CCD photometry of asteroid 932 Hooveria

Research output: Contribution to journalArticle

Abstract

CCD photometry of asteroid 932 Hooveria taken during October 2001 and January 2002 at the Universidad de Monterrey Observatory is reported. A synodic rotation period of either 29.947 or 30.370 hours is determined from eight nights of observations.
Original languageEnglish
Pages (from-to)22-23
JournalThe Minor Planet Bulletin
Volume31
Publication statusPublished - 1 Mar 2004

Fingerprint Dive into the research topics of 'CCD photometry of asteroid 932 Hooveria'. Together they form a unique fingerprint.

  • Cite this