Statistical properties of exoplanets: an update from recent results

Details Statistical properties of exoplanets: an update from recent results Statistical properties of exoplanets: an update from recent results

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.confr..29p&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

Astronomy and Astrophysics

Astronomy

Scientific paper

The most recent data for extra-solar planets are used in order to examine the diagrams correlating several of their basic parameters, e.g. mass, period, semi-major axis, orbital eccentricity and metallicity. Interesting conclusions are emerging such as the lack of light planets (M_pl < 0.15 M_jup) with semi-major axis of their orbit greater than 1.5 A.U. Monte Carlo simulations are used in order to reproduce the same results.

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