Lightcurve Photometry Results from Bigmuskie Observatory: Late 2010

Details Lightcurve Photometry Results from Bigmuskie Observatory: Late 2010 Lightcurve Photometry Results from Bigmuskie Observatory: Late 2010

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38...92f&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 photometric observations were made of four asteroids in 2010 September-December at the Bigmuskie Observatory, Italy, to determine rotation periods and lightcurve amplitudes. The results were: 1448 Lindbladia, P = 10.969 ± 0.002 h, A = 0.22 ± 0.02 mag; 5288 Nankichi, P = 12.763 ± 0.003 h, A = 0.19 ± 0.02 mag; 10217 Richardcook, P = 23.33 ± 0.01 h, A = 0.45 ± 0.02 mag; (14657) 1998 YU27, P= 33.58 ± 0.02 h, A=0.30 ± 0.02 mag.

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