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A PRECISE ASTEROSEISMIC AGE AND RADIUS FOR THE EVOLVED SUN-LIKE STAR KIC 11026764

Title
A PRECISE ASTEROSEISMIC AGE AND RADIUS FOR THE EVOLVED SUN-LIKE STAR KIC 11026764
Type
Article in International Scientific Journal
Year
2010
Authors
Metcalfe, TS
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Thompson, MJ
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Molenda Zakowicz, J
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Appourchaux, T
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Chaplin, WJ
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Dogan, G
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Eggenberger, P
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Bedding, TR
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Bruntt, H
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Creevey, OL
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O Quirion
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Stello, D
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Bonanno, A
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Silva S Aguirre
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Basu, S
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Esch, L
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Gai, N
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di Mauro, MP
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Kosovichev, AG
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Kitiashvili, IN
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Suarez, JC
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Moya, A
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Piau, L
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Garcia, RA
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Marques, JP
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Frasca, A
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Biazzo, K
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Sousa, SG
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Dreizler, S
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Bazot, M
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Karoff, C
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Frandsen, S
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Wilson, PA
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Brown, TM
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Christensen Dalsgaard, J
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Gilliland, RL
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Kjeldsen, H
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Campante, TL
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Fletcher, ST
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Handberg, R
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Regulo, C
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Salabert, D
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Schou, J
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Verner, GA
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Ballot, J
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M Broomhall
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Elsworth, Y
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Hekker, S
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Huber, D
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Mathur, S
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New, R
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Roxburgh, IW
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Sato, KH
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White, TR
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Borucki, WJ
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Koch, DG
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Jenkins, JM
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Journal
Title: Astrophysical JournalImported from Authenticus Search for Journal Publications
Vol. 723
Pages: 1583-1598
ISSN: 0004-637X
Scientific classification
FOS: Natural sciences > Physical sciences
CORDIS: Physical sciences > Astronomy
Other information
Authenticus ID: P-003-11E
Abstract (EN): The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-like planets. The asteroseismic capabilities of the mission are being used to determine precise radii and ages for the target stars from their solar-like oscillations. Chaplin et al. published observations of three bright G-type stars, which were monitored during the first 33.5 days of science operations. One of these stars, the subgiant KIC 11026764, exhibits a characteristic pattern of oscillation frequencies suggesting that it has evolved significantly. We have derived asteroseismic estimates of the properties of KIC 11026764 from Kepler photometry combined with ground-based spectroscopic data. We present the results of detailed modeling for this star, employing a variety of independent codes and analyses that attempt to match the asteroseismic and spectroscopic constraints simultaneously. We determine both the radius and the age of KIC 11026764 with a precision near 1%, and an accuracy near 2% for the radius and 15% for the age. Continued observations of this star promise to reveal additional oscillation frequencies that will further improve the determination of its fundamental properties.
Language: English
Type (Professor's evaluation): Scientific
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