Literature DB >> 16319828

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

John C Zarnecki1, Mark R Leese, Brijen Hathi, Andrew J Ball, Axel Hagermann, Martin C Towner, Ralph D Lorenz, J Anthony M McDonnell, Simon F Green, Manish R Patel, Timothy J Ringrose, Philip D Rosenberg, Karl R Atkinson, Mark D Paton, Marek Banaszkiewicz, Benton C Clark, Francesca Ferri, Marcello Fulchignoni, Nadeem A L Ghafoor, Günter Kargl, Håkan Svedhem, John Delderfield, Manuel Grande, David J Parker, Peter G Challenor, John E Geake.   

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 discussion. The Huygens probe entered Titan's atmosphere on 14 January 2005 and descended to the surface using a parachute system. Here we report measurements made just above and on the surface of Titan by the Huygens Surface Science Package. 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.

Year:  2005        PMID: 16319828     DOI: 10.1038/nature04211

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  3 in total

Review 1.  Formation, habitability, and detection of extrasolar moons.

Authors:  René Heller; Darren Williams; David Kipping; Mary Anne Limbach; Edwin Turner; Richard Greenberg; Takanori Sasaki; Emeline Bolmont; Olivier Grasset; Karen Lewis; Rory Barnes; Jorge I Zuluaga
Journal:  Astrobiology       Date:  2014-08-22       Impact factor: 4.335

2.  In situ methods for measuring thermal properties and heat flux on planetary bodies.

Authors:  Norbert I Kömle; Erika S Hütter; Wolfgang Macher; Erika Kaufmann; Günter Kargl; Jörg Knollenberg; Matthias Grott; Tilman Spohn; Roman Wawrzaszek; Marek Banaszkiewicz; Karoly Seweryn; Axel Hagermann
Journal:  Planet Space Sci       Date:  2011-06       Impact factor: 2.030

3.  The Role of Seasonal Sediment Transport and Sintering in Shaping Titan's Landscapes: A Hypothesis.

Authors:  Mathieu G A Lapôtre; Michael J Malaska; Morgan L Cable
Journal:  Geophys Res Lett       Date:  2022-04-25       Impact factor: 5.576

  3 in total

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