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Life in the Universe I. astronomy Páll Jakobsson (Palli) (pja@hi.is) 10 January 2013 “If you wish to make an apple pie from scratch, you must first invent the Universe.” Carl Sagan (1934-1996)
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1. Inngangur 1.1 Aaaaa 1.2 Bbbbb Distance: 25 light years
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Tracking Fomalhaut b from 2004-2012
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4 Distance: 130 light years
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Distance: 25 light years Distance: 70 light years M = 9 ∙ M Jupiter
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Known Exoplanets 1992: a few are discovered around a neutron star! 1995: the first around Sun-like star (indirect measurement). January 2013: 854 (http://exoplanet.eu): 1)Radial velocity + astrometry: 498 (386 planetary systems) 2)Transits: 291 (236 planetary systems) 3)Microlensing: 16 (15 planetary systems) 4)Imaging: 32 (28 planetary systems) 1), 2) and 3) are indirect measurements.
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Venus Transit in June 2012
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9 Transit Graph
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10 Transit Graph Provides information on the radius of the exoplanet.
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11 Probability of a Transit Detection?
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12 Where is Kepler Looking?
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The Kepler Planet Candidates (~2300) (NB: only 105 confirmed planets)
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Kepler-20: An Unusual Planetary System (5 planets in small orbits)
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Kepler-20: large, small, large, small, large Kepler-20b: 1.9 ∙ R Earth Kepler-20e: 0.9 ∙ R Earth Kepler-20c: 3.1 ∙ R Earth Kepler-20f: 1.0 ∙ R Earth Kepler-20d: 2.8 ∙ R Earth 760 °C 430 °C
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(the first rocky exoplanet to be discovered)
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18 6 planets!
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19 The Habitable Zone (shown in green)
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Earth 2.0
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Kepler-47 (a system with more than one planet orbiting a pair of stars)
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26 Astrometry (ísl: stjörnuvagg) A system of two (or more) bodies orbit around their mutual centre of mass. The change in the stellar position (wobble) gives the planet mass. Example: M Jupiter and d = 1 AU. Assume the system lies 3 light years from Earth. Stellar wobble: 1 milliarcsecond. Now put an “Earth” instead and move the system to 30 light years. Stellar wobble: 0.3 microarcsecond. No chance measuring that today. SIM PlanetQuest: 2016?
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Motion of the Sun (distance: 30 ly)
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