Lightcurve Analysis of 6901 Roybishop

Details Lightcurve Analysis of 6901 Roybishop Lightcurve Analysis of 6901 Roybishop

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012mpbu...39...83w&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

CCD photometry observations of the Hungaria asteroid 6901 Roybishop were made at the Palmer Divide Observatory and the Center for Solar System Studies in 2011 November. Data from a previous apparition gave indications of the asteroid having a satellite. The observations in 2011 did not provide any reasonable evidence that the asteroid was binary. Analysis of the data obtained over 4 nights found a synodic period of 4.785 ± 0.004 h and amplitude of only 0.04 ± 0.01 mag.

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