Lightcurve Analysis of (8639) 1991 GR

Details Lightcurve Analysis of (8639) 1991 GR Lightcurve Analysis of (8639) 1991 GR

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38..209w&link_type=abstract

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

Computer Science

Scientific paper

CCD photometry observations of the Eunomia member asteroid (8369) 1991 GR were made at the Palmer Divide Observatory and Center for Solar System Studies in 2011 March. Analysis using a single period search found a synodic period of 2.7368 ± 0.0001 h and lightcurve amplitude of 0.24 ± 0.02 mag. A dual-period search found a weak secondary period (assuming a bimodal lightcurve) of 49.24 ± 0.16 h. Subtracting this period noticeably improved the RMS fit of the short-period component.

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