Published September 20, 2009 | Version Published
Journal Article Open

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

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).

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

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Additional details

Identifiers

Eprint ID
16112
Resolver ID
CaltechAUTHORS:20090929-112118363

Funding

University of Keele
University of Leicester
University of St. Andrews
Queen's University Belfast
Open University
Science and Technology Facilities Council (STFC)

Dates

Created
2009-10-02
Created from EPrint's datestamp field
Updated
2021-11-08
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Infrared Processing and Analysis Center (IPAC)