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2012 Qg42: a Slow Rotator Nea.

Year: 2013

Type: article

Abstract: CCD photometric observations of the near-Earth asteroid 2012 QG42 were made by a collaboration of observers in the U.S. and Europe. The asteroid was found to be a slow rotator, having a synodic period of 24.22 ± 0.01 h based on a data set spanning nearly two weeks. The amplitude of the lightcurve was 1.18 ± 0.03 mag.

Source: PubMed

Authors: Brian D Warner, Ronald E Baker, Przemyslaw Bartczak, Anna Marciniak, Krzysztof Sobkowiak, Roman Hirsch, Krzysztof Kaminski, Paolo Bacci, Lorenzo Franco, Tomas Vorobjov, Robert E Holmes

Institution: The Chagrin Valley Astronomical Society

Language: English

Topic: Astro and Planetary Science

Subfield: Space and Planetary Science

Field: Earth and Planetary Sciences

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W2994885762

FWCI: 0.294

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Cited by: 1

Related to: 10