Towards the Rosetta Stone of planet formation
| Autor: | Markus M. Hohle, U. Kramm, M. Moualla, Izabela Spaleniak, T. Pribulla, Ch. Adam, Ch. Ginski, T. Roell, Ronny Errmann, A. Berndt, M. Seeliger, S. Fiedler, Markus Mugrauer, T. Eisenbeiss, C. Marka, T. O. B. Schmidt, Ralph Neuhäuser, Gracjan Maciejewski, L. Trepl, N. Tetzlaff, St. Raetz |
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| Rok vydání: | 2010 |
| Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics QC1-999 FOS: Physical sciences Radius Exoplanet Accretion (astrophysics) Astrobiology Planet Gravitational collapse Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Geology Astrophysics::Galaxy Astrophysics Astrophysics - Earth and Planetary Astrophysics Open cluster |
| Zdroj: | EPJ Web of Conferences, Vol 11, p 04006 (2011) |
| DOI: | 10.48550/arxiv.1010.3118 |
| Popis: | Transiting exoplanets (TEPs) observed just about 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. Comment: Poster contribution to Detection and Dynamics of Transiting Exoplanets (Haute Provence Observatory Colloquium, 23-27 August 2010) |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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