The asteroseismic potential of kepler: First results for solar-type stars

W. J. Chaplin; T. Appourchaux; Y. Elsworth; R. A. García; G. Houdek; C. Karoff; T. S. Metcalfe; J. Molenda-Akowicz; M. J.P.F.G. Monteiro; M. J. Thompson; T. M. Brown; J. Christensen-Dalsgaard; R. L. Gilliland; H. Kjeldsen; W. J. Borucki; D. Koch; J. M. Jenkins; J. Ballot; S. Basu; M. Bazot; T. R. Bedding; O. Benomar; A. Bonanno; I. M. Brandão; H. Bruntt; T. L. Campante; O. L. Creevey; M. P.Di Mauro; G. Doan; S. Dreizler; P. Eggenberger; L. Esch; S. T. Fletcher; S. Frandsen; N. Gai; P. Gaulme; R. Handberg; S. Hekker; R. Howe; D. Huber; S. G. Korzennik; J. C. Lebrun; S. Leccia; M. Martic; S. Mathur; B. Mosser; R. New; P. O. Quirion; C. Régulo; I. W. Roxburgh; D. Salabert; J. Schou; S. G. Sousa; D. Stello; G. A. Verner; T. Arentoft; C. Barban; K. Belkacem; S. Benatti; K. Biazzo; P. Boumier; P. A. Bradley; A. M. Broomhall; D. L. Buzasi; R. U. Claudi; M. S. Cunha; F. D'Antona; S. Deheuvels; A. Derekas; A. García Hernndez; M. S. Giampapa; M. J. Goupil; M. Gruberbauer; J. A. Guzik; S. J. Hale; M. J. Ireland; L. L. Kiss; I. N. Kitiashvili; K. Kolenberg; H. Korhonen; A. G. Kosovichev; F. Kupka; Y. Lebreton; B. Leroy; H. G. Ludwig; S. Mathis; E. Michel; A. Miglio; J. Montalbn; A. Moya; A. Noels; R. W. Noyes; P. L. Pallé; L. Piau; H. L. Preston; T. Roca Cortés; M. Roth; K. H. Sato; J. Schmitt; A. M. Serenelli; V. Silva Aguirre; I. R. Stevens; J. C. Surez; M. D. Suran; R. Trampedach; S. Turck-Chièze; K. Uytterhoeven; R. Ventura; P. A. Wilson

doi:10.1088/2041-8205/713/2/L169

The asteroseismic potential of kepler: First results for solar-type stars

W. J. Chaplin, T. Appourchaux, Y. Elsworth, R. A. García, G. Houdek, C. Karoff, T. S. Metcalfe, J. Molenda-Akowicz, M. J.P.F.G. Monteiro, M. J. Thompson, T. M. Brown, J. Christensen-Dalsgaard, R. L. Gilliland, H. Kjeldsen, W. J. Borucki, D. Koch, J. M. Jenkins, J. Ballot, S. Basu, M. BazotT. R. Bedding, O. Benomar, A. Bonanno, I. M. Brandão, H. Bruntt, T. L. Campante, O. L. Creevey, M. P.Di Mauro, G. Doan, S. Dreizler, P. Eggenberger, L. Esch, S. T. Fletcher, S. Frandsen, N. Gai, P. Gaulme, R. Handberg, S. Hekker, R. Howe, D. Huber, S. G. Korzennik, J. C. Lebrun, S. Leccia, M. Martic, S. Mathur, B. Mosser, R. New, P. O. Quirion, C. Régulo, I. W. Roxburgh, D. Salabert, J. Schou, S. G. Sousa, D. Stello, G. A. Verner, T. Arentoft, C. Barban, K. Belkacem, S. Benatti, K. Biazzo, P. Boumier, P. A. Bradley, A. M. Broomhall, D. L. Buzasi, R. U. Claudi, M. S. Cunha, F. D'Antona, S. Deheuvels, A. Derekas, A. García Hernndez, M. S. Giampapa, M. J. Goupil, M. Gruberbauer, J. A. Guzik, S. J. Hale, M. J. Ireland, L. L. Kiss, I. N. Kitiashvili, K. Kolenberg, H. Korhonen, A. G. Kosovichev, F. Kupka, Y. Lebreton, B. Leroy, H. G. Ludwig, S. Mathis, E. Michel, A. Miglio, J. Montalbn, A. Moya, A. Noels, R. W. Noyes, P. L. Pallé, L. Piau, H. L. Preston, T. Roca Cortés, M. Roth, K. H. Sato, J. Schmitt, A. M. Serenelli, V. Silva Aguirre, I. R. Stevens, J. C. Surez, M. D. Suran, R. Trampedach, S. Turck-Chièze, K. Uytterhoeven, R. Ventura, P. A. Wilson

