Eccentricity formation and habitable planets in OGLE-06-109L system

Details Eccentricity formation and habitable planets in OGLE-06-109L system Eccentricity formation and habitable planets in OGLE-06-109L system

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epjwc..1605005w&link_type=abstract

Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on O

Physics

Scientific paper

Recent observation of microlensing technique reveals two giant planets at 2.3 AU and 4.6 AU around the star OGLE-06-109L. We investigate the eccentricity formation of these two planets, and find that planetary scattering or resonance crossing may be the reason for their eccentricity excitation. In the inner region of the system, super-Earth planets may be survival in habitable zone (0.25-0.36 AU).

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