TPF-I SWG Report - Exoplanet Exploration Program - NASA
TPF-I SWG Report - Exoplanet Exploration Program - NASA
TPF-I SWG Report - Exoplanet Exploration Program - NASA
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Abstract<br />
Over the past two years, the focus of the project for the interferometric version of the Terrestrial Planet<br />
Finder (<strong>TPF</strong>-I) has been on the development of the scientific rational for the mission, the assessment of<br />
<strong>TPF</strong>-I architectures, the laboratory demonstration of key technologies, and the development of a detailed<br />
technology roadmap. The Science Working Group (<strong>SWG</strong>), in conjunction with European colleagues<br />
working on the European Space Agency’s (ESA’s) Darwin project, has reaffirmed the goals of <strong>TPF</strong>-I as<br />
part of a broad vision for the detection and characterization of Earth-like planets orbiting nearby stars and<br />
for the search for life on those planets. The <strong>SWG</strong> also helped to assess the performance of different<br />
interferometric configurations for <strong>TPF</strong>-I/Darwin. Building on earlier <strong>SWG</strong> reports, this document restates<br />
the scientific case for <strong>TPF</strong>-I, assesses suitable target stars and relevant wavelengths for observation,<br />
discusses dramatic new capabilities for general astrophysical observations, and summarizes how Spitzer<br />
has improved our knowledge of the incidence of zodiacal emission on the search for planets. This<br />
document discusses in some detail on laboratory advances in interferometric nulling and formation flying.<br />
Laboratory experiments have now achieved stable narrow- and broad-band nulling the levels of 10 -6 and<br />
2.0×10 -5 , respectively. A testbed has demonstrated formation flying using two realistic spacecraft<br />
mockups. With a suitably funded program of technology development, as summarized herein and<br />
described in more detail in the Technology Plan for the Terrestrial Planet Finder Interferometer (2005),<br />
the National Aeronautics and Space Administration (<strong>NASA</strong>) and ESA would be able to start within the<br />
coming decade a full-scale <strong>TPF</strong>-I/Darwin mission capable of finding Earths orbiting more than 150<br />
nearby stars, or a scaled back interferometer capable of studying more than 30 stars. Finding evidence for<br />
life on just one of those planets would revolutionize our understanding of our place in the cosmos.<br />
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