Center for Space Science

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

Abstract

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses, and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.

Original language	English (US)
Pages (from-to)	L169-L175
Journal	Astrophysical Journal Letters
Volume	713
Issue number	2 PART 2
DOIs	https://doi.org/10.1088/2041-8205/713/2/L169
State	Published - 2010

Keywords

Stars: interiors
Stars: late-type
Stars: oscillations

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1088/2041-8205/713/2/L169

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Chaplin, W. J., Appourchaux, T., Elsworth, Y., García, R. A., Houdek, G., Karoff, C., Metcalfe, T. S., Molenda-Akowicz, J., Monteiro, M. J. P. F. G., Thompson, M. J., Brown, T. M., Christensen-Dalsgaard, J., Gilliland, R. L., Kjeldsen, H., Borucki, W. J., Koch, D., Jenkins, J. M., Ballot, J., Basu, S., ... Wilson, P. A. (2010). The asteroseismic potential of kepler: First results for solar-type stars. Astrophysical Journal Letters, 713(2 PART 2), L169-L175. https://doi.org/10.1088/2041-8205/713/2/L169

Chaplin, WJ, Appourchaux, T, Elsworth, Y, García, RA, Houdek, G, Karoff, C, Metcalfe, TS, Molenda-Akowicz, J, Monteiro, MJPFG, Thompson, MJ, Brown, TM, Christensen-Dalsgaard, J, Gilliland, RL, Kjeldsen, H, Borucki, WJ, Koch, D, Jenkins, JM, Ballot, J, Basu, S, Bazot, M, Bedding, TR, Benomar, O, Bonanno, A, Brandão, IM, Bruntt, H, Campante, TL, Creevey, OL, Mauro, MPD, Doan, G, Dreizler, S, Eggenberger, P, Esch, L, Fletcher, ST, Frandsen, S, Gai, N, Gaulme, P, Handberg, R, Hekker, S, Howe, R, Huber, D, Korzennik, SG, Lebrun, JC, Leccia, S, Martic, M, Mathur, S, Mosser, B, New, R, Quirion, PO, Régulo, C, Roxburgh, IW, Salabert, D, Schou, J, Sousa, SG, Stello, D, Verner, GA, Arentoft, T, Barban, C, Belkacem, K, Benatti, S, Biazzo, K, Boumier, P, Bradley, PA, Broomhall, AM, Buzasi, DL, Claudi, RU, Cunha, MS, D'Antona, F, Deheuvels, S, Derekas, A, Hernndez, AG, Giampapa, MS, Goupil, MJ, Gruberbauer, M, Guzik, JA, Hale, SJ, Ireland, MJ, Kiss, LL, Kitiashvili, IN, Kolenberg, K, Korhonen, H, Kosovichev, AG, Kupka, F, Lebreton, Y, Leroy, B, Ludwig, HG, Mathis, S, Michel, E, Miglio, A, Montalbn, J, Moya, A, Noels, A, Noyes, RW, Pallé, PL, Piau, L, Preston, HL, Cortés, TR, Roth, M, Sato, KH, Schmitt, J, Serenelli, AM, Aguirre, VS, Stevens, IR, Surez, JC, Suran, MD, Trampedach, R, Turck-Chièze, S, Uytterhoeven, K, Ventura, R & Wilson, PA 2010, 'The asteroseismic potential of kepler: First results for solar-type stars', Astrophysical Journal Letters, vol. 713, no. 2 PART 2, pp. L169-L175. https://doi.org/10.1088/2041-8205/713/2/L169

