Title
CCD photometry, spin and shape model of the asteroid 1572 Posnania
Date Issued
01 January 2001
Access level
open access
Resource Type
journal article
Author(s)
Michałowski T.
Pych W.
Kwiatkowski T.
Kryszczyńska A.
Pravec P.
Borczyk W.
Erikson A.
Wisniewski W.
Berthier J.
Institut de Mecanique Celeste
Publisher(s)
EDP Sciences
Abstract
Lightcurves of the asteroid 1572 Posnania were obtained at six observatories on 19 nights during four apparitions: in 1993, 1994-95, 1996, and 1999. The synodical period is found to be 8.048 hours and the observed amplitudes of brightness variations are in the range of 0.37-0.40 mag. The sense of rotation is retrograde with a sidereal period Psid = 0.3353931 ± 0.0000003 days. The ecliptic coordinates of the pole of this asteroid are λp = 46° ± 6° and βp = -65° ± 5°. The shape of Posnania can be approximated by a triaxial ellipsoid model with semiaxes ratios a/b = 1.35 ± 0.01 and b/c = 1.04 ± 0.03.
Start page
748
End page
752
Volume
371
Issue
2
Language
English
OCDE Knowledge area
Astronomía
Scopus EID
2-s2.0-0035325497
Source
Astronomy and Astrophysics
ISSN of the container
00046361
Sources of information: Directorio de Producción Científica Scopus