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A method for the direct determination of the surface gravities of transiting extrasolar planets

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Southworth, J. (John), Wheatley, Peter J. and Sams, Giles. (2007) A method for the direct determination of the surface gravities of transiting extrasolar planets. Monthly Notices of the Royal Astronomical Society, Vol.379 (No.1). L11-L15. ISSN 0035-8711

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Official URL: http://dx.doi.org/10.1111/j.1745-3933.2007.00324.x

Abstract

We show that the surface gravity of a transiting extrasolar planet can be calculated from only the spectroscopic orbit of its parent star and the analysis of its transit light curve. This does not require additional constraints, such as are often inferred from theoretical stellar models or model atmospheres. The surface gravity of the planet can therefore be measured precisely and from only directly observable quantities. We outline the method and apply it to the case of the first known transiting extrasolar planet, HD 209458b. We find a surface gravity of g(p) = 9.28 +/- 0.15 m s(-2), which is an order of magnitude more precise than the best available measurements of its mass, radius and density. This confirms that the planet has a much lower surface gravity than that predicted by published theoretical models of gas giant planets. We apply our method to all 14 known transiting extrasolar planets and find a significant correlation between surface gravity and orbital period, which is related to the known correlation between mass and period. This correlation may be the underlying effect as surface gravity is a fundamental parameter in the evaporation of planetary atmospheres.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Wiley-Blackwell Publishing, Inc
ISSN: 0035-8711
Date: 21 July 2007
Volume: Vol.379
Number: No.1
Number of Pages: 5
Page Range: L11-L15
Identification Number: 10.1111/j.1745-3933.2007.00324.x
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
URI: http://wrap.warwick.ac.uk/id/eprint/31735

Data sourced from Thomson Reuters' Web of Knowledge

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