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Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution
Hanuš, J. and Durech, J. and Brož, M. and Marciniak, A. and Warner, B. D. and Pilcher, F. and Stephens, R. and Behrend, R. and Carry, B. and Čapek, D. and Antonini, P. and Audejean, M. and Augustesen, K. and Barbotin, E. and Baudouin, P. and Bayol, A. and Bernasconi, L. and Borczyk, W. and Bosch, J.-G. and Brochard, E. and Brunetto, L. and Casulli, S. and Cazenave, A. and Charbonnel, S. and Christophe, B. and Colas, F. and Coloma, J. and Conjat, M. and Cooney, W. and Correira, H. and Cotrez, V. and Coupier, A. and Crippa, R. and Cristofanelli, M. and Dalmas, Ch. and Danavaro, C. and Demeautis, C. and Droege, T. and Durkee, R. and Esseiva, N. and Esteban, M. and Fagas, M. and Farroni, G. and Fauvaud, M. and Fauvaud, S. and Del Freo, F. and Garcia, L. and Geier, S. and Godon, C. and Grangeon, K. and Hamanowa, H. and Hamanowa, H. and Heck, N. and Hellmich, S. and Higgins, D. and Hirsch, R. and Husarik, M. and Itkonen, T. and Jade, O. and Kamiński, K. and Kankiewicz, P. and Klotz, A. and Koff, R. A. and Kryszczyńska, A. and Kwiatkowski, T. and Laffont, A. and Leroy, A. and Lecacheux, J. and Leonie, Y. and Leyrat, C. and Manzini, F. and Martin, A. and Masi, G. and Matter, D. and Michałowski, J. and Michałowski, M. J. and Michałowski, T. and Michelet, J. and Michelsen, R. and Morelle, E. and Mottola, S. and Naves, R. and Nomen, J. and Oey, J. and Ogłoza, W. and Oksanen, A. and Oszkiewicz, D. and Pääkkönen, P. and Paiella, M. and Pallares, H. and Paulo, J. and Pavic, M. and Payet, B. and Polińska, M. and Polishook, D. and Poncy, R. and Revaz, Y. and Rinner, C. and Rocca, M. and Roche, A. and Romeuf, D. and Roy, R. and Saguin, H. and Salom, P. A. and Sanchez, S. and Santacana, G. and Santana-Ros, T. and Sareyan, J.-P. and Sobkowiak, K. and Sposetti, S. and Starkey, D. and Stoss, R. and Strajnic, J. and Teng, J.-P. and Trégon, B. and Vagnozzi, A. and Velichko, F. P. and Waelchli, N. and Wagrez, K. and Wücher, H.
(2013)
Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution.
Astronomy & Astrophysics, 551, A67.
EDP Sciences.
doi: 10.1051/0004-6361/201220701.
ISSN 0004-6361.
Full text not available from this repository. Official URL: http://dx.doi.org/10.1051/0004-6361/201220701 AbstractContext. The larger number of models of asteroid shapes and their rotational states derived by the lightcurve inversion give us better insight into
both the nature of individual objects and the whole asteroid population. With a larger statistical sample we can study the physical properties of
asteroid populations, such as main-belt asteroids or individual asteroid families, in more detail. Shape models can also be used in combination
with other types of observational data (IR, adaptive optics images, stellar occultations), e.g., to determine sizes and thermal properties.
Aims. We use all available photometric data of asteroids to derive their physical models by the lightcurve inversion method and compare the
observed pole latitude distributions of all asteroids with known convex shape models with the simulated pole latitude distributions.
Methods. We used classical dense photometric lightcurves from several sources (Uppsala Asteroid Photometric Catalogue, Palomar Transient
Factory survey, and from individual observers) and sparse-in-time photometry from the U.S. Naval Observatory in Flagstaff, Catalina Sky Survey,
and La Palma surveys (IAU codes 689, 703, 950) in the lightcurve inversion method to determine asteroid convex models and their rotational
states. We also extended a simple dynamical model for the spin evolution of asteroids used in our previous paper.
