W. J. Borucki, Science, vol.327, p.977, 2010.

W. J. Borucki, Science, vol.325, p.709, 2009.

R. L. Gilliland, Pub. Astron. Soc. Pac, vol.122, p.131, 2010.

D. Stello, Astrophys. J, vol.700, p.1589, 2009.

J. Christensen-dalsgaard, Astrophys. J, vol.713, p.164, 2010.

R. A. García, Science, vol.329, p.1032, 2010.

D. H. Hathaway and L. Rightmire, Science, vol.327, p.1035, 2010.

A. Broomhall, Astrophys. J, vol.700, p.162, 2009.

T. M. Brown and R. L. Gilliland, Ann. Rev. Astron. & Astrophys, vol.32, p.37, 1994.

J. Christensen-dalsgaard, Sol. Phys, vol.220, p.137, 2004.

G. Houdek, Astron. & Astrophys, vol.351, p.582, 1999.

R. Samadi, Astron. & Astrophys, vol.463, p.297, 2007.

D. O. Gough, Science, vol.272, p.1296, 1996.

J. Christensen-dalsgaard, Rev. Mod. Phys, vol.74, p.1073, 2002.

S. V. Vorontsov, Nature, vol.349, p.49, 1991.

C. Aerts, J. Christensen-dalsgaard, M. Cunha, and D. W. Kurtz, Sol. Phys, vol.251, p.3, 2008.

T. R. Bedding and H. Kjeldsen, 14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, vol.384, p.21, 2008.

T. R. Bedding, Astrophys. J, vol.713, p.935, 2010.

T. Appourchaux, Astron. & Astrophys, vol.488, p.705, 2008.

E. Michel, Science, vol.322, p.558, 2008.

W. J. Chaplin, Astrophys. J, vol.713, p.169, 2010.

, Solar-type stars oscillate in non-radial modes. The radial part is described by the order (i.e., overtone number) n, while the surface pattern may be described in terms of a spherical harmonic function of degree, l and azimuthal order m. The large separation is the separation

T. M. Brown, R. L. Gilliland, R. W. Noyes, and L. W. Ramsey, Astrophys. J, vol.368, p.599, 1991.

H. Kjeldsen and T. R. Bedding, Astron. & Astrophys, vol.293, 1995.

D. An, Astrophys J, vol.700, p.523, 2009.

T. M. Brown, Astrophys J. submitted, 2011.

, Materials and methods are available as supporting material on Science online

J. D. Ridder, Nature, vol.459, p.398, 2009.

T. R. Bedding, Astrophys. J, vol.713, p.176, 2010.

T. S. Metcalfe, Astrophys. J, vol.723, p.1583, 2010.

C. Turon, ESA-ESO Working Group on Galactic Populations, Chemistry and Dynamics, 2008.
URL : https://hal.archives-ouvertes.fr/hal-00492481

G. Torres, Astron. Astrophys. Rev, vol.18, p.67, 2010.

P. Marigo, Astron. & Astrophys, vol.483, p.883, 2008.

L. Girardi, Astron. & Astrophys, vol.436, p.895, 2005.

A. Miglio, Astron. & Astrophys, vol.523, p.21, 2009.

R. Gilliland, J. M. Jenkins, and W. J. Borucki, whose funding is provided by NASA's Science Mission Directorate. The authors thank the entire Kepler team, without whom these results would not be possible. The asteroseismology program of Kepler is being conducted by the Kepler, Asteroseismology Science Consortium. References S1, vol.713, p.160, 2009.

. S2, J. M. Jenkins, D. A. Caldwell, and H. Chandrasekaran, ApJ, vol.713, p.120, 2010.

. S3, T. M. Brown, D. W. Latham, M. E. Everett, and G. A. Esquerdo, ApJ, 2011.

. S4, N. M. Batalha, J. F. Rowe, and R. L. Gilliland, ApJ, vol.713, p.109, 2010.

