38. PM July 2004 July 2004 July 2008 September 2008 Did HR 8799 planets formed in a dust/gas disk?
39. Solar system formation leftover vs HR 8799 Spitzer IR excess, dust at ~10 AU (asteroid belt?) IRAS/ISO IR excess, dust at ~100 AU (Kuiper belt?) Spitzer dust emission at ~1000 AU (collisions+Prad?)
40. Also... A NEW PLANET! Coming 2010 in a Journal near you... CLASSIFIED SORRY... AREA 51 AREA 51 AREA 51 AREA 51 Ok - a small preview... ... but do not ask any question about it...
41. The near future with the Gemini Planet Imager Gemini Planet Imager GPI.berkeley.edu When: 2011 Where: Gemini South Who: PI’s B. Macintosh & J. Graham How: High-order AO with coronagraphy What: 0.9 – 2.4 icrons, m I < 9 mag stars, polarimetry, R~40 spectroscopy
42. Keck 10s 10s with GPI Keck 20 minutes (ADI) Simulated HR8799 system with GPI
45. Affordable? 2,000 years old question - answer cost ~1B US $ (1,400$ per day of waiting or 0.14$/Earthling) 2 B$ or 150 M$ per day or also one Avatar movie...
46. Life in the Galaxy Drake’s equation N = N s f p n e f l f i f c f L 100 billions 50% 1 50% 20% 20% 10,000 years 1000 systems & life like us?!?! Fermi’s paradox: where are they?