Volume 331, Issue 9-10 pp. 972-976
Editor's Choice
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Asteroseismology of solar-type stars with Kepler I: Data analysis

C. Karoff

Corresponding Author

C. Karoff

School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UKSearch for more papers by this author
W.J. Chaplin

W.J. Chaplin

School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

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T. Appourchaux

T. Appourchaux

Institut d'Astrophysique Spatiale, Université Paris XI-CNRS (UMR8617), Batiment 121, 91405 Orsay Cedex, France

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Y. Elsworth

Y. Elsworth

School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

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R.A. Garcia

R.A. Garcia

Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/SAp-SEDI, Centre de Saclay, 91191, Gif-sur-Yvette, France

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G. Houdek

G. Houdek

Institute of Astronomy, University of Vienna, A-1180 Vienna, Austria

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T.S. Metcalfe

T.S. Metcalfe

High Altitude Observatory and Scientific Computing Division, National Center for Atmospheric Research, Boulder, CO 80307, USA

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J. Molenda-Żakowicz

J. Molenda-Żakowicz

Astronomical Institute, University of Wroclaw, ul. Kopernika, 11, 51-622 Wroclaw, Poland

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M.J.P.F.G. Monteiro

M.J.P.F.G. Monteiro

Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Ruas das Estrelas, 4150-762 Porto, Portugal

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M.J. Thompson

M.J. Thompson

School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, UK

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J. Christensen-Dalsgaard

J. Christensen-Dalsgaard

Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

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R.L. Gilliland

R.L. Gilliland

Space Telescope Science Institute, Baltimore, MD 21218, USA

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H. Kjeldsen

H. Kjeldsen

Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

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S. Basu

S. Basu

Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA

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T.R. Bedding

T.R. Bedding

Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia

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T.L. Campante

T.L. Campante

Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Ruas das Estrelas, 4150-762 Porto, Portugal

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P. Eggenberger

P. Eggenberger

Geneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, Switzerland

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S.T. Fletcher

S.T. Fletcher

Materials Engineering Research Institute, Faculty of Arts, Computing, Engineering and Sciences, Sheffield Hallam University, Sheffield, S1 1WB, UK

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P. Gaulme

P. Gaulme

Institut d'Astrophysique Spatiale, Université Paris XI-CNRS (UMR8617), Batiment 121, 91405 Orsay Cedex, France

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R. Handberg

R. Handberg

Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

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S. Hekker

S. Hekker

School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

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M. Martic

M. Martic

LATMOS-IPSL, CNRS, Université de Versailles Saint-Quentin, 11, boulevard d'Alembert, 78280 Guyancourt, France

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S. Mathur

S. Mathur

High Altitude Observatory and Scientific Computing Division, National Center for Atmospheric Research, Boulder, CO 80307, USA

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B. Mosser

B. Mosser

LESIA, CNRS, Université Pierre et Marie Curie, Université, Denis Diderot, Observatoire de Paris, 92195 Meudon Cedex, France

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C. Regulo

C. Regulo

Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain

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I.W. Roxburgh

I.W. Roxburgh

Queen Mary University of London, Astronomy Unit, Mile End Road, London E1 4NS, UK

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D. Salabert

D. Salabert

Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain

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D. Stello

D. Stello

Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia

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G.A Verner

G.A Verner

Queen Mary University of London, Astronomy Unit, Mile End Road, London E1 4NS, UK

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K. Belkacem

K. Belkacem

Département d'Astrophysique, Géophysique et Océanographie (AGO), Université de Liége, Allée du 6 Aoüt 17 4000 Liége 1, Belgium

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K. Biazzo

K. Biazzo

Arcetri Astrophysical Observatory, Largo Enrico Fermi 5, 50125 Firenze, Italy

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M.S. Cunha

M.S. Cunha

Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Ruas das Estrelas, 4150-762 Porto, Portugal

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M. Gruberbauer

M. Gruberbauer

Department of Astronomy and Physics, Saint Mary's University, Halifax, NS B3H 3C3, Canada

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J.A. Guzik

J.A. Guzik

Los Alamos National Laboratory, Los Alamos, NM 87545-2345, USA

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F. Kupka

F. Kupka

Faculty of Mathematics, University of Vienna, Nordbergstraße 15, A-1090 Wien, Austria

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B. Leroy

B. Leroy

LESIA, CNRS, Université Pierre et Marie Curie, Université, Denis Diderot, Observatoire de Paris, 92195 Meudon Cedex, France

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H.-G. Ludwig

H.-G. Ludwig

ZAH – Landessternwarte, Königstuhl 12, 69117 Heidelberg, Germany

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S. Mathis

S. Mathis

Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/SAp Centre de Saclay, F-91191 Gif-sur-Yvette, France

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A. Noels

A. Noels

Département d'Astrophysique, Géophysique et Océanographie (AGO), Université de Liége, Allée du 6 Aoüt 17 4000 Liége 1, Belgium

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R.W. Noyes

R.W. Noyes

Smithsonian Astrophysical Observatory, Cambridge, MA, USA

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T. Roca Cortes

T. Roca Cortes

Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain

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M. Roth

M. Roth

Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany

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K.H. Sato

K.H. Sato

Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/SAp-SEDI, Centre de Saclay, 91191, Gif-sur-Yvette, France

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J. Schmitt

J. Schmitt

Observatoire de Haute-Provence, F-04870, St.Michel l'Observatoire, France

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M.D. Suran

M.D. Suran

Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint, 5, RO 40557, Bucharest, Romania

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R. Trampedach

R. Trampedach

JILA, University of Colorado, 440 UCB, Boulder, CO 80309-0440, USA

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K. Uytterhoeven

K. Uytterhoeven

Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/SAp-SEDI, Centre de Saclay, 91191, Gif-sur-Yvette, France

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R. Ventura

R. Ventura

INAF Osservatorio Astrofisico di Catania, Via S.Sofia 78, 95123, Catania, Italy

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P.A. Wilson

P.A. Wilson

Nordic Optical Telescope, Apartado 474, E-38700 Santa Cruz de la Palma, Santa Cruz de Tenerife, Spain

Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway

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First published: 22 November 2010
Citations: 8

Abstract

We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5 days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation can clearly be distinguished in each star. We discuss the appearance of the oscillation spectra, including the presence of a possible signature of faculae, and the presence of mixed modes in one of the three stars (© 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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