ASTEROSEISMOLOGY: THE NEXT FRONTIER IN STELLAR ASTROPHYHSICS A Science White Paper for the Astro 2010 Decadal Survey Submitted for consideration by the Stars and Stellar Evolution Panel Mark S. Giampapa National Solar Observatory 950 N. Cherry Ave. POB 26732 Tucson, AZ 85726-6732
[email protected] 520-318-8236 Conny Aerts, K.U.Leuven (Belgium) Tim Bedding, University of Sydney (Australia) Alfio Bonanno, INAF/Catania Astrophysical Observatory (Italy) Timothy M. Brown, Las Cumbres Observatory Global Telescope Jørgen Christensen-Dalsgaard, Aarhus University (Denmark) Martin Dominik, University of St. Andrews (UK) Jian Ge, University of Florida Ronald L. Gilliland, Space Telescope Science Institute J. W. Harvey, National Solar Observatory Frank Hill, National Solar Observatory Steven D. Kawaler, Iowa State University Hans Kjeldsen, Aarhus University (Denmark) D.W Kurtz, University of Lancaster (UK) Geoffrey W. Marcy, University of California Berkeley Jaymie M. Matthews, University of British Columbia Mario Joao P. F. G. Monteiro, University of Portugal Jesper Schou, Stanford University 1. Introduction The foundation of modern astrophysics, most especially the distance scale to the galaxies and the ages of stellar clusters, is based on a quantitative understanding of the fundamental parameters of stars: mass, age, chemical composition, and mixing length. The detection and measurement of acoustic (p-mode) oscillations in solar-type stars offers a new approach to measuring these parameters with significantly higher precision than has previously