Physical models of ten asteroids from an observers' collaboration network
- Durech, Josef
- Kaasalainen, Mikko
- Marciniak, A.
- Allen, W. H.
- Behrend, Raoul
- Bembrick, C.
- Bennett, T.
- Bernasconi, L.
- Berthier, Jerôme
- Bolt, G.
- Boroumand, S.
- Crespo da Silva, L.
- Crippa, R.
- Crow, M.
- Durkee, R.
- Dymock, R.
- Fagas, M.
- Fauerbach, M.
- Fauvaud, S.
- Frey, M.
- Goncalves, R.
- Hirsch, R.
- Jardine, D.
- Kaminski, K.
- Koff, R.
- Kwiatkowski, T.
- Lopez-Ariste, Arturo
- Manzini, F.
- Michalowski, T.
- Pacheco, R.
- Pan, Ming
- Pilcher, F.
- Poncy, R.
- Pray, D. P.
- Pych, W.
- Roy, R.
- Santacana, G.
- Slivan, S.
- Sposetti, Stefano
- Stephens, R.
- Warner, B.
- Wolf, M.
DOIAbstract
International audienceAims:We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys. Methods: The lightcurve inversion method was used to derive spin states and shape models of the asteroids. Results: We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred
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