Lightcurve Analysis of 932 Hooveria
Abstract
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.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2010
- Bibcode:
- 2010MPBu...37..139W