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 in | The Astrophysical journal Vol. 703; no. 1; pp. 752 - 756 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article Web Resource |
Language | English |
Published |
Bristol
IOP Publishing
20.09.2009
IOP University of Chicago Press |
Subjects | |
Online Access | Get full text |
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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). |
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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 |