Author
Listed:
- M. Pätzold
(Rheinisches Institut für Umweltforschung an der Universität zu Köln)
- T. Andert
(Institut für Raumfahrttechnik und Weltraumnutzung, Universität der Bundeswehr München)
- M. Hahn
(Rheinisches Institut für Umweltforschung an der Universität zu Köln)
- S. W. Asmar
(Jet Propulsion Laboratory, Caltech)
- J.-P. Barriot
(Université de la Polynésie Francaise)
- M. K. Bird
(Rheinisches Institut für Umweltforschung an der Universität zu Köln)
- B. Häusler
(Institut für Raumfahrttechnik und Weltraumnutzung, Universität der Bundeswehr München)
- K. Peter
(Rheinisches Institut für Umweltforschung an der Universität zu Köln)
- S. Tellmann
(Rheinisches Institut für Umweltforschung an der Universität zu Köln)
- E. Grün
(Max-Planck-Institut für Kernphysik)
- P. R. Weissman
(Planetary Science Institute)
- H. Sierks
(Max-Planck-Institut für Sonnensystemforschung)
- L. Jorda
(Laboratoire d’Astrophysique de Marseille)
- R. Gaskell
(Planetary Science Institute)
- F. Preusker
(Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt (DLR) Berlin-Adlershof)
- F. Scholten
(Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt (DLR) Berlin-Adlershof)
Abstract
The precise mass, bulk density, porosity and internal structure of the nucleus of comet 67P/Churyumov–Gerasimenko are calculated, on the basis of its gravity field, showing it to be dusty, homogeneous, low-density and highly porous.
Suggested Citation
M. Pätzold & T. Andert & M. Hahn & S. W. Asmar & J.-P. Barriot & M. K. Bird & B. Häusler & K. Peter & S. Tellmann & E. Grün & P. R. Weissman & H. Sierks & L. Jorda & R. Gaskell & F. Preusker & F. Scho, 2016.
"A homogeneous nucleus for comet 67P/Churyumov–Gerasimenko from its gravity field,"
Nature, Nature, vol. 530(7588), pages 63-65, February.
Handle:
RePEc:nat:nature:v:530:y:2016:i:7588:d:10.1038_nature16535
DOI: 10.1038/nature16535
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