Kepler Super-Earths And Constraints To The High-density Limit On Radius

Details Kepler Super-Earths And Constraints To The High-density Limit On Radius Kepler Super-Earths And Constraints To The High-density Limit On Radius

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21840202s&link_type=abstract

American Astronomical Society, AAS Meeting #218, #402.02; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The minimum radius for super-Earths of a given mass could be determined
by planet formation history, high-density mineral phases, and
evaporation. I will discuss theoretical models and constraints imposed
on them by Kepler mission observations.

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