The HARPS search for Earth-like planets in the habitable zone I. Very low-mass planets around HD 20794, HD 85512, and HD 192310

• Tipo: Artigo em Revista Científica Internacional
• Data: 2011

Autores

Pepe, F (Autor) Outra; Lovis, C (Autor) Outra; Segransan, D (Autor) Outra; Benz, W (Autor) Outra; Bouchy, F (Autor) Outra; Dumusque, X (Autor) Outra; Mayor, M (Autor) Outra; Queloz, D (Autor) Outra; N.C. Santos (Autor) FCUP; Udry, S (Autor) Outra

Revista

Título: Astronomy and Astrophysics

Vol. 534

Página Final: A58

ISSN: 0004-6361

Editora: EDP Sciences

Indexação

ISI Web of Knowledge - 217 Citações

Scopus - 227 Citações

Outras Informações

ID Authenticus: P-002-KV3

DOI: 10.1051/0004-6361/201117055

Abstract (EN): Context. In 2009 we started an intense radial-velocity monitoring of a few nearby, slowly-rotating and quiet solar-type stars within the dedicated HARPS-Upgrade GTO program. Aims. The goal of this campaign is to gather very-precise radial-velocity data with high cadence and continuity to detect tiny signatures of very-low-mass stars that are potentially present in the habitable zone of their parent stars. Methods. Ten stars were selected among the most stable stars of the original HARPS high-precision program that are uniformly spread in hour angle, such that three to four of them are observable at any time of the year. For each star we recorded 50 data points spread over the observing season. The data points consist of three nightly observations with a total integration time of 10 min each and are separated by two hours. This is an observational strategy adopted to minimize stellar pulsation and granulation noise. Results. We present the first results of this ambitious program. The radial-velocity data and the orbital parameters of five new and one confirmed low-mass planets around the stars HD 20794, HD 85512, and HD 192310 are reported and discussed, among which is a system of three super-Earths and one that harbors a 3.6 M(circle plus)-planet at the inner edge of the habitable zone. Conclusions. This result already confirms previous indications that low-mass planets seem to be very frequent around solar-type stars and that this may occur with a frequency higher than 30%.

Idioma: Inglês

Tipo (Avaliação Docente): Científica

Nº de páginas: 16