A hot Jupiter orbiting a 2-million-year-old solar-mass T Tauri star

J. F. Donati (), C. Moutou, L. Malo, C. Baruteau, L. Yu, E. Hébrard, G. Hussain, S. Alencar, F. Ménard, J. Bouvier, P. Petit, M. Takami, R. Doyon and A. Collier Cameron
Additional contact information
J. F. Donati: Université de Toulouse, UPS-OMP, IRAP
C. Moutou: Canada–France–Hawaii Telescope (CFHT) Corporation, 65-1238 Mamalahoa Highway
L. Malo: Canada–France–Hawaii Telescope (CFHT) Corporation, 65-1238 Mamalahoa Highway
C. Baruteau: Université de Toulouse, UPS-OMP, IRAP
L. Yu: Université de Toulouse, UPS-OMP, IRAP
E. Hébrard: York University
G. Hussain: European Southern Observatory (ESO), Karl-Schwarzschild-Strasse 2
S. Alencar: ICEx, UFMG
F. Ménard: Université Grenoble Alpes, IPAG, BP 53
J. Bouvier: Université Grenoble Alpes, IPAG, BP 53
P. Petit: Université de Toulouse, UPS-OMP, IRAP
M. Takami: Institute of Astronomy and Astrophysics, Academia Sinica
R. Doyon: Départment de physique, Université de Montréal, CP 6128, Succursale Centre-Ville
A. Collier Cameron: SUPA, School of Physics and Astronomy, University of St Andrews

Nature, 2016, vol. 534, issue 7609, 662-666

Abstract: The radial velocities of a young star are measured, revealing the presence of a planet of mass about three-quarters that of Jupiter, orbiting its host star very closely, and thus demonstrating that ‘hot Jupiters’ can migrate inwards in less than two million years.

Date: 2016
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DOI: 10.1038/nature18305

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