JPL Home NASA Home Caltech Home
Follow this link to skip to the main content
NASA Logo - Jet Propulsion Laboratory   + View the NASA Portal
Search JPL
JPL Home Earth Solar System Stars & Galaxies Technology
Science Visitor and Colloquium Program
SVCP Home
Meetings
Information for Visitors
Contact
Restricted
 
Astrophysics Luncheon Seminar

From the Statistics to the Individual Characterization of Exoplanets
Presented by Jean-Michel Desert
California Institute of Technology

Monday, June 17, 2013
12:00 noon in 169-336

Abstract
The field of exoplanetology has recently transitioned from the investigation of individual objects to statistical studies. In this talk, I discuss both the statistical approach of planetary detection and the individual characterization of their atmospheres. The CoRoT and Kepler space missions have revealed an unprecedented number of small exoplanet candidates. However, a fundamental question remains about the large sample of Kepler candidates: are these objects really bonafide planets? I will discuss methods that we are employing to answer this question. Answers to key questions about exoplanet science come not only from statistics, but also from individual characterization. Studying the atmospheres of exoplanets is the next step in leveraging their detections to further transform our understanding of planetary formation and physics. This is because a planet's atmosphere provides a fossil record of its primordial origins and controls its fate, size and appearance. I present ongoing comparative exoplanetology programs that aim to characterize planetary systems transiting nearby stars through the observations of their atmospheres. I combine ground- and space-based multi-wavelength observations secured over wide spectral regions in order to probe exoplanet atmospheres. These projects provide insights into the formation and evolution of planetary systems and enhance our understanding of our own Solar System's formation. Finally, I also discuss the prospect of probing rocky exoplanet atmospheres orbiting in the habitable zone of their parent stars with future facilities.


SVCP Astrophysics


Privacy / Copyrights
  NASA Home Page
Site Manager:
Webmaster:

CL 08-3220