Homogeneous Internal Structure of CM-Like Asteroid (41) Daphne?,?? B
A&A 623, A132 (2019) Astronomy https://doi.org/10.1051/0004-6361/201833898 & © B. Carry et al. 2019 Astrophysics Homogeneous internal structure of CM-like asteroid (41) Daphne?,?? B. Carry1, F. Vachier2, J. Berthier2, M. Marsset3, P. Vernazza4, J. Grice1,5, W. J. Merline6, E. Lagadec1, A. Fienga7, A. Conrad8, E. Podlewska-Gaca9,11, T. Santana-Ros9, M. Viikinkoski12, J. Hanuš14, C. Dumas15, J. D. Drummond16, P. M. Tamblyn6,17, C. R. Chapman6, R. Behrend18, L. Bernasconi18, P. Bartczak9, Z. Benkhaldoun10, M. Birlan2, J. Castillo-Rogez19, F. Cipriani20, F. Colas2, A. Drouard4, J. Durechˇ 14, B. L. Enke6, S. Fauvaud18,21, M. Ferrais22, R. Fetick4, T. Fusco4, M. Gillon22, E. Jehin22, L. Jorda4, M. Kaasalainen12, M. Keppler13, A. Kryszczynska9, P. Lamy4, F. Marchis23, A. Marciniak9, T. Michalowski9, P. Michel1, M. Pajuelo2,24, P. Tanga1, A. Vigan4, B. Warner25, O. Witasse20, B. Yang26, and A. Zurlo4,27,28 (Affiliations can be found after the references) Received 18 July 2018 / Accepted 7 January 2019 ABSTRACT Context. CM-like asteroids (Ch and Cgh classes) are a major population within the broader C-complex, encompassing about 10% of the mass of the main asteroid belt. Their internal structure has been predicted to be homogeneous, based on their compositional similarity as inferred from spectroscopy and numerical modeling of their early thermal evolution. Aims. Here we aim to test this hypothesis by deriving the density of the CM-like asteroid (41) Daphne from detailed modeling of its shape and the orbit of its small satellite. Methods. We observed Daphne and its satellite within our imaging survey with the Very Large Telescope extreme adaptive-optics SPHERE/ZIMPOL camera and complemented this data set with earlier Keck/NIRC2 and VLT/NACO observations.
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