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Astronomy 305/Frontiers in Astronomy Class web site: http://glast.sonoma.edu/~lynnc/courses/a305 Office: Darwin 329A and NASA E/PO (707) 664-2655 Best way to reach me: [email protected] 10/7/03 Prof. Lynn Cominsky 1 Astrobiology Questions (3 weeks) Is there life elsewhere in our Solar system? Are Earth-like planets common? Are we alone? 10/7/03 Prof. Lynn Cominsky 2 Group 6 10/7/03 Prof. Lynn Cominsky 3 Are Earth-like planets common? 10/7/03 Prof. Lynn Cominsky 4 Question to ponder: When will Voyager get to the next star? It was launched in 1977 and has just passed Pluto. A) 2020 AD B) 8200 AD C) 82,000 AD D) 182,000 AD 10/7/03 Prof. Lynn Cominsky 5 Answer Voyager is travelling about 37,000 mph, which is about c/20000 The nearest star (Proxima Centauri) is about 4 light years away It will therefore take about 80,000 years to reach Proxima Centauri The correct answer is therefore C 10/7/03 Prof. Lynn Cominsky 6 Planets around other stars Over 100 planets around other stars are known 10/7/03 Prof. Lynn Cominsky 7 Planets around other stars PSR 1257+12 (a radio pulsar, Wolczan 1995) 3 objects orbiting this stellar corpse 1 is the size of the Moon 2 are the size of the Earth probably formed after the supernova explosion that made the pulsar 51 Pegasi (Sun-like star, Mayor and Queloz 1996) at least one object, about 1/2 of Jupiter orbit of only 4 days closer to star than Mercury, so very hot 42 light years from Earth 10/7/03 Prof. Lynn Cominsky 8 Planets around other stars 70 Virginis (Sun-like star, Marcy and Butler 1996) 116 day orbit 9 Jupiter masses (1 Jupiter = 317 Earth masses) temperature of planet may allow liquid water to exist 78 light years from Earth 47 Ursae Majoris (Marcy and Butler 1996) 1100 day orbit 3 Jupiter masses temperature of planet may allow liquid water to exist 44 light years from Earth 10/7/03 Prof. Lynn Cominsky 9 Another solar system Upsilon Andromedae: Multiple planet solar system discovered by Marcy et al. a) 4.6 d b) 240 d c) 1313 d Ups And 10/7/03 Prof. Lynn Cominsky 10 How they find extra-solar planets Stars are too bright to see reflected light from planets directly Unseen planet causes star to wobble as it orbits – star’s light is Doppler shifted 10/7/03 Prof. Lynn Cominsky 11 Doppler Shift Wavelength is shorter when approaching Stationary waves Wavelength is longer when receding 10/7/03 Prof. Lynn Cominsky 12 Doppler Shift Comparison of laboratory to blue-shifted object Comparison of laboratory to red-shifted object 10/7/03 Prof. Lynn Cominsky 13 Doppler Shift Doppler shift song by AstroCapella 10/7/03 Prof. Lynn Cominsky 14 Other methods: Astrometry – measuring the exact position of a star as it wobbles Hipparcos was an ESA satellite operational from 1989-93 10/7/03 Prof. Lynn Cominsky 15 Other methods: Photometry – measuring the change in brightness of a star as a planet transits in front of it, obscuring some of the light (~2%) 10/7/03 Prof. Lynn Cominsky 16 The first transiting planet HD209548 – a visualization by Aurore Simonnet 10/7/03 Prof. Lynn Cominsky 17 The first transiting planet STARE project found the first transit in HD209548 – Brown and Charbonneau 1999 The planet’s mass is 63% of Jupiter (about 200 Earth masses) with radius 1.3 times Jupiter density 0.39 g/cm3 (< water!) It transits the star every 3.5 days Its atmosphere is very hot (1100oC) since it is only 6.4 million km from the star When the planet passed in front of the star, the star’s light passed through the planet’s atmosphere and sodium was observed by HST 10/7/03 Prof. Lynn Cominsky 18 Saturn mass planets (95 times Earth) Both planets are very close to their stars This makes them easier to detect If each planet orbited the Earth’s Sun: 10/7/03 Prof. Lynn Cominsky 19 Latest news (7/03) (See exoplanets.org) 110 planets are now known outside our solar system Earlier searches preferentially found closer orbiting planets, more massive planets and eccentric orbits (“hot Jupiters”) – now smaller planets are being found in orbits that are closer and more circular Jupiter-analog found around HD70642 Sub-Saturn planet found around HD 3651 10/7/03 Prof. Lynn Cominsky 20 Iron abundance vs. planets The probability that a star harbors a planet depends on the star's metal content. 10/7/03 Prof. Lynn Cominsky 21 Inventing Alien Life forms This activity is from the Univ. of Washington http://www.astro.washington.edu/labs/clearinghouse /activities/aliens.html Take one dice for each group of 2 students and try the evolution experiment to create your own alien. The rolling of the dice reproduces the random elements in evolution. When you have finished, draw a picture of your alien and give it a a name 10/7/03 Prof. Lynn Cominsky 22 Inventing Alien Life forms Write a paragraph that has the following information: Describe the environment your creature needs to survive. Where in our solar system would you be most likely to find such a creature? What sort of food source might your creature need? Is your creature alone in its environment? If not, how does it coexist with other species? 10/7/03 Prof. Lynn Cominsky 23 Web Resources Voyager mission http://vraptor.jpl.nasa.gov/voyager/voyager.html Extra-solar planet searches http://exoplanets.org STARE: http://www.hao.ucar.edu/public/research/stare/stare. html Latest news: (and a cool interactive) http://planetquest.jpl.nasa.gov/news/tau1_gruis.html Hipparcos Space Astrometry Mission http://astro.estec.esa.nl/Hipparcos/ 10/7/03 Prof. Lynn Cominsky 24