DAViNCI 1 M.Shao, B. M.Levine, G. Vasisht, C. Zhai, J. Sandhu JPL, B. F. Lane, Draper Labs, R. Woodruff, G. Vasudevan, Lockheed-Martin, R. Samuele, Northop.
Barcelona, September 14, 20091 SCIENTIFIC OUTPUT OF SINGLE APERTURE IMAGING OF EXOPLANETS Raffaele Gratton, INAF-OAPD, I Anthony Boccaletti, LESIA-OAPM,
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Planet detection and characterization through high contrast imaging Raffaele Gratton INAF – Osservatorio Astronomico di Padova La ricerca sui pianeti extrasolari.
2nd Midterm: Mean: 85 St.Dev: 11 For help: For help: See GSI or Prof. Manga or Prof. Marcy.
First direct image of extrasolar planets. 10.7 billion miles.
2nd Midterm: Difficult Exam... Common Mistakes 1. Greenhouse Effect: CO2 absorbs IR light (not UV). 2. Geological activity on Jupiter’s moons is due to.
Properties of Extrasolar Planets Roman Rafikov (Institute for Advanced Study) Methods of detection Characterization Theoretical ideas Future prospects.
EXTRASOLAR PLANETARY SYSTEMS DETECTION METHODS, RESULTS AND PERSPECTIVES MICHAŁ RÓŻYCZKA
Diversity of Data in the Search for Exoplanets Rachel Akeson NASA Exoplanet Science Institute
The Small Star Opportunity to Find and Characterize Habitable Planets
Progress of LiJET and transit search with Lijiang 2.4m telescope
