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arXiv · 1407.7710

A Spin-Orbit Alignment for the Hot Jupiter HATS-3b

B. C. Addison·C. G. Tinney·D. J. Wright·D. Bayliss
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Abstract

We have measured the alignment between the orbit of HATS-3b (a recently discovered, slightly inflated Hot Jupiter) and the spin-axis of its host star. Data were obtained using the CYCLOPS2 optical-fiber bundle and its simultaneous calibration system feeding the UCLES spectrograph on the Anglo-Australian Telescope. The sky-projected spin-orbit angle of $\lambda = 3\pm25^{\circ}$ was determined from spectroscopic measurements of Rossiter-McLaughlin effect. This is the first exoplanet discovered through the HATSouth transit survey to have its spin-orbit angle measured. Our results indicate that the orbital plane of HATS-3b is consistent with being aligned to the spin axis of its host star. The low obliquity of the HATS-3 system, which has a relatively hot mid F-type host star, agrees with the general trend observed for Hot Jupiter host stars with effective temperatures $>6250$K to have randomly distributed spin-orbit angles.

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B. C. Addison, C. G. Tinney, D. J. Wright, D. Bayliss. 2014-07-29. A Spin-Orbit Alignment for the Hot Jupiter HATS-3b. https://doi.org/10.1088/0004-637x/792/2/112

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