Physical characterization of double asteroid (617) Patroclus from 2007/2012 mutual events observations

Autor: F. Colas, Florent Deleflie, Felipe Braga-Ribas, J. Normand, Hiromi Hamanowa, Alain Klotz, Pascal Descamps, P. Vingerhoets, J. A. Farrell, L. Maquet, K. Archer, G. Dubos, Vishnu Reddy, T. Pauwels, Frédéric Vachier, A. Peyrot, Joe Pollock, F. Marchis, A. Leroy, Pedro V. Sada, Jérôme Berthier, Sylvain Bouley, J.-P. Teng-Chuen-Yu
Přispěvatelé: Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), 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 de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Géosciences Paris Saclay (GEOPS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Association T60, Observatoire Midi-Pyrénées, Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France
Jazyk: angličtina
Rok vydání: 2020
Předmět:
Zdroj: Icarus
Icarus, Elsevier, 2020, ⟨10.1016/j.icarus.2020.113990⟩
Icarus, 2020, ⟨10.1016/j.icarus.2020.113990⟩
HAL
ISSN: 0019-1035
1090-2643
DOI: 10.1016/j.icarus.2020.113990⟩
Popis: International audience; We publish a set of 16 light curves of mutual events inside the synchronous system of the Jupiter Trojan (617) Patroclus. Patroclus is th only binary system of the six target asteroids of the forthcoming NASA Discovery-class mission Lucy. Determining the physical parameters of the system is therefore of primary importance in helping to plan the flyby mission.Light curves were acquired during two follow-up campaigns of 6 months each between January-June 2007 and July-December 2012. Eight small eclipse events of amplitude of 0.2-0.3 mag were recorded in 2007. On the other hand, in 2012, the amplitudes of the phenomena were much deeper, between 0.6 and 0.8 mag, due to a nearly edge-on configuration of the system.We refined the sidereal period to 102.78624 ± 0.00015h = 4.282760 ± 0.000005days. The J2000 ecliptic coordinates of the pole of the system were found to be λ = 235.3 ± 1.2° andβ = - 62.4 ± 0.2°. The volume ratio was determined equal to q = 0.69 ± 0.08. By using a model of inhomogeneous Roche ellipsoids in hydrostatic equilibrium, we derived a bulk density of 0.81 ± 0.16g/cm3 and a surface grain density of 2.69 ± 0.36g/cm3 in agreement with spectroscopic observations of this P-type asteroid.As a validation, our solution was applied to revisit recent results obtained from observations of another type: AO astrometry and stellar occultation. Our model is thus perfectly able to account for these observations after fitting the mutual separation to the value of 695 ± 10km. Consequently, the area-equivalent diameter of the system as a whole is derived DΑ = 168.8 ± 2.6km.
Databáze: OpenAIRE
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