Thermal and mechanical properties of the near-surface layers of comet 67P/Churyumov-Gerasimenko

Author:

Spohn T.1,Knollenberg J.1,Ball A. J.2,Banaszkiewicz M.3,Benkhoff J.2,Grott M.1,Grygorczuk J.3,Hüttig C.1,Hagermann A.4,Kargl G.5,Kaufmann E.4,Kömle N.5,Kührt E.1,Kossacki K. J.6,Marczewski W.3,Pelivan I.1,Schrödter R.1,Seiferlin K.7

Affiliation:

1. Institute of Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany.

2. European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, Netherlands.

3. Space Research Center, Warsaw, Poland.

4. Department of Physical Sciences, The Open University, Milton Keynes, UK.

5. Space Research Institute, Austrian Academy of Sciences Graz, Austria.

6. Faculty of Physics, University of Warsaw, Warsaw, Poland.

7. Physics Institute, University of Berne, Berne, Switzerland.

Abstract

Thermal and mechanical material properties determine comet evolution and even solar system formation because comets are considered remnant volatile-rich planetesimals. Using data from the Multipurpose Sensors for Surface and Sub-Surface Science (MUPUS) instrument package gathered at the Philae landing site Abydos on comet 67P/Churyumov-Gerasimenko, we found the diurnal temperature to vary between 90 and 130 K. The surface emissivity was 0.97, and the local thermal inertia was 85 ± 35 J m −2 K −1 s -1/2 . The MUPUS thermal probe did not fully penetrate the near-surface layers, suggesting a local resistance of the ground to penetration of >4 megapascals, equivalent to >2 megapascal uniaxial compressive strength. A sintered near-surface microporous dust-ice layer with a porosity of 30 to 65% is consistent with the data.

Funder

UK Science and Technology Facilities Council

Helmholtz Association

Austrian Academy of Sciences

Polish Academy of Sciences

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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