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…Star & Planet Forming Regions… IR, submm, mm spectra reveal gas phase, ices, mineralogical signatures of many species, incl: H 2 O, CO 2 , CH 3 OH, CO, CH 4 , formic acid (HCOOH) and formaldehyde (H 2 CO), etc.
…and distant galaxies • Polycyclic Aromatic Hydrocarbons (PAHs) – Complex 2-D carbon molecules (>25 carbon atoms) – Found in many active galaxies PAH ?? Barthel 2001 z=1.5 • Perhaps in distant quasar at z~1.5 (wait for SIRTF) • CO detected in a very distant quasar (z=4.1!) – Found with more complex species in more nearby objects Pierre et al 2001
Page 1 and 2: The Search for (Habitable) Planets
Page 3: Organic Chemistry Ubiquitous: Comet
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 and 16: Transit Determines Planet’s Prope
Page 17 and 18: • Make astrometric census of plan
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

Santa Cruz

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