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title = "The asteroseismic potential of kepler: First results for solar-type stars",

abstract = "We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses, and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.",

keywords = "Stars: interiors, Stars: late-type, Stars: oscillations",

author = "Chaplin, {W. J.} and T. Appourchaux and Y. Elsworth and Garc{\'i}a, {R. A.} and G. Houdek and C. Karoff and Metcalfe, {T. S.} and J. Molenda-Akowicz and Monteiro, {M. J.P.F.G.} and Thompson, {M. J.} and Brown, {T. M.} and J. Christensen-Dalsgaard and Gilliland, {R. L.} and H. Kjeldsen and Borucki, {W. J.} and D. Koch and Jenkins, {J. M.} and J. Ballot and S. Basu and M. Bazot and Bedding, {T. R.} and O. Benomar and A. Bonanno and Brand{\~a}o, {I. M.} and H. Bruntt and Campante, {T. L.} and Creevey, {O. L.} and Mauro, {M. P.Di} and G. Doan and S. Dreizler and P. Eggenberger and L. Esch and Fletcher, {S. T.} and S. Frandsen and N. Gai and P. Gaulme and R. Handberg and S. Hekker and R. Howe and D. Huber and Korzennik, {S. G.} and Lebrun, {J. C.} and S. Leccia and M. Martic and S. Mathur and B. Mosser and R. New and Quirion, {P. O.} and C. R{\'e}gulo and Roxburgh, {I. W.} and D. Salabert and J. Schou and Sousa, {S. G.} and D. Stello and Verner, {G. A.} and T. Arentoft and C. Barban and K. Belkacem and S. Benatti and K. Biazzo and P. Boumier and Bradley, {P. A.} and Broomhall, {A. M.} and Buzasi, {D. L.} and Claudi, {R. U.} and Cunha, {M. S.} and F. D'Antona and S. Deheuvels and A. Derekas and Hernndez, {A. Garc{\'i}a} and Giampapa, {M. S.} and Goupil, {M. J.} and M. Gruberbauer and Guzik, {J. A.} and Hale, {S. J.} and Ireland, {M. J.} and Kiss, {L. L.} and Kitiashvili, {I. N.} and K. Kolenberg and H. Korhonen and Kosovichev, {A. G.} and F. Kupka and Y. Lebreton and B. Leroy and Ludwig, {H. G.} and S. Mathis and E. Michel and A. Miglio and J. Montalbn and A. Moya and A. Noels and Noyes, {R. W.} and Pall{\'e}, {P. L.} and L. Piau and Preston, {H. L.} and Cort{\'e}s, {T. Roca} and M. Roth and Sato, {K. H.} and J. Schmitt and Serenelli, {A. M.} and Aguirre, {V. Silva} and Stevens, {I. R.} and Surez, {J. C.} and Suran, {M. D.} and R. Trampedach and S. Turck-Chi{\`e}ze and K. Uytterhoeven and R. Ventura and Wilson, {P. A.}",

year = "2010",

doi = "10.1088/2041-8205/713/2/L169",

language = "English (US)",

volume = "713",

pages = "L169--L175",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "2 PART 2",

}

TY - JOUR

T1 - The asteroseismic potential of kepler

T2 - First results for solar-type stars

AU - Chaplin, W. J.

AU - Appourchaux, T.

AU - Elsworth, Y.

AU - García, R. A.

AU - Houdek, G.

