Alan T. Waterman Lecture May 12, 2009, 11:00 am NSF Room 110
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Alan T. Waterman Lecture Alan T. Waterman Lecture May 12, 2009, 11:00 am May 12, 2009, 11:00 am NSF Room 110 NSF Room 110 DAVID B. CHARBONNEAU DAVID B. CHARBONNEAU 2009 Alan T. Waterman Award 2009 Alan T. Waterman Award winner winner How to Find a Habitable Exoplanet When exoplanets eclipse their parent stars, we are granted direct estimates of their masses and physical sizes and we can study their atmospheres. Such systems have profoundly impacted our understanding of giant exoplanets akin to Jupiter, yet no eclipsing examples of rocky exoplanets have yet been found. By targeting nearby low-mass stars, a survey using humble telescopes is capable of discovering rocky planets orbiting at the distance required to permit liquid water on their surfaces. The discovery of such planets would provide fundamental constraints on the physical structure of planets that are primarily rock and ice in Sponsored by MPS and OIA
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Alan T. Waterman Lecture May 12, 2009, 11:00 am NSF Room 110. How to Find a Habitable Exoplanet - PowerPoint PPT Presentation
Transcript of Alan T. Waterman Lecture May 12, 2009, 11:00 am NSF Room 110
Alan T. Waterman LectureAlan T. Waterman LectureMay 12, 2009, 11:00 amMay 12, 2009, 11:00 am
NSF Room 110NSF Room 110
DAVID B. CHARBONNEAUDAVID B. CHARBONNEAU2009 Alan T. Waterman Award winner2009 Alan T. Waterman Award winner
How to Find a Habitable Exoplanet
When exoplanets eclipse their parent stars, we are granted direct estimates of their masses and physical sizes and we can study their atmospheres. Such systems have profoundly impacted our understanding of giant exoplanets akin to Jupiter, yet no eclipsing examples of rocky exoplanets have yet been found. By targeting nearby low-mass stars, a survey using humble telescopes is capable of discovering rocky planets orbiting at the distance required to permit liquid water on their surfaces. The discovery of such planets would provide fundamental constraints on the physical structure of planets that are primarily rock and ice in composition. Moreover, we can study the atmospheric chemistry of these potentially habitable worlds, and ultimately search for biomarkers indicating life.
Sponsored by MPS and OIA
