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This bar indicates that you are within the PDS enterprise which includes 6 science discipline nodes and 2 support nodes which are overseen by the Project Management Office at NASA's Goddard Space Flight Center (GSFC). Each node is led by an expert in the subject discipline, supported by an advisory group of other practitioners of that discipline, and subject to selection and approval under a regular NASA Research Announcement.
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List		 Addition DateSort Ascending Target Mission Instrument Size
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 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 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 2004-07-03 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)
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