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The Synodic Rotation Period of Comet 17P/Holmes

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dc.contributor.author Betzler, Alberto Silva
dc.contributor.author Ferreira, Diego Henrique
dc.contributor.author Ribeiro dos Santos, Tárcio Henrique
dc.contributor.author Novaes, Alberto Brum
dc.contributor.author Celedon, Julian Hermógenes Quezada
dc.creator Betzler, Alberto Silva
dc.creator Ferreira, Diego Henrique
dc.creator Ribeiro dos Santos, Tárcio Henrique
dc.creator Novaes, Alberto Brum
dc.creator Celedon, Julian Hermógenes Quezada
dc.date.accessioned 2018-02-28T21:24:01Z
dc.date.available 2018-02-28T21:24:01Z
dc.date.issued 2008
dc.identifier.citation BETZLER, Alberto Silva et al. The synodic rotation period of Comet 17P/Holmes. Journal of the Association of Lunar & Planetary Observers, The Strolling Astronomer. Springfield, v. 50, n. 3, p. 23-26, jun., 2008. pt_BR
dc.identifier.issn 0039-2502
dc.identifier.uri http://repositorio.ufba.br/ri/handle/ri/25389
dc.description.abstract Comet 17P/Holmes was observed in October and November 2007, after the brightness outburst of 24 October. Approximately 11.5 hours of data were collected. A time series analysis reveals a periodicity of 6.29±0.01 hour in the brightness of the inner coma with a single-peak light curve. The object probably has an extremely active area in the nucleus. Therefore, the synodic rotation period is probably equal to the 6.29-hour periodicity that we found. pt_BR
dc.description.sponsorship Fundação Vitae, FAPESB pt_BR
dc.language.iso en pt_BR
dc.publisher Association of Lunar & Planetary Observers pt_BR
dc.rights Acesso Aberto pt_BR
dc.subject Photometry pt_BR
dc.subject Comets pt_BR
dc.subject Rotation Rates pt_BR
dc.subject Comet 17P/Holmes pt_BR
dc.title The Synodic Rotation Period of Comet 17P/Holmes pt_BR
dc.type Artigo de Periódico pt_BR
dc.description.localpub Springfield, Illinois pt_BR
dc.identifier.number v.50, n.3 pt_BR
dc.publisher.country Brasil pt_BR


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