CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

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Abstract

CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.
Original languageEnglish
Pages (from-to)161-162
JournalThe Minor Planet Bulletin
Volume35
Publication statusPublished - 1 Oct 2008

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@article{f0b81a1fc03e4146b0271c6c1e22b194,
title = "CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory",
abstract = "CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.",
author = "Sada, {Pedro V.}",
year = "2008",
month = "10",
day = "1",
language = "English",
volume = "35",
pages = "161--162",
journal = "The Minor Planet Bulletin",
issn = "1052-8091",

}

CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory. / Sada, Pedro V.

In: The Minor Planet Bulletin, Vol. 35, 01.10.2008, p. 161-162.

Research output: Contribution to journalArticle

TY - JOUR

T1 - CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

AU - Sada, Pedro V.

PY - 2008/10/1

Y1 - 2008/10/1

N2 - CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.

AB - CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.

M3 - Article

VL - 35

SP - 161

EP - 162

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -