Evidence for differentiation of the most primitive small bodies

• Published in: Astronomy & Astrophysics
• Main Authors: Carry, Benoit, Vernazza, P., Vachier, F., Neveu, M., Berthier, J., Hanuš, J., Ferrais, M., Jorda, Laurent, Marsset, M., Viikinkoski, M., Bartczak, P., Behrend, R., Benkhaldoun, Z., Birlan, M, Castillo-Rogez, J., Cipriani, F., Colas, F, Drouard, A., Dudziński, G., Desmars, J., Dumas, C., Ďurech, J., Fetick, R., Fusco, T., Grice, J., Jehin, E., Kaasalainen, M., Kryszczynska, A., Lamy, Philippe, Marchis, F., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Podlewska-Gaca, E., Rambaux, N., Santana-Ros, T., Storrs, A., Tanga, P., Vigan, A., Warner, B., Wieczorek, M., Witasse, Olivier, Yang, Bin
• Other Authors: Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (. - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS), 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), University of Maryland College Park, University of Maryland System, NASA Goddard Space Flight Center (GSFC), Institute of Astronomy Prague, Charles University Prague (CU), Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, Department of Earth, Atmospheric and Planetary Sciences MIT, Cambridge (EAPS), Massachusetts Institute of Technology (MIT), Department of Mathematics Tampere, Tampere University of Technology Tampere (TUT), Astronomical Observatory Poznan, Adam Mickiewicz University in Poznań (UAM), Geneva Observatory, University of Geneva Switzerland, Oukaimeden Observatory, Université Cadi Ayyad Marrakech (UCA), Astronomical Institute of Romanian Academy, Romanian Academy, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Institut Polytechnique des Sciences Avancées (IPSA), Thirty Meter Telescope Observatory, The Open University Milton Keynes (OU), University of Tampere Finland, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), SETI Institute, Pontificia Universidad Católica del Perú (PUCP), Institute of Physics Szczecin, University of Szczecin, Universidad de Alicante, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), Towson University Towson, MD, United States, Center for Solar System Studies (CS3), European Southern Observatory (ESO)
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 2021
• Subjects: Minor planets; asteroids; Sylvia; Kuiper belt; [SDU]Sciences of the Universe [physics]; Jupiter; Tagish; Tagish Lake
• Online Access: https://hal-insu.archives-ouvertes.fr/insu-03184663; https://hal-insu.archives-ouvertes.fr/insu-03184663v2/document; https://hal-insu.archives-ouvertes.fr/insu-03184663v2/file/aa40342-21.pdf; https://doi.org/10.1051/0004-6361/202140342

International audience Dynamical models of Solar System evolution have suggested that the so-called P-and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related to the Jupiter Trojans, the comets and small Kuiper-belt objects (KBOs)...