Photometric Observations and Analysis of 1082 Pirola

Details Photometric Observations and Analysis of 1082 Pirola Photometric Observations and Analysis of 1082 Pirola

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38..111b&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 observations of the main-belt asteroid 1082 Pirola were recorded during the period 2010 October to 2011 January. Analysis of the lightcurve found a synodic period of P = 15.8525 ± 0.0005 h and amplitude A = 0.53 ± 0.01 mag. The phase curve referenced to mean magnitude suggests the absolute magnitude and phase slope parameter: H = 10.507 ± 0.014 mag; G = 0.080 ± 0.016. The phase curve referenced to maximum light suggests: H = 10.320 ± 0.013 mag; G = 0.107 ± 0.016.

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