Lightcurve for Hungaria asteroid 1600 Vyssotsky over several apparitions

Details Lightcurve for Hungaria asteroid 1600 Vyssotsky over several apparitions Lightcurve for Hungaria asteroid 1600 Vyssotsky over several apparitions

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mpbu...33...45w&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

1

Minor Planets, Light Curves, Periods

Scientific paper

Photometric observations of the Hungaria asteroid 1600 Vyssotsky were previously reported by Warner (1999). Those data were reanalyzed to confirm and, if possible, refine the original results. In addition, analysis was performed on previously unpublished data obtained during the 2004 and 2005 apparitions. The average synodic period for the three apparitions was found to be 3.2011±0.0004h, with the periods for each apparition within 1-sigma of the average. The amplitude of the lightcurve varied from 0.16-0.18m but most notable was the change in the shape of the curve.

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