CCD photometry of asteroid 12753 Povenmire

Details CCD photometry of asteroid 12753 Povenmire CCD photometry of asteroid 12753 Povenmire

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mpbu...31...56g&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

Minor Planets, Periods, Ccd Photometry

Scientific paper

Main-belt asteroid 12753 Povenmire was observed to have a lightcurve period of 12.85 hours and a brightness variation of 0.50 magnitude during its 2003 opposition. The lightcurve was symmetrical throughout the 3-month observing period, consistent with a simple shape. BVRI photometry measurements yield the following color indices: V-R = 1.34±0.18 (redder than the sun) and R-I = 0.33±0.10 (solar-like), implying a typically red, then flattening spectral curve. The asteroid was 0.3 magnitudes fainter than perdicted, suggesting H = 12.8 as a revised absolute magnitude.

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