Measurement of the Spin-Orbit Angle of Exoplanet HAT-P-1b

The Astrophysical Journal (Impact Factor: 6.73). 12/2008; 686(1):649. DOI: 10.1086/591078
Source: arXiv

ABSTRACT We present new spectroscopic and photometric observations of the HAT-P-1 planetary system. Spectra obtained during three transits exhibit the Rossiter-McLaughlin effect, allowing us to measure the angle between the sky projections of the stellar spin axis and orbit normal, λ = 3.7°± 2.1°. The small value of λ for this and other systems suggests that the dominant planet migration mechanism preserves spin-orbit alignment. Using two new transit light curves, we refine the transit ephemeris and reduce the uncertainty in the orbital period by an order of magnitude. We find a upper limit on the orbital eccentricity of 0.067, with 99% confidence, by combining our new radial velocity measurements with those obtained previously.

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    The Astrophysical Journal 11/2008; · 6.73 Impact Factor
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    The Astrophysical Journal 07/2009; · 6.73 Impact Factor


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