Evidence for differentiation of the most primitive small bodies

• Published in: Astronomy & Astrophysics
• Main Authors: Carry, Benoît, Vernazza, Pierre, Vachier, Frédéric, Neveu, Marc, Berthier, Jérôme, Hanuš, Josef, Ferrais, Marin, Jorda, Laurent, Marsset, Michaël, Viikinkoski, Matti, Bartczak, Przemyslaw, Behrend, Raoul, Benkhaldoun, Zouhair, Birlan, Mirel, Castillo-Rogez, Julie, Cipriani, Fabrice, Colas, François, Drouard, Alexis, Dudziński, Grzegorz, Desmars, Josselin, Dumas, Christophe, Ďurech, Josef, Fétick, Romain, Fusco, Thierry, Grice, Jonny, Jehin, Emmanuel, Kaasalainen, Mikko, Kryszczynska, Agnieszka, Lamy, Philippe, Marchis, Franck, Marciniak, Anna, Michalowski, Tadeusz, Michel, Patrick, Pajuelo, Myriam, Podlewska-Gaca, Edyta, Rambaux, Nicolas, Santana-Ros, Toni, Storrs, Alexander, Tanga, Paolo, Vigan, Arthur, Warner, Brian, Wieczorek, Mark, Witasse, Olivier, Yang, Bin
• Other Authors: Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal
• Format: Article in Journal/Newspaper
• Language: English
• Published: EDP Sciences 2021
• Subjects: Minor planets; asteroids: general; Kuiper belt: general; asteroids: individual: Sylvia; Física Aplicada; Jupiter; Tagish; Tagish Lake
• Online Access: http://hdl.handle.net/10045/116358; https://doi.org/10.1051/0004-6361/202140342

Context. 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, comets, and small Kuiper belt objects (KBOs). Indeed, the spectra...