Lightcurve Analysis of 932 Hooveria

Details Lightcurve Analysis of 932 Hooveria Lightcurve Analysis of 932 Hooveria

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mpbu...37..139w&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 932 Hooveria in 2010 February
and March led to a lightcurve with a synodic period of P = 39.15
± 0.05 h. This contradicted a period of 30 h (Sada, 2004).
Re-analysis of the Sada data set gives P = 39.23 ± 0.02 h,
putting the two periods in fairly close agreement.

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