Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/12121
Title: WASP-43b: the closest-orbiting hot Jupiter
Authors: Hellier, C.
Anderson, D. R.
Cameron, A. C.
Gillon, M.
Jehin, E.
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.
First Published: Nov-2011
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy & Astrophysics, 2011, 535
Abstract: We report the discovery of WASP-43b, a hot Jupiter transiting a K7V star every 0.81 d. At 0.6-M⊙ the host star has the lowest mass of any star currently known to host 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.
DOI Link: 10.1051/0004-6361/201117081
ISSN: 0004-6361
Links: http://hdl.handle.net/2381/12121
http://www.aanda.org/articles/aa/abs/2011/11/aa17081-11/aa17081-11.html
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2011 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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