Discovery of Fog at the South Pole of Titan
While Saturn's moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. The indirect evidence, while compelling, could be misleading. It is possible, for example, that the identified lake features could be filled wi...
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ftcaltechauth:oai:authors.library.caltech.edu:bt6gj-jnt96 2024-09-15T18:36:38+00:00 Discovery of Fog at the South Pole of Titan Brown, M. E. Smith, A. L. Chen, C. Ãdámkovics, M. 2009-11-20 https://doi.org/10.1088/0004-637X/706/1/L110 unknown American Astronomical Society https://arxiv.org/abs/0908.4087 https://doi.org/10.1088/0004-637X/706/1/L110 oai:authors.library.caltech.edu:bt6gj-jnt96 eprintid:16821 resolverid:CaltechAUTHORS:20091130-080407164 info:eu-repo/semantics/openAccess Other Astrophysical Journal Letters, 706(1), L110-L113, (2009-11-20) infrared: solar system planets and satellites: individual (Titan) info:eu-repo/semantics/article 2009 ftcaltechauth https://doi.org/10.1088/0004-637X/706/1/L110 2024-08-06T15:35:01Z While Saturn's moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. The indirect evidence, while compelling, could be misleading. It is possible, for example, that the identified lake features could be filled with ethane, an involatile long-term residue of atmospheric photolysis; the apparent stream and channel features could be ancient remnants of a previous climate; and the tropospheric methane clouds, while frequent, could cause no rain to reach the surface. We report here the detection of fog at the south pole of Titan during late summer using observations from the VIMS instrument on board the Cassini spacecraft. While terrestrial fog can form from a variety of causes, most of these processes are inoperable on Titan. Fog on Titan can only be caused by evaporation of nearly pure liquid methane; the detection of fog provides the first direct link between surface and atmospheric methane. Based on the detections presented here, liquid methane appears widespread at the south pole of Titan in late southern summer, and the hydrological cycle on Titan is currently active. © 2009 The American Astronomical Society. Received 2009 August 27; accepted 2009 October 16; published 2009 November 2. This research has been supported by a grant from the NSF Planetary Astronomy program. Published - Brown2009p6413Astrophys_J_Lett.pdf Submitted - 0908.4087.pdf Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) The Astrophysical Journal 706 1 L110 L113 |
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infrared: solar system planets and satellites: individual (Titan) |
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infrared: solar system planets and satellites: individual (Titan) Brown, M. E. Smith, A. L. Chen, C. Ãdámkovics, M. Discovery of Fog at the South Pole of Titan |
topic_facet |
infrared: solar system planets and satellites: individual (Titan) |
description |
While Saturn's moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. The indirect evidence, while compelling, could be misleading. It is possible, for example, that the identified lake features could be filled with ethane, an involatile long-term residue of atmospheric photolysis; the apparent stream and channel features could be ancient remnants of a previous climate; and the tropospheric methane clouds, while frequent, could cause no rain to reach the surface. We report here the detection of fog at the south pole of Titan during late summer using observations from the VIMS instrument on board the Cassini spacecraft. While terrestrial fog can form from a variety of causes, most of these processes are inoperable on Titan. Fog on Titan can only be caused by evaporation of nearly pure liquid methane; the detection of fog provides the first direct link between surface and atmospheric methane. Based on the detections presented here, liquid methane appears widespread at the south pole of Titan in late southern summer, and the hydrological cycle on Titan is currently active. © 2009 The American Astronomical Society. Received 2009 August 27; accepted 2009 October 16; published 2009 November 2. This research has been supported by a grant from the NSF Planetary Astronomy program. Published - Brown2009p6413Astrophys_J_Lett.pdf Submitted - 0908.4087.pdf |
format |
Article in Journal/Newspaper |
author |
Brown, M. E. Smith, A. L. Chen, C. Ãdámkovics, M. |
author_facet |
Brown, M. E. Smith, A. L. Chen, C. Ãdámkovics, M. |
author_sort |
Brown, M. E. |
title |
Discovery of Fog at the South Pole of Titan |
title_short |
Discovery of Fog at the South Pole of Titan |
title_full |
Discovery of Fog at the South Pole of Titan |
title_fullStr |
Discovery of Fog at the South Pole of Titan |
title_full_unstemmed |
Discovery of Fog at the South Pole of Titan |
title_sort |
discovery of fog at the south pole of titan |
publisher |
American Astronomical Society |
publishDate |
2009 |
url |
https://doi.org/10.1088/0004-637X/706/1/L110 |
genre |
South pole |
genre_facet |
South pole |
op_source |
Astrophysical Journal Letters, 706(1), L110-L113, (2009-11-20) |
op_relation |
https://arxiv.org/abs/0908.4087 https://doi.org/10.1088/0004-637X/706/1/L110 oai:authors.library.caltech.edu:bt6gj-jnt96 eprintid:16821 resolverid:CaltechAUTHORS:20091130-080407164 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1088/0004-637X/706/1/L110 |
container_title |
The Astrophysical Journal |
container_volume |
706 |
container_issue |
1 |
container_start_page |
L110 |
op_container_end_page |
L113 |
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1810480325864718336 |