Letter to the editor (Scientific journals)
WASP-43b: The closest-orbiting hot Jupiter
Hellier, Coel; Anderson, D. R.; Collier Cameron, A. et al.
2011In Astronomy and Astrophysics, 535, p. 5
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Keywords :
Astrophysics - Earth and Planetary Astrophysics
Abstract :
[en] We report the discovery of WASP-43b, a hot Jupiter transiting a K7V star every 0.81 d. At 0.6-Msun the host star has the lowest mass of any star hosting a hot Jupiter. It also shows a 15.6-d rotation period. The planet has a mass of 1.8 Mjup, a radius of 0.9 Rjup, and with a semi-major axis of only 0.014 AU has the smallest orbital distance of any known hot Jupiter. The discovery of such a planet around a K7V star shows that planets with apparently short remaining lifetimes owing to tidal decay of the orbit are also found around stars with deep convection zones.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Hellier, Coel
Anderson, D. R.
Collier Cameron, A.
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Jehin, Emmanuel  
Lendl, M.
Maxted, P. F. L.
Pepe, F.
Pollacco, D.
Queloz, D.
Segransan, D.
Smalley, B.
Smith, A. M. S.
Southworth, J.
Triaud, A H M J
Udry, S.
West, R. G.
More authors (7 more) Less
Language :
English
Title :
WASP-43b: The closest-orbiting hot Jupiter
Publication date :
14 November 2011
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
535
Pages :
5
Peer reviewed :
Peer Reviewed verified by ORBi
Commentary :
4 pages
Available on ORBi :
since 11 July 2011

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