CCD photometry of asteroid 932 Hooveria

Pedro V. Sada

CCD photometry of asteroid 932 Hooveria

Pedro V. Sada

Departamento de Física y Matemáticas

Research output: Contribution to journal › Article › peer-review

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 language	English
Pages (from-to)	22-23
Journal	The Minor Planet Bulletin
Volume	31
Publication status	Published - 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 = mar,

day = "1",

language = "English",

volume = "31",

pages = "22--23",

journal = "The Minor Planet Bulletin",

issn = "1052-8091",

}

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

SN - 1052-8091

VL - 31

SP - 22

EP - 23

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

ER -

CCD photometry of asteroid 932 Hooveria

Abstract

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