WASP-16b: A New Jupiter-Like Planet Transiting a Southern Solar Analog

We report the discovery from WASP-South of a new Jupiter-like extrasolar planet, WASP-16b, which transits its solar analog host star every 3.12 days. Analysis of the transit photometry and radial velocity spectroscopic data leads to a planet with R p = 1.008 +/- 0.071 R Jup and M p = 0.855 +/- 0.059...

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Published inThe Astrophysical journal Vol. 703; no. 1; pp. 752 - 756
Main Authors Lister, T. A, Anderson, D. R, Gillon, M, Hebb, L, Smalley, B. S, Triaud, A. H. M. J, Collier Cameron, A, Wilson, D. M, West, R. G, Bentley, S. J, Christian, D. J, Enoch, R, Haswell, C. A, Hellier, C, Horne, K, Irwin, J, Joshi, Y. C, Kane, S. R, Mayor, M, Maxted, P. F. L, Norton, A. J, Parley, N, Pepe, F, Pollacco, D, Queloz, D, Ryans, R, Segransan, D, Skillen, I, Street, R. A, Todd, I, Udry, S, Wheatley, P. J
Format Journal Article Web Resource
LanguageEnglish
Published Bristol IOP Publishing 20.09.2009
IOP
University of Chicago Press
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Summary:We report the discovery from WASP-South of a new Jupiter-like extrasolar planet, WASP-16b, which transits its solar analog host star every 3.12 days. Analysis of the transit photometry and radial velocity spectroscopic data leads to a planet with R p = 1.008 +/- 0.071 R Jup and M p = 0.855 +/- 0.059 M Jup, orbiting a host star with R * = 0.946 +/- 0.054 R and M * = 1.022 +/- 0.101 M. Comparison of the high resolution stellar spectrum with synthetic spectra and stellar evolution models indicates the host star is a near-solar metallicity ([Fe/H] =0.01 +/- 0.10) solar analog (T eff = 5700 +/- 150 K and log g = 4.5 +/- 0.2) of intermediate age ( Delta *t = 2.3+5.8 -2.2 Gyr).
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
scopus-id:2-s2.0-70549111248
ISSN:0004-637X
1538-4357
1538-4357
DOI:10.1088/0004-637X/703/1/752