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

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@article{4a504c7a1aec4c5a95fe21ab05eacdff,
title = "CCD photometry of asteroid 932 Hooveria",
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.",
author = "Sada, {Pedro V.}",
year = "2004",
month = "3",
day = "1",
language = "English",
volume = "31",
pages = "22--23",
journal = "The Minor Planet Bulletin",
issn = "1052-8091",

}

CCD photometry of asteroid 932 Hooveria. / Sada, Pedro V.

In: The Minor Planet Bulletin, Vol. 31, 01.03.2004, p. 22-23.

Research output: Contribution to journalArticle

TY - JOUR

T1 - CCD photometry of asteroid 932 Hooveria

AU - Sada, Pedro V.

PY - 2004/3/1

Y1 - 2004/3/1

N2 - 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.

AB - 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.

M3 - Article

VL - 31

SP - 22

EP - 23

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -