Transient features in a Titan sea
| dc.contributor.author | HOFGARTNER, J. D. | |
| hal.structure.identifier | Division of Geological and Planetary Sciences [Pasadena] | |
| dc.contributor.author | HAYES, Alexander G. | |
| hal.structure.identifier | University of Arizona | |
| dc.contributor.author | LUNINE, J.I. | |
| hal.structure.identifier | SSE 2014 | |
| dc.contributor.author | PAILLOU, Philippe | |
| dc.contributor.author | AND, All | |
| dc.date.accessioned | 2021-07-07T16:18:55Z | |
| dc.date.available | 2021-07-07T16:18:55Z | |
| dc.date.issued | 2014 | |
| dc.identifier.issn | 1752-0894 | |
| dc.identifier.uri | https://oskar-bordeaux.fr/handle/20.500.12278/96226 | |
| dc.description.abstractEn | Titan's surface-atmosphere system bears remarkable similarities to Earth's, the most striking being an active, global methane cycle akin to Earth's water cycle1, 2. Like the hydrological cycle of Earth, Titan's seasonal methane cycle is driven by changes in the distribution of solar energy2. The Cassini spacecraft, which arrived at Saturn in 2004 in the midst of northern winter and southern summer, has observed surface changes, including shoreline recession, at Titan's south pole3, 4 and equator5. However, active surface processes have yet to be confirmed in the lakes and seas in Titan's north polar region6, 7, 8. As the 2017 northern summer solstice approaches, the onset of dynamic phenomena in this region is expected6, 7, 9, 10, 11, 12. Here we present the discovery of bright features in recent Cassini RADAR data that appeared in Titan's northern sea, Ligeia Mare, in July 2013 and disappeared in subsequent observations. We suggest that these bright features are best explained by the occurrence of ephemeral phenomena such as surface waves, rising bubbles, and suspended or floating solids. We suggest that our observations are an initial glimpse of dynamic processes that are commencing in the northern lakes and seas as summer nears in the northern hemisphere. | |
| dc.language.iso | en | |
| dc.publisher | Nature Publishing Group | |
| dc.title.en | Transient features in a Titan sea | |
| dc.type | Article de revue | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
| bordeaux.journal | Nature Geoscience | |
| bordeaux.page | online | |
| bordeaux.hal.laboratories | Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804 | * |
| bordeaux.institution | CNRS | |
| bordeaux.institution | Université de Bordeaux | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-01012060 | |
| hal.version | 1 | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-01012060v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Nature%20Geoscience&rft.date=2014&rft.spage=online&rft.epage=online&rft.eissn=1752-0894&rft.issn=1752-0894&rft.au=HOFGARTNER,%20J.%20D.&HAYES,%20Alexander%20G.&LUNINE,%20J.I.&PAILLOU,%20Philippe&AND,%20All&rft.genre=article |
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