakota spider spirit.
A bright spot can be seen on the left side of Rhea in this image from NASA's Cassini spacecraft. The spot is the crater Inktomi, named for a Lakota spider spirit.

Little Bright Spot

A bright spot can be seen on the left side of Rhea in this image from NASA's Cassini spacecraft. The spot is the crater Inktomi, named for a Lakota spider spirit.

Target: Rhea
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18300
Added: 2015-01-12

Views: 772

Little Bright Spot

A bright spot can be seen on the left side of Rhea in this image from NASA's Cassini spacecraft. The spot is the crater Inktomi, named for a Lakota spider spirit.

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What's that bright point of light in the outer A ring? It's a star, bright enough to be visible through the ring as seen by NASA's Cassini spacecraft.
What's that bright point of light in the outer A ring? It's a star, bright enough to be visible through the ring as seen by NASA's Cassini spacecraft.

Wish Upon a Star

What's that bright point of light in the outer A ring? It's a star, bright enough to be visible through the ring as seen by NASA's Cassini spacecraft.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18297
Added: 2015-01-05

Views: 2161

Wish Upon a Star

What's that bright point of light in the outer A ring? It's a star, bright enough to be visible through the ring as seen by NASA's Cassini spacecraft.

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NASA's Cassini orbiter looks toward the trailing hemisphere of Mimas.
NASA's Cassini orbiter looks toward the trailing hemisphere of Mimas.

Polar Scars

NASA's Cassini orbiter looks toward the trailing hemisphere of Mimas.

Target: Mimas
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18292
Added: 2014-12-29

Views: 2935

Polar Scars

NASA's Cassini orbiter looks toward the trailing hemisphere of Mimas.

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NASA's Cassini orbiter shows Saturn's main rings, seen here on their 'lit' face, appear much darker than normal. That's because they tend to scatter light back toward its source -- in this case, the Sun.
NASA's Cassini orbiter shows Saturn's main rings, seen here on their 'lit' face, appear much darker than normal. That's because they tend to scatter light back toward its source -- in this case, the Sun.

Darkness

NASA's Cassini orbiter shows Saturn's main rings, seen here on their 'lit' face, appear much darker than normal. That's because they tend to scatter light back toward its source -- in this case, the Sun.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Wide Angle
ID#: PIA18294
Added: 2014-12-22

Views: 2222

Darkness

NASA's Cassini orbiter shows Saturn's main rings, seen here on their 'lit' face, appear much darker than normal. That's because they tend to scatter light back toward its source -- in this case, the Sun.

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NASA's Cassini orbiter shows that Tethys appears to be peeking out from behind Rhea, watching the watcher. Scientists believe that Tethys' surprisingly high albedo is due to the water ice jets emerging from its neighbor, Enceladus.
NASA's Cassini orbiter shows that Tethys appears to be peeking out from behind Rhea, watching the watcher. Scientists believe that Tethys' surprisingly high albedo is due to the water ice jets emerging from its neighbor, Enceladus.

Tethys the Spy

NASA's Cassini orbiter shows that Tethys appears to be peeking out from behind Rhea, watching the watcher. Scientists believe that Tethys' surprisingly high albedo is due to the water ice jets emerging from its neighbor, Enceladus.

Target: Tethys
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18293
Added: 2014-12-15

Views: 1254

Tethys the Spy

NASA's Cassini orbiter shows that Tethys appears to be peeking out from behind Rhea, watching the watcher. Scientists believe that Tethys' surprisingly high albedo is due to the water ice jets emerging from its neighbor, Enceladus.

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Although solid-looking in many images, NASA's Cassini orbiter shows that Saturn's rings are actually translucent.
Although solid-looking in many images, NASA's Cassini orbiter shows that Saturn's rings are actually translucent.

Translucent Rings

Although solid-looking in many images, NASA's Cassini orbiter shows that Saturn's rings are actually translucent.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Wide Angle
ID#: PIA18295
Added: 2014-12-08

Views: 988

Translucent Rings

Although solid-looking in many images, NASA's Cassini orbiter shows that Saturn's rings are actually translucent.

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NASA's Cassini orbiter shows that Enceladus (visible in the lower-left corner of the image) is but a speck before enormous Saturn, but even a small moon can generate big waves of excitement throughout the scientific community.
NASA's Cassini orbiter shows that Enceladus (visible in the lower-left corner of the image) is but a speck before enormous Saturn, but even a small moon can generate big waves of excitement throughout the scientific community.

Mighty Little Dot

NASA's Cassini orbiter shows that Enceladus (visible in the lower-left corner of the image) is but a speck before enormous Saturn, but even a small moon can generate big waves of excitement throughout the scientific community.

Target: Enceladus
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Wide Angle
ID#: PIA18296
Added: 2014-12-01

Views: 1241

Mighty Little Dot

NASA's Cassini orbiter shows that Enceladus (visible in the lower-left corner of the image) is but a speck before enormous Saturn, but even a small moon can generate big waves of excitement throughout the scientific community.

