POLE ORIENTATION AND SHAPE OF 12 ASTEROIDS

Citation
E. Dotto et al., POLE ORIENTATION AND SHAPE OF 12 ASTEROIDS, Icarus, 117(2), 1995, pp. 313-327
Citations number
73
Categorie Soggetti
Astronomy & Astrophysics
Journal title
IcarusACNP
ISSN journal
00191035
Volume
117
Issue
2
Year of publication
1995
Pages
313 - 327
Database
ISI
SICI code
0019-1035(1995)117:2<313:POASO1>2.0.ZU;2-B
Abstract
We present the results of photometric observations of 12 asteroids, pe rformed from 1985 through 1989 at the Astronomical Observatory of Tera mo (Italy), Astronomical Observatory of Turin (Italy), and European So uthern Observatory (ESO, La Silla, Chile). Using the EA pole determina tion method described in G. De Angelis (Planet. Space Sci., 41, 285-29 0, 1993), we have obtained the first spin and shape solution of 85 Io and 360 Carlova and an improvement of the previous determinations for 12 Victoria, 192 Nausikaa and 423 Diotima, for which we determined for the first time the sidereal period and the sense of rotation. We have checked the determinations obtained by other authors for the asteroid s 3 June, 6 Hebe, 20 Massalia, 43 Ariadne, and 52 Europa, and suggeste d a very rough estimate of the spin and shape parameters of 115 Thyra. (C) 1995 Academic Press, Inc.