Lightcurve Analysis of 932 Hooveria

Brian D. Warner; Pedro V. Sada; J. Pollock; Daniel Reichart; Ivan Ivarsen; Josh Haislip; Aaron Lacluyze; Melissa Nysewander

Lightcurve Analysis of 932 Hooveria

Brian D. Warner, Pedro V. Sada, J. Pollock, Daniel Reichart, Ivan Ivarsen, Josh Haislip, Aaron Lacluyze, Melissa Nysewander

Departamento de Física y Matemáticas

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

Abstract

CCD observations of the main-belt asteroid 932 Hooveria in 2010 February and March led to a lightcurve with a synodic period of P = 39.15 ± 0.05 h. This contradicted a period of 30 h (Sada, 2004). Re-analysis of the Sada data set gives P = 39.23 ± 0.02 h, putting the two periods in fairly close agreement.

Original language	English
Pages (from-to)	139
Journal	The Minor Planet Bulletin
Volume	37
Publication status	Published - 1 Oct 2010

Access to Document

http://adsabs.harvard.edu/abs/2010MPBu...37..139W

Cite this

@article{2b06a67316254b0991260feb504b93e8,

title = "Lightcurve Analysis of 932 Hooveria",

abstract = "CCD observations of the main-belt asteroid 932 Hooveria in 2010 February and March led to a lightcurve with a synodic period of P = 39.15 ± 0.05 h. This contradicted a period of 30 h (Sada, 2004). Re-analysis of the Sada data set gives P = 39.23 ± 0.02 h, putting the two periods in fairly close agreement.",

author = "Warner, \{Brian D.\} and Sada, \{Pedro V.\} and J. Pollock and Daniel Reichart and Ivan Ivarsen and Josh Haislip and Aaron Lacluyze and Melissa Nysewander",

year = "2010",

month = oct,

day = "1",

language = "English",

volume = "37",

pages = "139",

journal = "The Minor Planet Bulletin",

issn = "1052-8091",

}

TY - JOUR

T1 - Lightcurve Analysis of 932 Hooveria

AU - Warner, Brian D.

AU - Sada, Pedro V.

AU - Pollock, J.

AU - Reichart, Daniel

AU - Ivarsen, Ivan

AU - Haislip, Josh

AU - Lacluyze, Aaron

AU - Nysewander, Melissa

PY - 2010/10/1

Y1 - 2010/10/1

N2 - CCD observations of the main-belt asteroid 932 Hooveria in 2010 February and March led to a lightcurve with a synodic period of P = 39.15 ± 0.05 h. This contradicted a period of 30 h (Sada, 2004). Re-analysis of the Sada data set gives P = 39.23 ± 0.02 h, putting the two periods in fairly close agreement.

AB - CCD observations of the main-belt asteroid 932 Hooveria in 2010 February and March led to a lightcurve with a synodic period of P = 39.15 ± 0.05 h. This contradicted a period of 30 h (Sada, 2004). Re-analysis of the Sada data set gives P = 39.23 ± 0.02 h, putting the two periods in fairly close agreement.

M3 - Article

SN - 1052-8091

VL - 37

SP - 139

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

ER -

Lightcurve Analysis of 932 Hooveria

Abstract

Access to Document

Fingerprint

Cite this