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Astrometric Search for Planets • Astrometry measures positional wobble due to planets • Interferometry enables measurements at the microarcsecond level • Result of new observing systems will be a census of planets down to a few M earth over the next 10-20 years
• Make astrometric census of planets • Detect “Hot Jupiter’s” • Detect exo-zodiacal dust clouds • Image protostellar disks Interferometery Is One Key to Planet Detection • Break link between diameter, baseline • Enables precision astrometry, high resolution imaging, starlight nulling
Page 1 and 2: The Search for (Habitable) Planets
Page 3 and 4: Organic Chemistry Ubiquitous: Comet
Page 5 and 6: …and distant galaxies • Polycyc
Page 7 and 8: Earth’s Gases With And Without Li
Page 9 and 10: Star Formation & Protoplanetary Dis
Page 11 and 12: SIRTF Observations of Disks •NASA
Page 13 and 14: • Observations at 24, 70, 160 µm
Page 15: Transit Determines Planet’s Prope
Page 19 and 20: Search for Planets Around Young Sta
Page 21 and 22: The Challenge of Angular Resolution
Page 23 and 24: TPF Science Requirements-I • Dete
Page 25 and 26: TPF Candidate Architectures • Vis
Page 27 and 28: Visible Light Planet Detection •
Page 29 and 30: IR Interferometer Goal Earth at 10
Page 31 and 32: Selection of Final Architecture Jun
Page 33: Collaboration on TPF/Darwin • Str

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