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New and updated convex shape models of asteroids based on optical data from a large collaboration network

2015; EDP Sciences; Volume: 586; Linguagem: Inglês

10.1051/0004-6361/201527441

1432-0746

J. Hanuš, Josef Ďurech, Dagmara Oszkiewicz, R. Behrend, B. Carry, Marco Delbó, Ouorou Adam, V. V. Afonina, R. Anquetin, P. Antonini, L. Arnold, M. Audejean, P. Aurard, M. Bachschmidt, B. Baduel, E. Barbotin, Pierre Barroy, P. Baudouin, L. Berard, Nicolas Berger, L. Bernasconi, J. G. Bosch, Sylvain Bouley, I. Bozhinova, James W. Brinsfield, L. Brunetto, G. Canaud, J. Caron, F. Carrier, Giovanni Battista Casalnuovo, Silvano Casulli, M. Cerda, L. Chalamet, S. Charbonnel, Benedetto Chinaglia, Aleksandar Cikota, F. Colas, J.-F. Coliac, Agwilh Collet, J. M. Coloma, M. Conjat, E. Conseil, R. Costa, R. Crippa, M. Cristofanelli, Y. Damerdji, André Debackère, Alice Decock, Q. Déhais, T. Déléage, S. Delmelle, C. Demeautis, M. Dróżdż, G. Dubos, T. Dulcamara, M. Dumont, Russell I. Durkee, R. Dymock, A. Escalante del Valle, N. Esseiva, R. Esseiva, M. Esteban, Thomas Fauchez, M. Fauerbach, M. Fauvaud, S. Fauvaud, E. Forné, C. Fournel, D. Fradet, J. Garlitz, O. Gerteis, C. Gillier, M. Gillon, R. Giraud, J.-P. Godard, R. Gonçalves, Hiroko Hamanowa, Hiromi Hamanowa, K. L. Hay, S. Hellmich, S. Heterier, David Higgins, R. Hirsch, Gabriella Hodosán, M. Hren, A. P. S. Hygate, N. Innocent, H. Jacquinot, S. Jawahar, Emmanuël Jehin, L. Jerosimic, A. Klotz, W. Koff, P. Korlevic, E. Kosturkiewicz, P. Krafft, Yu. N. Krugly, F. Kugel, O. Labrevoir, J. Lecacheux, M. Lehký, A. Leroy, B. Lesquerbault, M. J. López-Gonzáles, Mikaël Lutz, B. Mallecot, Jean Manfroid, F. Manzini, A. Marciniak, Amaya Moro‐Martín, B. Modave, R. Montaigut, J. Montier, Etienne Morelle, B. Morton, S. Mottola, R. Naves, J. Nomen, Julian Oey, W. Ogłoza, M. Paiella, H. Pallares, A. Peyrot, Frederick Pilcher, Jacques Pirenne, Pierre Piron, M. Polińska, M. Polotto, R. Poncy, J. P. Previt, F. Reignier, D. Renauld, D. Ricci, F. Richard, C. Rinner, V. Risoldi, Denis Robilliard, D. Romeuf, Guy Rousseau, R. Roy, John C. Ruthroff, P. A. Salom, Luigi Salvador, Salvador Sánchez, T. Santana-Ros, A. Scholz, G. Séné, B. A. Skiff, K. Sobkowiak, P. Sogorb, F. Soldán, A. Spiridakis, E. Splanska, S. Sposetti, D. Starkey, Robert D. Stephens, A. Stiepen, R. Stoss, J. Strajnic, J. P. Teng, G. Tumolo, A. Vagnozzi, B. Vanoutryve, J.-M. Vugnon, B. Warner, M. Waucomont, O. Wertz, M. Winiarski, M. Wolf,

Geological and Geochemical Analysis

Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. These efforts already provided deep insight into physical properties of main-belt asteroids or large collisional families. Going into finer detail (e.g., smaller collisional families, asteroids with sizes ≲20 km) requires knowledge of physical parameters of more objects.