Issue |
A&A
Volume 590, June 2016
|
|
---|---|---|
Article Number | A46 | |
Number of page(s) | 15 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201528029 | |
Published online | 10 May 2016 |
Possible interpretation of the precession of comet 67P/Churyumov-Gerasimenko
1
Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n., 18080
Granada, Spain
2
Aix-Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique
de Marseille) UMR 7326, 13388
Marseille,
France
3
Planetary Science Institute, Tucson, Arizona
85719,
USA
4
Department of Physics and Astronomy, Uppsala
University, Box
516, 75120
Uppsala,
Sweden
5
German Aerospace Center (DLR), Institut für
Planetenforschung, Rutherfordstraße
2, 12489
Berlin,
Germany
6
Institut für Geophysik und extraterrestrische Physik (IGEP),
Technische Universität Braunschweig, Mendelssohnstraße 3, 38106
Braunschweig,
Germany
7
IMCCE/Observatoire de Paris, 61 avenue de l’Observatoire, 75014
Paris,
France
8
Centro de Astrobiología (INTA-CSIC), European Space Agency (ESA),
European Space Astronomy Centre (ESAC), PO Box 78, 28691
Villanueva de la Cañada,
Madrid,
Spain
9
International Space Science Institute,
Hallerstraße 6, 3012
Bern,
Switzerland
10
Max-Planck-Institut für Sonnensystemforschung,
Justus-von-Liebig-Weg 3,
37077
Göttingen,
Germany
11
University of Padova, Department of Physics and
Astronomy, Vicolo dell’Osservatorio
3, 35122
Padova,
Italy
12
Scientific Support Office, European Space Research and Technology
Centre/ESA, Keplerlaan 1, Postbus
299, 2201 AZ
Noordwijk ZH, The
Netherlands
13
PAS Space Research Center, Bartycka 18A,
00716
Warszawa,
Poland
14
University of Maryland, Department of Astronomy,
College Park, MD
20742-2421,
USA
15 LESIA-Observatoire de Paris, CNRS,
Université Pierre et Marie Curie, Université Paris Diderot,
5 place J. Janssen,
92195
Meudon Principal Cedex
France
16
LATMOS, CNRS/UVSQ/IPSL, 11 boulevard d’Alembert, 78280
Guyancourt,
France
17
Centro di Ateneo di Studi ed Attivitá Spaziali “Giuseppe Colombo”
(CISAS), University of Padova, via
Venezia 15, 35131
Padova,
Italy
18
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
19
CNR-IFN UOS Padova LUXOR, Via Trasea, 7, 35131
Padova,
Italy
20
Department of Information Engineering, University of
Padova, via Gradenigo,
6/B, 35131
Padova,
Italy
21
University of Trento, via Sommarive, 9, 38123
Trento,
Italy
22
Physikalisches Institut der Universität Bern,
Sidlerstr. 5, 3012
Bern,
Switzerland
23
INAF – Osservatorio Astronomico di Trieste,
via Tiepolo 11, 34014
Trieste,
Italy
24
Graduate Institute of Astronomy, National Central
University, 300 Chung-Da
Rd, 32054
Chung-Li,
Taiwan
25 Operations Department, European
Space Astronomy Centre/ESA, PO Box
78, 28691
Villanueva de la Cañada (Madrid),
Spain
26
Solar System Exploration Research Virtual Institute, Southwest
Research Institute, 1050 Walnut
St., Suite 300, Boulder, CO
80302,
USA
27
Instituto Nacional de Tecnica Aeroespacial,
Carretera de Ajalvir, p.k. 4, 28850 Torrejon de
Ardoz, Madrid,
Spain
28
Center for Space and Habitability, University of
Bern, 3012
Bern,
Switzerland
29
MTA CSFK Konkoly Observatory, 1121
Budapest,
Hungary
Received: 22 December 2015
Accepted: 15 March 2016
Context. Data derived from the reconstruction of the nucleus shape of comet 67P/Churyumov-Gerasimenko (67P) from images of the OSIRIS camera onboard ROSETTA show evidence that the nucleus rotates in complex mode. First, the orientation of the spin axis is not fixed in an inertial reference frame, which suggests a precessing motion around the angular momentum vector with a periodicity of approximately 257 h ± 12 h.Second, periodograms of the right ascension and declination (RA/Dec) coordinates of the body-frame Z axis show a very significant (higher than 99.99%) periodicity at 276 h ± 12 h, different from the rotational period of 12.40 h as previously determined from light-curve analysis.
Aims. The main goal is to interpret the data and associated periodicities of the spin axis orientation in space.
Methods. We analyzed the spin axis orientation in space and associated periodicities and compared them with solutions of Euler equations under the assumption that the body rotates in torque-free conditions. Statistical tests comparing the observationally derived spin axis orientation with the outcome from simulations were applied to determine the most likely inertia moments, excitation level, and periods.
Results. Under the assumption that the body is solid-rigid and rotates in torque-free conditions, the most likely interpretation is that 67P is spinning around the principal axis with the highest inertia moment with a period of about 13 h. At the same time, the comet precesses around the angular momentum vector with a period of about 6.35 h. While the rotating period of such a body would be about 12.4 h, RA/Dec coordinates of the spin axis would have a periodicity of about 270 h as a result of the combination of the two aforementioned motions.
Conclusions. The most direct and simple interpretation of the complex rotation of 67P requires a ratio of inertia moments significantly higher than that of a homogeneous body.
Key words: comets: general / comets: individual: 67P/Churyumov-Gerasimenko
© ESO, 2016
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