EPJ Web of Conferences
Volume 11, 2011Detection and Dynamics of Transiting Exoplanets
|Number of page(s)||3|
|Section||Session 4: Planetary formation and migration|
|Published online||16 February 2011|
Towards the Rosetta Stone of planet formation
Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
2 Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, 85741 Garching, Germany
3 Institut für Physik, Univ. Rostock, D-18051 Rostock, Germany
Transiting exoplanets (TEPs) observed just ~10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (planet formation would then be possible within 10 Myrs), the radius of the planet could indicate whether planets form by gravitational collapse (being larger when young) or accretion growth (being smaller when young). We present a survey, the main goal of which is to ﬁnd and then characterise TEPs in very young open clusters.
© Owned by the authors, published by EDP Sciences, 2011
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