Towards the Rosetta Stone of planet formation

Towards the Rosetta Stone of planet formation

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)...

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Bibliographic Details
Main Authors: Schmidt T.O.B., Roell T., Raetz St., Pribulla T., Moualla M., Marka C., Kramm U., Hohle M., Ginski Ch., Fiedler S., Eisenbeiss T., Berndt A., Adam Ch., Mugrauer M., Errmann R., Neuhäuser R., Maciejewski G., Seeliger M., Spaleniak I., Tetzlaff N., Trepl L.
Format: Article
Language:English
Published: EDP Sciences 2011-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20101104006

Internet

http://dx.doi.org/10.1051/epjconf/20101104006

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