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We are not alone: Other planets, other earths?: 

Edmund Bertschinger MIT Department of Physics and Kavli Institute for Astrophysics and Space Research We are not alone: Other planets, other earths?

Earth and Mars – or Mars and Earth?: 

Earth and Mars – or Mars and Earth? Mars is drier than the Atacama (or Sahara) desert.

Life on Mars?: 

Life on Mars? R. Villard, STScI

Martian Meteorite found in Antarctica: 

Martian Meteorite found in Antarctica McKay et al. 1996: carbonate globules – evidence for microbial life? Lunar and Planetary Institute

Slide7: 

Methane rivers and oceans on Titan (Huygens lander, European Space Agency)

Family Portrait: 4 rocky planets, 2 gas giants, 2 ice giants: 

Family Portrait: 4 rocky planets, 2 gas giants, 2 ice giants

Slide10: 

Planets around other stars: exoplanets After 10 years of study, 170 known (California-Carnegie Planet Search, G. Marcy)

How to find other planetary systems: 

How to find other planetary systems Doppler measurement of stellar wobble: planets’ gravity pulls on star

Slide12: 

Figure from California-Carnegie Planet Search First success: 1995, Mayor and Queloz

How to find other planetary systems: 

How to find other planetary systems Transit: planet passes in front of star, dims the light a tiny amount

Slide14: 

Both the Doppler and Transit methods can much more easily find close-in, Jupiter mass planets than earth-like planets

How to find other planetary systems: 

How to find other planetary systems Infrared emission from dusty disks

How to find other planetary systems: 

How to find other planetary systems Direct imaging

How to find other planetary systems: 

How to find other planetary systems Gravitational Microlensing

Slide20: 

The gravity of a planet orbiting a star causes light rays to bend, changing the amount of light reaching the earth. Background star Enhanced image at earth 25 January 2006: the star OGLE-2005-BLG-390L has a planet of mass about 5 earth masses, in a 10-year orbit!

Family Comparison: 

Family Comparison

Family Comparison: 

Family Comparison R. Villard, STScI

What have we learned?: 

What have we learned? At least a few percent of sunlike stars have massive planets

What have we learned?: 

What have we learned? Surprise: “Hot Jupiters” on wildly eccentric orbits (California-Carnegie Planet Search)

What have we learned?: 

What have we learned? Stars with more heavy elements are more likely to host planets (California-Carnegie Planet Search)

What have we learned?: 

What have we learned? Some planets likely have right conditions for liquid water (it’s 300K in here!)

Habitable zone for life: 

Habitable zone for life Darren Williams, Penn State Erie

Habitable zone for life: 

Habitable zone for life Darren Williams, Penn State Erie

Future: search for earthlike planets and life: 

Future: search for earthlike planets and life Kepler: 2008 launch scheduled Search method: transits European Corot mission may scoop US. Terrestrial Planet Finder: 2015 or later Atmospheric Spectroscopy

Additional Credits and Information: 

Additional Credits and Information Credits: Water on Mars: antwrp.gsfc.nasa.gov/apod/ - Astronomy Picture of the Day Sahara Desert and Mars: Lunar and Planetary Institute “Hubble detects a transiting planet” and Beta Pictoris images: Space Telescope Science Institute Black hole embedding diagram: Scott Hughes, MIT Figures showing Mean Orbital Distance created online at http://extrasolar.net/charts.asp Kepler and TPF: NASA/Jet Propulsion Laboratory Books: Origins: Fourteen Billion Years of Cosmic Evolution, Neil deGrasse Tyson and Donald Goldsmith Earth: An Intimate History, Richard Fortey The Ancestor’s Tale: A Pilgrimage to the Dawn of Evolution, Richard Dawkins

Websites for more information: 

Websites for more information Extrasolar.net – General information about exoplanets Exoplanets.org – California-Carnegie exoplanet searches www.astrobio.net - Astrobiology Solstation.com – General astronomy information, sky maps antwrp.gsfc.nasa.gov/apod/ - Astronomy Picture of the Day