Lightcurve Analysis of 932 Hooveria

Brian D. Warner, Pedro V. Sada, J. Pollock, Daniel Reichart, Ivan Ivarsen, Josh Haislip, Aaron Lacluyze, Melissa Nysewander

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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.
Original languageEnglish
Pages (from-to)139
JournalThe Minor Planet Bulletin
Volume37
Publication statusPublished - 1 Oct 2010

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Warner, B. D., Sada, P. V., Pollock, J., Reichart, D., Ivarsen, I., Haislip, J., Lacluyze, A., & Nysewander, M. (2010). Lightcurve Analysis of 932 Hooveria. The Minor Planet Bulletin, 37, 139.