Lightcurve Analysis of 669 Kypria

Craig S. Bennefeld, Pedro V. Sada

Research output: Contribution to journalArticle

Abstract

Photometric observations of 669 Kypria were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 14.283 ± 0.001 h and amplitude of ~0.60 mag.
Original languageEnglish
Pages (from-to)87-88
JournalThe Minor Planet Bulletin
Volume35
Publication statusPublished - 1 Jun 2008

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Bennefeld, Craig S. ; Sada, Pedro V. / Lightcurve Analysis of 669 Kypria. In: The Minor Planet Bulletin. 2008 ; Vol. 35. pp. 87-88.
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abstract = "Photometric observations of 669 Kypria were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 14.283 ± 0.001 h and amplitude of ~0.60 mag.",
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Lightcurve Analysis of 669 Kypria. / Bennefeld, Craig S.; Sada, Pedro V.

In: The Minor Planet Bulletin, Vol. 35, 01.06.2008, p. 87-88.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Lightcurve Analysis of 669 Kypria

AU - Bennefeld, Craig S.

AU - Sada, Pedro V.

PY - 2008/6/1

Y1 - 2008/6/1

N2 - Photometric observations of 669 Kypria were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 14.283 ± 0.001 h and amplitude of ~0.60 mag.

AB - Photometric observations of 669 Kypria were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 14.283 ± 0.001 h and amplitude of ~0.60 mag.

M3 - Article

VL - 35

SP - 87

EP - 88

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -