Lightcurve Photometry and H-G Parameters for 1342 Brabantia

Details Lightcurve Photometry and H-G Parameters for 1342 Brabantia Lightcurve Photometry and H-G Parameters for 1342 Brabantia

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mpbu...38..132f&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

The main-belt asteroid 1342 Brabantia was observed over seven nights in 2010 December and 2011 January- February with filtered and non-filtered systems. The resulting synodic period is P = 4.1754 ± 0.0001 h with an amplitude AV = 0.19 ± 0.01 mag. The color index V-R = 0.41 ± 0.02 mag. The measured absolute visual magnitude, HV = 11.30 ± 0.05 mag, and the slope parameter, G = 0.23 ± 0.06, are consistent with a medium albedo object, e.g., type M or S. The diameter is estimated to be D = 18 ± 2 km.

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