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A soft solid surface on Titan as revealed by the Huygens Surface Science Package

Authors :
Marcello Fulchignoni
B. Hathi
Mark Paton
Andrew J. Ball
John C. Zarnecki
D. J. Parker
Marek Banaszkiewicz
J. E. Geake
K.R. Atkinson
Peter Challenor
Manuel Grande
J. Delderfield
J. Anthony M. McDonnell
Mark Leese
T. J. Ringrose
Günter Kargl
Manish R. Patel
Nadeem Ghafoor
Francesca Ferri
Benton C. Clark
Håkan Svedhem
Axel Hagermann
Martin C. Towner
Simon F. Green
Ralph D. Lorenz
Philip D. Rosenberg
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Pôle Planétologie du LESIA
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
Nature, Nature, 2005, 438, pp.792-795. ⟨10.1038/nature04211⟩, ResearcherID
Publication Year :
2005
Publisher :
HAL CCSD, 2005.

Abstract

The surface of Saturn's largest satellite —Titan — is largely obscured by an optically thick atmospheric haze, and so its nature has been the subject of considerable speculation and discussion1. The Huygens probe entered Titan's atmosphere on 14 January 2005 and descended to the surface using a parachute system2. Here we report measurements made just above and on the surface of Titan by the Huygens Surface Science Package3, 4. Acoustic sounding over the last 90 m above the surface reveals a relatively smooth, but not completely flat, surface surrounding the landing site. Penetrometry and accelerometry measurements during the probe impact event reveal that the surface was neither hard (like solid ice) nor very compressible (like a blanket of fluffy aerosol); rather, the Huygens probe landed on a relatively soft solid surface whose properties are analogous to wet clay, lightly packed snow and wet or dry sand. The probe settled gradually by a few millimetres after landing.

Details

Language :
English
ISSN :
00280836 and 14764687
Database :
OpenAIRE
Journal :
Nature, Nature, 2005, 438, pp.792-795. ⟨10.1038/nature04211⟩, ResearcherID
Accession number :
edsair.doi.dedup.....24b9ae4f2d65a62170cda2aad0ac3add
Full Text :
https://doi.org/10.1038/nature04211⟩