Detectability of Terrestrial Planets in Multi-Planet Systems: Preliminary Report
RAYMOND, Sean N.
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Université Sciences et Technologies - Bordeaux 1 [UB]
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Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Université Sciences et Technologies - Bordeaux 1 [UB]
Language
en
Communication dans un congrès
This item was published in
EAS Publications Series, EAS Publications Series, 2008-08-25, torun. 2010, vol. 42, p. 191-199
English Abstract
We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind ...Read more >
We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind calculations designed to answer this question.Read less <
Origin
Hal imported