Terrestrial Planet Finder Coronagraph Science and Technology Definition
JPL Document D-34923 Terrestrial Planet Finder Coronagraph Science and Technology Definition Team (STDT) Report Editors: Marie Levine, Stuart Shaklan and James Kasting (Penn State University) June 12, 2006 National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California TPF-C STDT REPORT ii TPF-C STDT REPORT Approvals iii TPF-C STDT REPORT Goals for the Terrestrial Planet Finder Coronagraph Mission The question "are we alone?" has its roots deep in human consciousness, and its answer could revo- lutionize our world view. Starting with Galileo's invention of the telescope 400 years ago, which he used to prove the existence of other worlds, and continuing through a century of astonishing dis- coveries—galaxies, stars, planets, and distant oceans—science has given us a dramatically clearer pic- ture of the universe and our place within it. Today, we finally have tools within reach to seek life be- yond Earth, and to answer this age-old question. The Terrestrial Planet Finder-Coronagraph (TPF-C) mission is a giant step towards that goal. Over the last decade, extrasolar planets have been discovered around nearly 200 nearby stars. Most of these planetary systems are quite different from our own—with Jupiter-sized planets orbiting close to their parent stars—mainly because radial velocity measurements are most sensitive to such planets. New observing techniques, such as coronagraphy and nulling interferometry, are needed to detect smaller, Earth-like planets by their own light and to characterize them as possible harbors for life. Characterization of a terrestrial-sized planet at its most fundamental level means learning about its mass, diameter, temperature, and atmospheric and surface composition.
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