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List		 Addition DateSort Ascending Target Mission Instrument Size
Add Image to Favorite List 2004-07-03 Titan Cassini-Huygens
 Ion and Neutral Mass Spectrometer
Magnetospheric Imaging Instrument (MIMI)
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Images from the magnetospheric imaging instrument and the ion and neutral camera onboard NASA's Cassini spacecraft reveal aspects of the interactions between Saturn's dynamic population of hot energetic ions and the clouds of cold neutral atoms.
PIA06409:
Neutral Gas Cloud Around Titan
Full Resolution:     TIFF (311.9 kB)     JPEG (17.75 kB)
Add Image to Favorite List 2004-10-27 Titan Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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This graph shows data acquired by NASA's Cassini spacecraft as it flew by Titan at an altitude of 1,200 kilometers (745 miles) on Oct. 26, 2004 revealing a diversity of hydrocarbons in the high atmosphere above Titan.
PIA06980:
Lots of Hydrocarbons
Full Resolution:     TIFF (583.9 kB)     JPEG (142.1 kB)
Add Image to Favorite List 2004-10-27 Titan Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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This graph shows data acquired by NASA's Cassini spacecraft as it flew by Titan at an altitude of 1,200 kilometers (745 miles) on Oct. 26, 2004 revealing the amount of light nitrogen in the atmosphere of Titan is much less than that around other planets.
PIA06981:
Case of the Lost Atmosphere
Full Resolution:     TIFF (98.87 kB)     JPEG (27.12 kB)
Add Image to Favorite List 2005-04-22 Titan Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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During its closest flyby of Saturn's moon Titan on April 16, NASA's Cassini spacecraft came within 1,025 kilometers (637 miles) of the moon's surface and found that the outer layer of the thick, hazy atmosphere is brimming with complex hydrocarbons.
PIA07865:
Titan's Upper Atmosphere: A "Factory" of Hydrocarbons
Full Resolution:     TIFF (1.168 MB)     JPEG (49.75 kB)
Add Image to Favorite List 2005-08-30 Enceladus Cassini-Huygens
 Ion and Neutral Mass Spectrometer
Cosmic Dust Analyzer
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This plot shows results from NASA's Cassini's ion neutral mass spectrometer and cosmic dust analyzer, obtained during the spacecraft's close approach to Enceladus on July 14, 2005.
PIA03553:
Water Vapor & Particles Over Enceladus
Full Resolution:     TIFF (2.5 MB)     JPEG (63.22 kB)
Add Image to Favorite List 2008-03-26 Enceladus Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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The lower panel is a mass spectrum that shows the chemical constituents sampled in Saturn's moon Enceladus' plume by NASA's Cassini Ion and Neutral Mass Spectrometer during its fly-through of the plume on Mar. 12, 2008.
PIA10356:
Enceladus Plume Neutral Mass Spectrum
Full Resolution:     TIFF (4.674 MB)     JPEG (102.5 kB)
Add Image to Favorite List 2008-03-26 Enceladus Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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This graph from the Ion and Neutral Mass Spectrometer onboard NASA's Cassini spacecraft shows the range of cometary values with similar chemistry as Saturn's moon Enceladus.
PIA10357:
Comets and Enceladus - Similar Chemistry
Full Resolution:     TIFF (4.674 MB)     JPEG (114.6 kB)
Add Image to Favorite List 2008-03-26 Enceladus Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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The number of water particles in Enceladus' plume peaked over the area highlighted by the circle in this image of Saturn's moon Enceladus, which is overlain by data from NASA's Cassini Ion and Neutral Mass Spectrometer.
PIA10362:
Peak Water Density
Full Resolution:     TIFF (14.83 MB)     JPEG (197.3 kB)
Add Image to Favorite List 2017-04-13 Enceladus Cassini-Huygens
 Ion and Neutral Mass Spectrometer
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This graphic illustrates how Cassini scientists think water interacts with rock at the bottom of the ocean of Saturn's icy moon Enceladus, producing hydrogen gas.
PIA21442:
Enceladus Hydrothermal Activity
Full Resolution:     TIFF (12.23 MB)     JPEG (494.7 kB)
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