Statistics
Scientific paper
Sep 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ess.....2.1601y&link_type=abstract
American Astronomical Society, ESS meeting #2, #16.01
Statistics
Scientific paper
Exoplanet discoveries can be used to evaluate and develop planet formation theories. I will describe, and critically evaluate, two complementary approaches. The first examines a single mechanism in detail, such as orbital evolution due to secular dynamics or planetesimal formation via streaming instabilities. The effects of that mechanism on exoplanet statistics can be assessed. The second approach is commonly known as planetary population synthesis. It attempts to combine simplified versions of all processes relevant to planet formation and evolution. I will describe how the wealth of planet candidates provided by the Kepler survey can constrain both types of models. Finally, I will provocatively discuss whether a deterministic and/or predictive theory of planet formation is possible, or even necessary.
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