AU - Karoff, C.

AU - Metcalfe, T. S.

AU - Molenda-Akowicz, J.

AU - Monteiro, M. J.P.F.G.

AU - Thompson, M. J.

AU - Brown, T. M.

AU - Christensen-Dalsgaard, J.

AU - Gilliland, R. L.

AU - Kjeldsen, H.

AU - Borucki, W. J.

AU - Koch, D.

AU - Jenkins, J. M.

AU - Ballot, J.

AU - Basu, S.

AU - Bazot, M.

AU - Bedding, T. R.

AU - Benomar, O.

AU - Bonanno, A.

AU - Brandão, I. M.

AU - Bruntt, H.

AU - Campante, T. L.

AU - Creevey, O. L.

AU - Mauro, M. P.Di

AU - Doan, G.

AU - Dreizler, S.

AU - Eggenberger, P.

AU - Esch, L.

AU - Fletcher, S. T.

AU - Frandsen, S.

AU - Gai, N.

AU - Gaulme, P.

AU - Handberg, R.

AU - Hekker, S.

AU - Howe, R.

AU - Huber, D.

AU - Korzennik, S. G.

AU - Lebrun, J. C.

AU - Leccia, S.

AU - Martic, M.

AU - Mathur, S.

AU - Mosser, B.

AU - New, R.

AU - Quirion, P. O.

AU - Régulo, C.

AU - Roxburgh, I. W.

AU - Salabert, D.

AU - Schou, J.

AU - Sousa, S. G.

AU - Stello, D.

AU - Verner, G. A.

AU - Arentoft, T.

AU - Barban, C.

AU - Belkacem, K.

AU - Benatti, S.

AU - Biazzo, K.

AU - Boumier, P.

AU - Bradley, P. A.

AU - Broomhall, A. M.

AU - Buzasi, D. L.

AU - Claudi, R. U.

AU - Cunha, M. S.

AU - D'Antona, F.

AU - Deheuvels, S.

AU - Derekas, A.

AU - Hernndez, A. García

AU - Giampapa, M. S.

AU - Goupil, M. J.

AU - Gruberbauer, M.

AU - Guzik, J. A.

AU - Hale, S. J.

AU - Ireland, M. J.

AU - Kiss, L. L.

AU - Kitiashvili, I. N.

AU - Kolenberg, K.

AU - Korhonen, H.

AU - Kosovichev, A. G.

AU - Kupka, F.

AU - Lebreton, Y.

AU - Leroy, B.

AU - Ludwig, H. G.

AU - Mathis, S.

AU - Michel, E.

AU - Miglio, A.

AU - Montalbn, J.

AU - Moya, A.

AU - Noels, A.

AU - Noyes, R. W.

AU - Pallé, P. L.

AU - Piau, L.

AU - Preston, H. L.

AU - Cortés, T. Roca

AU - Roth, M.

AU - Sato, K. H.

AU - Schmitt, J.

AU - Serenelli, A. M.

AU - Aguirre, V. Silva

AU - Stevens, I. R.

AU - Surez, J. C.

AU - Suran, M. D.

AU - Trampedach, R.

AU - Turck-Chièze, S.

AU - Uytterhoeven, K.

AU - Ventura, R.

AU - Wilson, P. A.

PY - 2010

Y1 - 2010

N2 - We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses, and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.

AB - We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses, and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.

KW - Stars: interiors

KW - Stars: late-type

KW - Stars: oscillations

UR - http://www.scopus.com/inward/record.url?scp=77950577829&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=77950577829&partnerID=8YFLogxK

U2 - 10.1088/2041-8205/713/2/L169

DO - 10.1088/2041-8205/713/2/L169

M3 - Article

AN - SCOPUS:77950577829

SN - 2041-8205

VL - 713

SP - L169-L175

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2 PART 2

ER -

The asteroseismic potential of kepler: First results for solar-type stars

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Keywords

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