Issue |
A&A
Volume 508, Number 3, December IV 2009
|
|
---|---|---|
Page(s) | 1503 - 1507 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/200912741 | |
Published online | 08 October 2009 |
Photometry and models of selected main belt asteroids*,**
VII. 350 Ornamenta, 771 Libera, and 984 Gretia
1
Astronomical Observatory, Adam Mickiewicz University, Słoneczna 36, 60-286 Poznań, Poland e-mail: aniab@lab.astro.amu.edu.pl
2
Geneva Observatory, 1290 Sauverny, Switzerland
3
Les Engarouines Observatory, 84570 Mallemort-du-Comtat, France
4
IMCCE – Paris Observatory – UMR 8028 CNRS, 77 av. Denfert-Rochereau, 75014 Paris, France
5
Observatoire du Bois de Bardon, 16110 Taponnat, France
6
Association T60, 14 avenue Edouard Belin, 31400 Toulouse, France
7
Université de Rennes 1, Campus de Beaulieu, 35042 Rennes Cedex, France
8
Makes Observatory, 18 rue G. Bizet – Les Makes, 97421 La Rivière, France
Received:
22
June
2009
Accepted:
14
September
2009
We analyze photometric observations of the three main-belt asteroids 350 Ornamenta, 771 Libera, and 984 Gretia, conducted over a twelve-year interval. Our data and those of other authors allow us to determine pole and shape models using the lightcurve inversion technique. In all three cases, a single pole solution was obtained without any significant mirror solution:
Ornamenta – h,
,
Libera –
h,
,
Gretia –
h,
,
.
This analysis and the development of asteroid models increase the set of asteroids with known spin and shape parameters, which consists of only around 100 objects.
Key words: techniques: photometric / minor planets, asteroids
© ESO, 2009
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