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Collection:
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NASA Cassini-Huygens Collection
Collection
NASA Cassini-Huygens Collection
Collection
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Title:
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False Color Look at Enceladus
Title
False Color Look at Enceladus
Title
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Description:
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False Color Look at Enceladus
description
False Color Look at Enceladus
Description
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Full Description:
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A fresh look at Saturn's moon Enceladus reveals tempting new details about the brightest real estate in the solar system. This false-color image shows that some of the linear features on Enceladus have a slightly different color from their surroundings. Different colors of ice may be caused by varying compositions or varying ice crystal sizes. Either of which can indicate different formation mechanisms or different ages. Enceladus is 505 kilometers (314 miles) across. The new view shows some of the smooth plains noted in NASA's Voyager spacecraft images and earlier Cassini images. At about the seven o'clock position are interwoven linear patterns that are reminiscent of the wispy-terrain features on two of Saturn's other moons, Dione and Rhea. Imaging scientists are not sure whether these brighter markings are evidence for contamination of the ice in the linear features by some other material. Analysis of high resolution images of Enceladus should also show whether, like the surprising terrain seen on Dione, the "wisps" are curvilinear fractures that are not quite resolved at this scale. This false color view combines images obtained using filters sensitive to ultraviolet, polarized green and infrared light. The images were obtained with the Cassini spacecraft narrow angle camera on Feb. 16, 2005, at distances ranging from 179,727 to 179,601 kilometers (111,677 to 111,599 miles) from Enceladus and at a Sun-Enceladus-spacec raft, or phase, angle of 22 degrees. Resolution in the image is about 1 kilometer (0.6 mile) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.n
. For images visit the Cassini imaging team home page http://ciclops.org. *Credit:* NASA/JPL/Space Science Institute
Full_Description
A fresh look at Saturn's moon Enceladus reveals tempting new details about the brightest real estate in the solar system. This false-color image shows that some of the linear features on Enceladus have a slightly different color from their surroundings. Different colors of ice may be caused by varying compositions or varying ice crystal sizes. Either of which can indicate different formation mechanisms or different ages. Enceladus is 505 kilometers (314 miles) across. The new view shows some of the smooth plains noted in NASA's Voyager spacecraft images and earlier Cassini images. At about the seven o'clock position are interwoven linear patterns that are reminiscent of the wispy-terrain features on two of Saturn's other moons, Dione and Rhea. Imaging scientists are not sure whether these brighter markings are evidence for contamination of the ice in the linear features by some other material. Analysis of high resolution images of Enceladus should also show whether, like the surprising terrain seen on Dione, the "wisps" are curvilinear fractures that are not quite resolved at this scale. This false color view combines images obtained using filters sensitive to ultraviolet, polarized green and infrared light. The images were obtained with the Cassini spacecraft narrow angle camera on Feb. 16, 2005, at distances ranging from 179,727 to 179,601 kilometers (111,677 to 111,599 miles) from Enceladus and at a Sun-Enceladus-spacec raft, or phase, angle of 22 degrees. Resolution in the image is about 1 kilometer (0.6 mile) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.n
. For images visit the Cassini imaging team home page http://ciclops.org. *Credit:* NASA/JPL/Space Science Institute
Full Description
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Date:
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February 18, 2005
Date
February 18, 2005
Date
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Keywords:
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wispy terrain
keywords
wispy terrain
Keywords
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Keywords:
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Endeladus
keywords
Endeladus
Keywords
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facet_what:
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Saturn
facet_what
Saturn
facet_what
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facet_what:
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Cassini
facet_what
Cassini
facet_what
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facet_what:
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Cassini-Huygens
facet_what
Cassini-Huygens
facet_what
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facet_what:
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Huygens Probe
facet_what
Huygens Probe
facet_what
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facet_what:
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Moon
facet_what
Moon
facet_what
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facet_what:
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Dione
facet_what
Dione
facet_what
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facet_what:
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Cassini Orbiter
facet_what
Cassini Orbiter
facet_what
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facet_what:
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Rhea
facet_what
Rhea
facet_what
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facet_what:
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Sun
facet_what
Sun
facet_what
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facet_what:
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Voyager
facet_what
Voyager
facet_what
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facet_what:
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Enceladus
facet_what
Enceladus
facet_what
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facet_where:
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Saturn
facet_where
Saturn
facet_where
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facet_where:
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Dione
facet_where
Dione
facet_where
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facet_where:
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Jet Propulsion Laboratory
facet_where
Jet Propulsion Laboratory
facet_where
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facet_where:
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California
facet_where
California
facet_where
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facet_where:
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Washington
facet_where
Washington
facet_where
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facet_where:
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Rhea
facet_where
Rhea
facet_where
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facet_where:
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Enceladus
facet_where
Enceladus
facet_where
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facet_where:
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Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
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facet_where:
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Washington, D.C.
facet_where
Washington, D.C.
facet_where
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facet_when:
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February 18, 2005
facet_when
February 18, 2005
facet_when
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facet_when_year:
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2005
facet_when_year
2005
facet_when_year
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UID:
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SPD-SATRN-1386
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original url:
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original_url
original url
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