Photometry and models of selected main belt asteroids

Free access article

Issue		A&A Volume 443, Number 1, November III 2005


Page(s)		329 - 335
Section		Planets and planetary systems
DOI		http://dx.doi.org/10.1051/0004-6361:20053656

A&A 443, 329-335 (2005)
DOI: 10.1051/0004-6361:20053656

II. 173 Ino, 376 Geometria, and 451 Patientia

T. Michalowski¹, M. Kaasalainen², A. Marciniak¹, P. Denchev³, T. Kwiatkowski¹, A. Kryszczynska¹, R. Hirsch¹, F. P. Velichko⁴, A. Erikson⁵, Gy. M. Szabó⁶ and R. Kowalski⁷

¹ Astronomical Observatory, Adam Mickiewicz University, Sloneczna 36, 60-286 Poznan, Poland
² Rolf Nevanlinna Institute, University of Helsinki PO Box 4, 00014 Helsinki, Finland
³ Institute of Astronomy, Rozhen National Observatory, PO Box 136, 4700 Smolyan, Bulgaria
⁴ Research Institute of Astronomy, Kharkiv Karazin National University, Sums'ka 35, 61022 Kharkiv, Ukraine
⁵ Institute of Space Sensor Technology and Planetary Exploration, Rutherford str. 2, 12489 Berlin, Germany
⁶ Department of Experimental Physics & Astronomical Observatory, University of Szeged, 6720 Szeged, Dóm tér 9, Hungary
⁷ Quail Hollow Observatory, 7630 Conrad St., Zephyrhills, FL, USA

(Received 18 June 2005 / Accepted 19 July 2005)

Abstract
Photometric observations for 173 Ino (1998, 1999, 2002), 376 Geometria (1996, 1997/98, 1999, 2000, 2004) and 451 Patientia (1998, 2002, 2003) carried out at six observatories are presented. Using all available lightcurves, the spin vectors, senses of rotation and shape models of these three asteroids were determined.

Key words: techniques: photometric -- minor planets, asteroids

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