Lightcurve Analysis of Minor Planets 2544 Gubarev and 2599 Veseli

Details Lightcurve Analysis of Minor Planets 2544 Gubarev and 2599 Veseli Lightcurve Analysis of Minor Planets 2544 Gubarev and 2599 Veseli

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007mpbu...34...43b&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

Scientific paper

Minor planet 2599 Veseli was observed over four nights in July 2004, and minor planet 2544 Gubarev was observed over eight nights in April 2005. The synodic rotation period for 2544 Gubarev was found to be 4.750 ± 0.001 hr with an amplitude of 0.42 mag. For 2599 Veseli, the results were less secure and found to fit two possible synodic periods, 13.25 ± 0.05 hr and 18.54 ± 0.05 hr, with an amplitude of 0.33 mag.

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