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NASA's Cassini orbiter shows Saturn is circled by its rings (nearly edge-on in this image), as well as by the moons Tethys (the large bright body near the lower right corner) and Mimas (seen as a slight crescent against Saturn's disk above the rings).
NASA's Cassini orbiter shows Saturn is circled by its rings (nearly edge-on in this image), as well as by the moons Tethys (the large bright body near the lower right corner) and Mimas (seen as a slight crescent against Saturn's disk above the rings).

Circling Saturn

NASA's Cassini orbiter shows Saturn is circled by its rings (nearly edge-on in this image), as well as by the moons Tethys (the large bright body near the lower right corner) and Mimas (seen as a slight crescent against Saturn's disk above the rings).

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Wide Angle
ID#: PIA18288
Added: 2014-11-24

Views: 1829

Circling Saturn

NASA's Cassini orbiter shows Saturn is circled by its rings (nearly edge-on in this image), as well as by the moons Tethys (the large bright body near the lower right corner) and Mimas (seen as a slight crescent against Saturn's disk above the rings).

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Nature is an artist, and this time she seems to have let her paints swirl together a bit. What the viewer might perceive to be Saturn's surface captured by NASA's Cassini orbiter is really just the tops of its uppermost cloud layers.
Nature is an artist, and this time she seems to have let her paints swirl together a bit. What the viewer might perceive to be Saturn's surface captured by NASA's Cassini orbiter is really just the tops of its uppermost cloud layers.

Mixing Paints

Nature is an artist, and this time she seems to have let her paints swirl together a bit. What the viewer might perceive to be Saturn's surface captured by NASA's Cassini orbiter is really just the tops of its uppermost cloud layers.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Narrow Angle
ID#: PIA18290
Added: 2014-11-17

Views: 890

Mixing Paints

Nature is an artist, and this time she seems to have let her paints swirl together a bit. What the viewer might perceive to be Saturn's surface captured by NASA's Cassini orbiter is really just the tops of its uppermost cloud layers.

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NASA's Cassini's radar instrument images show that a bright feature appeared in Kraken Mare, Titan's largest sea.
NASA's Cassini's radar instrument images show that a bright feature appeared in Kraken Mare, Titan's largest sea.

Bright Feature Appears in Titan's Kraken Mare

NASA's Cassini's radar instrument images show that a bright feature appeared in Kraken Mare, Titan's largest sea.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19047
Added: 2014-11-10

Views: 2566

Bright Feature Appears in Titan's Kraken Mare

NASA's Cassini's radar instrument images show that a bright feature appeared in Kraken Mare, Titan's largest sea.

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NASA's Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn's moon Titan near the mouth of a large, flooded river valley.
NASA's Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn's moon Titan near the mouth of a large, flooded river valley.

Plumbing Coastal Depths in Titan's Kraken Mare

NASA's Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn's moon Titan near the mouth of a large, flooded river valley.

Target: Titan
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Radar Mapper
ID#: PIA19046
Added: 2014-11-10

Views: 3122

Plumbing Coastal Depths in Titan's Kraken Mare

NASA's Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn's moon Titan near the mouth of a large, flooded river valley.

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A new day dawns on Saturn as the part of the planet is seen emerging once more into the Sun's light by NASA's Cassini orbiter. With an estimated rotation period of 10 hours and 40 minutes, Saturn's days and nights are much shorter than those on Earth.
A new day dawns on Saturn as the part of the planet is seen emerging once more into the Sun's light by NASA's Cassini orbiter. With an estimated rotation period of 10 hours and 40 minutes, Saturn's days and nights are much shorter than those on Earth.

Sunrise on Saturn

A new day dawns on Saturn as the part of the planet is seen emerging once more into the Sun's light by NASA's Cassini orbiter. With an estimated rotation period of 10 hours and 40 minutes, Saturn's days and nights are much shorter than those on Earth.

Target: S Rings
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem - Wide Angle
ID#: PIA18289
Added: 2014-11-10

Views: 3291

Sunrise on Saturn

A new day dawns on Saturn as the part of the planet is seen emerging once more into the Sun's light by NASA's Cassini orbiter. With an estimated rotation period of 10 hours and 40 minutes, Saturn's days and nights are much shorter than those on Earth.

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This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.
This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

Color Maps of Tethys - 2014

This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

Target: Tethys
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem
ID#: PIA18439
Added: 2014-11-04

Views: 2323

Color Maps of Tethys - 2014

This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

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This set of global, color mosaics of Saturn's moon Rhea was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.
This set of global, color mosaics of Saturn's moon Rhea was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

Color Maps of Rhea - 2014

This set of global, color mosaics of Saturn's moon Rhea was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

Target: Rhea
Mission: Cassini-Huygens
Spacecraft: Cassini Orbiter
Instrument: Imaging Science Subsystem
ID#: PIA18438
Added: 2014-11-04

Views: 1959

Color Maps of Rhea - 2014

This set of global, color mosaics of Saturn's moon Rhea was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system.

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