Results. We present 119 new asteroid models derived from combined dense and sparse-in-time photometry. We discuss the reliability of asteroid
shape models derived only from Catalina Sky Survey data (IAU code 703) and present 20 such models. By using different values for a scaling
parameter cYORP (corresponds to the magnitude of the YORPmomentum) in the dynamical model for the spin evolution and by comparing synthetic
and observed pole-latitude distributions, we were able to constrain the typical values of the cYORP parameter as between 0.05 and 0.6. Item URL in elib: | https://elib.dlr.de/82219/ |
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Document Type: | Article |
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Title: | Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution |
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Authors: | Authors | Institution or Email of Authors | Author's ORCID iD | ORCID Put Code |
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Hanuš, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Durech, J. | Astronomical Institute, Charles University in Prague, Faculty of Mathematics and Physics, V Holesovickach 2, 18000 Prague, Czech Republic | UNSPECIFIED | UNSPECIFIED | Brož, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Marciniak, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Warner, B. D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Pilcher, F. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Stephens, R. | Santana Observatory, USA | UNSPECIFIED | UNSPECIFIED | Behrend, R. | Observatoire de Geneve, Switzerland | UNSPECIFIED | UNSPECIFIED | Carry, B. | Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, 5 Place Jules Janssen, Meudon F-92195, France | UNSPECIFIED | UNSPECIFIED | Čapek, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Antonini, P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Audejean, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Augustesen, K. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Barbotin, E. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Baudouin, P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Bayol, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Bernasconi, L. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Borczyk, W. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Bosch, J.-G. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Brochard, E. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Brunetto, L. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Casulli, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Cazenave, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Charbonnel, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Christophe, B. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Colas, F. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Coloma, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Conjat, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Cooney, W. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Correira, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Cotrez, V. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Coupier, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Crippa, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Cristofanelli, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Dalmas, Ch. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Danavaro, C. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Demeautis, C. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Droege, T. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Durkee, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Esseiva, N. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Esteban, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Fagas, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Farroni, G. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Fauvaud, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Fauvaud, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Del Freo, F. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Garcia, L. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Geier, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Godon, C. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Grangeon, K. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Hamanowa, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Hamanowa, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Heck, N. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Hellmich, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Higgins, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Hirsch, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Husarik, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Itkonen, T. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Jade, O. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Kamiński, K. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Kankiewicz, P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Klotz, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Koff, R. A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Kryszczyńska, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Kwiatkowski, T. | Astronomical Obervatory, Adam Mickiewicz University, Poznán, Poland | UNSPECIFIED | UNSPECIFIED | Laffont, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Leroy, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Lecacheux, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Leonie, Y. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Leyrat, C. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Manzini, F. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Martin, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Masi, G. | Physics Dept., University of Rome ``Tor Vergata'', Italy | UNSPECIFIED | UNSPECIFIED | Matter, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Michałowski, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Michałowski, M. J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Michałowski, T. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Michelet, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Michelsen, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Morelle, E. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Mottola, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Naves, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Nomen, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Oey, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Ogłoza, W. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Oksanen, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Oszkiewicz, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Pääkkönen, P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Paiella, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Pallares, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Paulo, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Pavic, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Payet, B. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Polińska, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Polishook, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Poncy, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Revaz, Y. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Rinner, C. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Rocca, M. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Roche, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Romeuf, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Roy, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Saguin, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Salom, P. A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Sanchez, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Santacana, G. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Santana-Ros, T. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Sareyan, J.-P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Sobkowiak, K. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Sposetti, S. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Starkey, D. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Stoss, R. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Strajnic, J. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Teng, J.-P. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Trégon, B. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Vagnozzi, A. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Velichko, F. P. | Astronomical Observatory, Kharkov State University, Kharkov, Ukraine | UNSPECIFIED | UNSPECIFIED | Waelchli, N. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Wagrez, K. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED | Wücher, H. | UNSPECIFIED | UNSPECIFIED | UNSPECIFIED |
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Date: | 2013 |
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Journal or Publication Title: | Astronomy & Astrophysics |
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Refereed publication: | Yes |
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Open Access: | No |
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Gold Open Access: | No |
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In SCOPUS: | Yes |
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In ISI Web of Science: | Yes |
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Volume: | 551 |
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DOI: | 10.1051/0004-6361/201220701 |
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Page Range: | A67 |
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Publisher: | EDP Sciences |
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ISSN: | 0004-6361 |
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Status: | Published |
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Keywords: | minor planets, asteroids: general |
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HGF - Research field: | Aeronautics, Space and Transport |
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HGF - Program: | Space |
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HGF - Program Themes: | Space Exploration |
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DLR - Research area: | Raumfahrt |
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DLR - Program: | R EW - Space Exploration |
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DLR - Research theme (Project): | R - Vorhaben Asteroiden und Kometen (old) |
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Location: |
Berlin-Adlershof
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Institutes and Institutions: | Institute of Planetary Research > Asteroids and Comets |
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Deposited By: |
Mottola, Dr.phys. Stefano
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Deposited On: | 06 May 2013 12:56 |
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Last Modified: | 23 Aug 2016 09:49 |
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