Lightcurve Analysis of 932 Hooveria
- Brian D. Warner,
- ,
- J. Pollock,
- Daniel Reichart,
- Ivan Ivarsen,
- Josh Haislip
Research Output:
Contribution to journal
Article
Peer-reviewAbstract
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 Information
Output type
Research Output:
Contribution to journal
Article
Peer-reviewOriginal language
EnglishPages from-to (Number of pages)
Pages 139Journal (Volume, Issue Number)
The Minor Planet Bulletin (Volume 37)Publication milestones
- Published - 01/10/2010
Publication status
Published - 01/10/2010