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

Lister, T. A. and Anderson, D. R. and Gillon, M. and Hebb, L. and Smalley, B. S. and Triaud, A. H. M. J. and Collier Cameron, A. and Wilson, D. M. and West, R. G. and Bentley, S. J. and Christian, D. J. and Enoch, R. and Haswell, C. A. and Hellier, C. and Horne, K. and Irwin, J. and Joshi, Y. C. and Kane, S. R. and Mayor, M. and Maxted, P. F. L. and Norton, A. J. and Parley, N. and Pepe, F. and Pollacco, D. and Queloz, D. and Ryans, R. and Segransan, D. and Skillen, I. and Street, R. A. and Todd, I. and Udry, S. and Wheatley, P. J. (2009) WASP-16b: A New Jupiter-Like Planet Transiting a Southern Solar Analog. Astrophysical Journal, 703 (1). pp. 752-756. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20090929-112118363

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Abstract

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 (τ = 2.3^(+5.8)_(–2.2) Gyr).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/703/1/752DOIArticle
http://www.iop.org/EJ/abstract/0004-637X/703/1/752/PublisherArticle
ORCID:
AuthorORCID
Gillon, M.0000-0003-1462-7739
Hebb, L.0000-0003-1263-8637
Triaud, A. H. M. J.0000-0002-5510-8751
Collier Cameron, A.0000-0002-8863-7828
Wilson, D. M.0000-0001-6002-423X
Kane, S. R.0000-0002-7084-0529
Queloz, D.0000-0002-3012-0316
Street, R. A.0000-0001-6279-0552
Wheatley, P. J.0000-0003-1452-2240
Additional Information:© 2009 American Astronomical Society. Print publication: Issue 1 (2009 September 20); received 2009 April 24; accepted for publication 2009 August 4; published 2009 September 1. The WASP Consortium comprises the Universities of Keele, Leicester, St. Andrews, the Queen’s University Belfast, the Open University, and the Isaac Newton Group. WASP-South is hosted by the South African Astronomical Observatory, and we are grateful for their support and assistance. Funding for WASP comes from the consortium universities and from the UK’s Science and Technology Facilities Council. Facilities: Euler1.2m, ESO:3.6m
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
University of KeeleUNSPECIFIED
University of LeicesterUNSPECIFIED
University of St. AndrewsUNSPECIFIED
Queen's University BelfastUNSPECIFIED
Open UniversityUNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Subject Keywords:planetary systems; stars: abundances; stars: individual (WASP-16b)
Issue or Number:1
Record Number:CaltechAUTHORS:20090929-112118363
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20090929-112118363
Official Citation:WASP-16b: A New Jupiter-Like Planet Transiting a Southern Solar Analog T. A. Lister, D. R. Anderson, M. Gillon, L. Hebb, B. S. Smalley, A. H. M. J. Triaud, A. Collier Cameron, D. M. Wilson, R. G. West, S. J. Bentley, D. J. Christian, R. Enoch, C. A. Haswell, C. Hellier, K. Horne, J. Irwin, Y. C. Joshi, S. R. Kane, M. Mayor, P. F. L. Maxted, A. J. Norton, N. Parley, F. Pepe, D. Pollacco, D. Queloz, R. Ryans, D. Segransan, I. Skillen, R. A. Street, I. Todd, S. Udry, and P. J. Wheatley 2009 ApJ 703 752-756 doi: 10.1088/0004-637X/703/1/752
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:16112
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:02 Oct 2009 21:54
Last Modified:09 Mar 2020 13:19

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