NASA's Kepler mission will fly a photometer based on a wide-field Schmidt camera with a 0.95 m aperture, staring at a single field continuously for at least 4 years. Although the mission's principal aim is to locate transiting extrasolar planets, it will provide an unprecedented opportunity to make asteroseismic observations on a wide variety of stars. Plans are now being developed to exploit this opportunity to the fullest.
@article{arxiv.astro-ph/0701323,
title = {Asteroseismology with the Kepler mission},
author = {J. Christensen-Dalsgaard and T. Arentoft and T. M. Brown and R. L. Gilliland and H. Kjeldsen and W. J. Borucki and D. Koch},
journal= {arXiv preprint arXiv:astro-ph/0701323},
year = {2009}
}
Comments
Proc. Vienna Workshop on the Future of Asteroseismology, 20 - 22 September 2006. Comm. in Asteroseismology, Vol. 150, in the press