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Published January 1, 2009 | Published
Journal Article Open

Wasp-7: A Bright Transiting-Exoplanet System in the Southern Hemisphere

Abstract

We report that a Jupiter-mass planet, WASP-7b, transits the V = 9.5 star HD 197286 every 4.95 d. This is the brightest discovery from the WASP-South transit survey so far and is currently the brightest transiting-exoplanet system in the southern hemisphere. WASP-7b is among the densest of the known Jupiter-mass planets, suggesting that it has a massive core. The planet mass is 0.96+0.12 –0.18 M Jup, the radius is 0.915+0.046 –0.040 R Jup, and the density is 1.26+0.25 –0.21 ρJup (1.67+0.33 –0.28 g cm^–3).

Additional Information

© 2009 The American Astronomical Society. Received 2008 May 17, accepted for publication 2008 November 17. Published 2008 December 11. Print publication: Issue 1 (2009 January 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 consortium universities and from the UK's Science and Technology Facilities Council.

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