Nearinfrared spectral mapping of Titan's mountains and channels
Cassini studies of the surface of Titan are beginning to reveal its nature. In addition to hills, channels, and cobbles seen by the Huygens probe, the Visual and Infrared Mapping Spectrometer (VIMS) and RADAR instruments onboard the orbiter have seen sand dunes , channels , mountains [5, 6], and cry...
| Main Authors: | , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Conference Object |
| Language: | English |
| Published: |
Lunar and Planetary Institute, Houston
2007
|
| Subjects: | |
| Online Access: | https://elib.dlr.de/51374/ https://elib.dlr.de/51374/1/2028.pdf http://www.lpi.usra.edu/meetings/lpsc2007/pdf/2028.pdf |
| _version_ | 1835018598481920000 |
|---|---|
| author | Barnes, J.W. Radebaugh, J. Brown, R.H. Wall, S. Soderblum, L. Lunine, J. Buratti, B.J. Baines, K.H. Sotin, C. Le Mouelic, S. Rodriguez, S. Clark, R.N. Nicholson, P.D. Jaumann, Ralf Lopes, R. Mitchell, K. Lorenz, R. Wood, C.A. |
| author_facet | Barnes, J.W. Radebaugh, J. Brown, R.H. Wall, S. Soderblum, L. Lunine, J. Buratti, B.J. Baines, K.H. Sotin, C. Le Mouelic, S. Rodriguez, S. Clark, R.N. Nicholson, P.D. Jaumann, Ralf Lopes, R. Mitchell, K. Lorenz, R. Wood, C.A. |
| author_sort | Barnes, J.W. |
| collection | Unknown |
| description | Cassini studies of the surface of Titan are beginning to reveal its nature. In addition to hills, channels, and cobbles seen by the Huygens probe, the Visual and Infrared Mapping Spectrometer (VIMS) and RADAR instruments onboard the orbiter have seen sand dunes , channels , mountains [5, 6], and cryovolcanic candidates. Recently the RADAR team announced the discovery of possible lakes near Titan’s north pole. |
| format | Conference Object |
| genre | North Pole |
| genre_facet | North Pole |
| geographic | North Pole |
| geographic_facet | North Pole |
| id | ftdlr:oai:elib.dlr.de:51374 |
| institution | Open Polar |
| language | English |
| op_collection_id | ftdlr |
| op_relation | https://elib.dlr.de/51374/1/2028.pdf Barnes, J.W. und Radebaugh, J. und Brown, R.H. und Wall, S. und Soderblum, L. und Lunine, J. und Buratti, B.J. und Baines, K.H. und Sotin, C. und Le Mouelic, S. und Rodriguez, S. und Clark, R.N. und Nicholson, P.D. und Jaumann, Ralf und Lopes, R. und Mitchell, K. und Lorenz, R. und Wood, C.A. (2007) Nearinfrared spectral mapping of Titan's mountains and channels. In: Lunar and Planetary Science XXXVIII, 1338, Abstract#2028. Lunar and Planetary Institute, Houston. 38th Lunar and Plantetary Science Conference, 2007-03-12 - 2007-03-16, League City, TX (USA). ISSN 1540-7845. |
| publishDate | 2007 |
| publisher | Lunar and Planetary Institute, Houston |
| record_format | openpolar |
| spelling | ftdlr:oai:elib.dlr.de:51374 2025-06-15T14:43:51+00:00 Nearinfrared spectral mapping of Titan's mountains and channels Barnes, J.W. Radebaugh, J. Brown, R.H. Wall, S. Soderblum, L. Lunine, J. Buratti, B.J. Baines, K.H. Sotin, C. Le Mouelic, S. Rodriguez, S. Clark, R.N. Nicholson, P.D. Jaumann, Ralf Lopes, R. Mitchell, K. Lorenz, R. Wood, C.A. 2007 application/pdf https://elib.dlr.de/51374/ https://elib.dlr.de/51374/1/2028.pdf http://www.lpi.usra.edu/meetings/lpsc2007/pdf/2028.pdf en eng Lunar and Planetary Institute, Houston https://elib.dlr.de/51374/1/2028.pdf Barnes, J.W. und Radebaugh, J. und Brown, R.H. und Wall, S. und Soderblum, L. und Lunine, J. und Buratti, B.J. und Baines, K.H. und Sotin, C. und Le Mouelic, S. und Rodriguez, S. und Clark, R.N. und Nicholson, P.D. und Jaumann, Ralf und Lopes, R. und Mitchell, K. und Lorenz, R. und Wood, C.A. (2007) Nearinfrared spectral mapping of Titan's mountains and channels. In: Lunar and Planetary Science XXXVIII, 1338, Abstract#2028. Lunar and Planetary Institute, Houston. 38th Lunar and Plantetary Science Conference, 2007-03-12 - 2007-03-16, League City, TX (USA). ISSN 1540-7845. Institut für Planetenforschung Konferenzbeitrag PeerReviewed 2007 ftdlr 2025-06-04T04:58:09Z Cassini studies of the surface of Titan are beginning to reveal its nature. In addition to hills, channels, and cobbles seen by the Huygens probe, the Visual and Infrared Mapping Spectrometer (VIMS) and RADAR instruments onboard the orbiter have seen sand dunes , channels , mountains [5, 6], and cryovolcanic candidates. Recently the RADAR team announced the discovery of possible lakes near Titan’s north pole. Conference Object North Pole Unknown North Pole |
| spellingShingle | Institut für Planetenforschung Barnes, J.W. Radebaugh, J. Brown, R.H. Wall, S. Soderblum, L. Lunine, J. Buratti, B.J. Baines, K.H. Sotin, C. Le Mouelic, S. Rodriguez, S. Clark, R.N. Nicholson, P.D. Jaumann, Ralf Lopes, R. Mitchell, K. Lorenz, R. Wood, C.A. Nearinfrared spectral mapping of Titan's mountains and channels |
| title | Nearinfrared spectral mapping of Titan's mountains and channels |
| title_full | Nearinfrared spectral mapping of Titan's mountains and channels |
| title_fullStr | Nearinfrared spectral mapping of Titan's mountains and channels |
| title_full_unstemmed | Nearinfrared spectral mapping of Titan's mountains and channels |
| title_short | Nearinfrared spectral mapping of Titan's mountains and channels |
| title_sort | nearinfrared spectral mapping of titan's mountains and channels |
| topic | Institut für Planetenforschung |
| topic_facet | Institut für Planetenforschung |
| url | https://elib.dlr.de/51374/ https://elib.dlr.de/51374/1/2028.pdf http://www.lpi.usra.edu/meetings/lpsc2007/pdf/2028.pdf |