Skip to Main content Skip to Navigation
Conference papers

Composition, seasonal change and bathymetry of Ligeia Mare, Titan, derived from its 2.2-cm thermal emission

Alice Le Gall 1 R.D. Lorenz 2 M.J. Malaska 3 M.A. Janssen 3 T. Tokano 4 A.G. Hayes 5 M. Mastrogiuseppe 5 Gaëlle Veyssière 1
1 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
2 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
3 JPL - Jet Propulsion Laboratory
4 Institut für Geophysik und Meteorologie [Köln]
5 Department of Astronomy [Ithaca]
Abstract : Ligeia Mare is the second largest sea of Saturn's moon Titan. It is also the first extraterritorial sea for which a bathymetry profile was obtained. In this paper, we analyze all data acquired up to July 2013 in the passive mode of the RADAR (i.e., radiometry mode) on board the Cassini probe in order to constrain its composition, seasonal change and bathymetry.
Document type :
Conference papers
Complete list of metadatas

Cited literature [4 references]  Display  Hide  Download
https://hal-insu.archives-ouvertes.fr/insu-01211601
Contributor : Catherine Cardon <>
Submitted on : Monday, October 5, 2015 - 2:14:01 PM
Last modification on : Friday, January 10, 2020 - 3:42:29 PM
Document(s) archivé(s) le : Wednesday, January 6, 2016 - 10:39:06 AM

File

Vignette du document
EPSC2015-504.pdf
Publisher files allowed on an open archive

Identifiers

  • HAL Id : insu-01211601, version 1

Collections

INSU | CNRS | UPMC | UVSQ | LATMOS | UNIV-PARIS-SACLAY | SORBONNE-UNIVERSITE | SU-SCIENCES

Citation

Alice Le Gall, R.D. Lorenz, M.J. Malaska, M.A. Janssen, T. Tokano, et al.. Composition, seasonal change and bathymetry of Ligeia Mare, Titan, derived from its 2.2-cm thermal emission. European Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-504. ⟨insu-01211601⟩

Export

BibTeX TEI DC DCterms EndNote

Share

Metrics

Record views

240

Files downloads

301

Contact

Informations

CCSD