Keith Horne: Extra-solar planets

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Radius vs Mass At least 2 parameters Rapid inward migration ---> no time to cool
Wide Transit Survey Discovery Potential Assume HD 209458 (V=7.6 mag) is brightest. mag 8 9 10 11 12 13 all sky 1 4 16 64 256 1024 16 o x16 o - - 0.1 0.4 1.6 7 How long to find them all ? ~ 150 16 o x16 o fields ~ 2 months / field ~ 25/N years N = number of 16 o x16 o cameras
Page 1 and 2: Extra-Solar Planets The Ongoing Dis
Page 4 and 5: Direct Imaging HARD! Extreme Adapti
Page 6: Exoplanet Discovery Space Jupiter E
Page 9 and 10: 1995 First Doppler Wobble Planet: 5
Page 11 and 12: Wide range of planet masses and orb
Page 13 and 14: High metalicity of planet host star
Page 15 and 16: Lessons from Doppler Wobbles • >
Page 17 and 18: Computer simulations of planet form
Page 19 and 20: Ida & Lin Model Distribution Observ
Page 22 and 23: Transit Lightcurves Depth: ∆f f r
Page 24 and 25: STARE data HD 209458 “Bloated”
Page 26 and 27: HST: Fit Residuals ~10 -4 No Moons
Page 28 and 29: HST Transit Spectroscopy detects Na
Page 30 and 31: Star occults planet 0.2 % Spitzer/I
Page 32 and 33: 19 mag = 1.3m OGLE 3 kpc 13 mag = 1
Page 34 and 35: 2004 Nov Deep surveys of Galactic P
Page 38 and 39: UK WASP Experiment Wide-Angle Searc
Page 40 and 41: How to find Earths ? • Hot Earths
Page 42 and 43: Hot Earths Transits from Space ∆f
Page 44 and 45: “The Habitable Zone” T~300K ⊕
Page 46 and 47: Gravitational Microlensing Hunting
Page 48 and 49: Lensing by a Star with a Planet Len
Page 50 and 51: Three-Stage Approach • Stage 1: d
Page 52 and 53: Planet Detection Zones OGLE III dat
Page 54 and 55: Microlens Follow-up Networks: PLANE
Page 56 and 57: RoboNet 1 --> REX REX = Robotic EXo
Page 58 and 59: OB-05-071 m ~ 3 m J Udalski et al.
Page 60 and 61: Ida & Lin Model Distribution Observ
Page 62 and 63: ESA: Darwin ~ 2015-20? infrared spa
Page 64 and 65: Life’s Signature: disequilibrium
Page 66 and 67: Thanks for listening!
Page 68: Thanks for listening!

Keith Horne: Extra-solar planets

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