. S5, R. A. García, S. Turck-chièze, and P. Boumier, A&A, vol.442, p.385, 2005.

. S6, T. L. Campante, C. Karoff, W. J. Chaplin, Y. Elsworth et al., MNRAS, vol.408, p.542, 2010.

J. S7.-christensen-dalsgaard, T. Arentoft, T. M. Brown, R. L. Gilliland, H. Kjeldsen et al., J. Phys. Conf. Ser, vol.118, p.12039, 2008.

. S8, S. Hekker, A. Broomhall, and W. J. Chaplin, MNRAS, vol.402, p.2049, 2010.

. S9, D. Huber, D. Stello, T. R. Bedding, W. J. Chaplin et al., , vol.160, p.74, 2009.

. S10, C. Karoff, T. L. Campante, and W. J. Chaplin, , 2010.

. S11, B. Mosser, and T. Appourchaux, A&A, vol.508, p.877, 2009.

. S12, S. Mathur, R. A. García, and C. Régulo, A&A, vol.511, p.46, 2010.

. S13 and I. W. Roxburgh, A&A, vol.506, p.435, 2009.

. S14, W. J. Chaplin, T. Appourchaux, and T. Arentoft, AN, vol.329, p.549, 2008.

. S15, D. Stello, W. J. Chaplin, and H. Bruntt, ApJ, vol.700, p.1589, 2009.

J. S16.-christensen-dalsgaard, ASP. Conf. Ser. 42, Proc. GONG 1992, Seismic Investigation of the Sun and Stars, p.347, 1993.

H. S17.-kjeldsen and T. R. Bedding, A&A, vol.293, p.87, 1995.

. S18, T. R. Bedding, and H. Kjeldsen, PASA, vol.20, p.203, 2003.

. S19, W. J. Chaplin, G. Houdek, T. Appourchaux, Y. Elsworth et al., A&A, vol.485, p.813, 2008.

. S20, B. Mosser, K. Belkacem, and M. Goupil, A&A, vol.517, p.22, 2010.

. S21, T. Kallinger, W. W. Weiss, and C. Barban, A&A, vol.509, p.77, 2010.

D. S22.-an, M. H. Pinsonneault, and T. Masseron, ApJ, vol.700, p.523, 2009.

. S23, S. Basu, W. J. Chaplin, and Y. Elsworth, ApJ, vol.710, p.1596, 2010.

P. S24.-quirion, J. Christensen-dalsgaard, and T. Arentoft, ApJ, vol.725, p.2176, 2010.

. S25, N. Gai, S. Basu, W. J. Chaplin, and Y. Elsworth, ApJ, vol.730, p.63, 2011.

H. S26.-kjeldsen, T. R. Bedding, and J. Christensen-dalsgaard, ApJ, vol.683, p.175, 2008.

. S27, H. Bruntt, T. R. Bedding, and P. Quirion, MNRAS, vol.405, p.1907, 2010.

. S28, L. Girardi, A. Bressan, G. Bertelli, and C. Chiosi, A&ASS, vol.141, p.371, 2000.

. S29, M. A. Perryman, L. Lindegren, and J. Kovalevsky, A&A, vol.323, p.49, 1997.

. S30, R. M. Cutri, M. F. Skrutskie, and S. Van-dyk, 2MASS All Sky Catalog of point sources S31, A&A, vol.379, p.740, 2001.

. S32, P. S. Osmer, J. D. Kennefick, P. B. Hall, and R. F. Green, ApJS, vol.119, p.189, 1998.

. S33, D. J. Schlegel, D. P. Finkbeiner, and M. Davis, ApJ, vol.500, p.525, 1998.

. S34 and T. Appourchaux, A&A, vol.428, p.1039, 2004.

. S35, A. Broomhall, W. J. Chaplin, Y. Elsworth, T. Appourchaux et al., MNRAS, vol.406, p.767, 2010.

S. Figure, Large frequency separations, ??, and frequencies of maximum oscillations power, ? max