Lightcurve Analysis of 669 Kypria

Craig S. Bennefeld; Pedro V. Sada

Lightcurve Analysis of 669 Kypria

Craig S. Bennefeld, Pedro V. Sada

Departamento de Física y Matemáticas

Producción científica › revisión exhaustiva

Resumen

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.

Idioma original	English
Páginas (desde-hasta)	87-88
Publicación	The Minor Planet Bulletin
Volumen	35
Estado	Published - 1 jun 2008

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@article{7648d2a1e85d45dbb45cafe27702a2c9,

title = "Lightcurve Analysis of 669 Kypria",

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.",

author = "Bennefeld, {Craig S.} and Sada, {Pedro V.}",

year = "2008",

month = jun,

day = "1",

language = "English",

volume = "35",

pages = "87--88",

journal = "The Minor Planet Bulletin",

issn = "1052-8091",

}

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

SN - 1052-8091

VL - 35

SP - 87

EP - 88

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

ER -

Lightcurve Analysis of 669 Kypria

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