CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory

Pedro V. Sada

Research output: Contribution to journal › Article

Abstract

CCD photometry of six asteroids was obtained at the Universidad de Monterrey Observatory during January and February 2008. The resulting synodic rotation periods and amplitudes are as follows: 1292 Luce, 6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878 ± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999 ± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842 ± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ± 0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001 h, 0.20 ± 0.01 mag.
Original languageEnglish
Pages (from-to)105-107
JournalThe Minor Planet Bulletin
Volume35
Publication statusPublished - 1 Sep 2008

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Sada, Pedro V. / CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory. In: The Minor Planet Bulletin. 2008 ; Vol. 35. pp. 105-107.
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abstract = "CCD photometry of six asteroids was obtained at the Universidad de Monterrey Observatory during January and February 2008. The resulting synodic rotation periods and amplitudes are as follows: 1292 Luce, 6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878 ± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999 ± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842 ± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ± 0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001 h, 0.20 ± 0.01 mag.",
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Sada, PV 2008, 'CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory', The Minor Planet Bulletin, vol. 35, pp. 105-107.

CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory. / Sada, Pedro V.

In: The Minor Planet Bulletin, Vol. 35, 01.09.2008, p. 105-107.

Research output: Contribution to journal › Article

TY - JOUR

T1 - CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory

AU - Sada, Pedro V.

PY - 2008/9/1

Y1 - 2008/9/1

N2 - CCD photometry of six asteroids was obtained at the Universidad de Monterrey Observatory during January and February 2008. The resulting synodic rotation periods and amplitudes are as follows: 1292 Luce, 6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878 ± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999 ± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842 ± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ± 0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001 h, 0.20 ± 0.01 mag.

AB - CCD photometry of six asteroids was obtained at the Universidad de Monterrey Observatory during January and February 2008. The resulting synodic rotation periods and amplitudes are as follows: 1292 Luce, 6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878 ± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999 ± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842 ± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ± 0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001 h, 0.20 ± 0.01 mag.

M3 - Article

VL - 35

SP - 105

EP - 107

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -

Sada PV. CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory. The Minor Planet Bulletin. 2008 Sep 1;35:105-107.

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