Journal
ASTRONOMY & ASTROPHYSICS
Volume 527, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201016331
Keywords
planets and satellites: dynamical evolution and stability; techniques: radial velocities; planetary systems; stars: individual: HAT-P-6
Categories
Funding
- CNRS/INSU
- Swiss National Science Foundation
- French National Research Agency [ANR-08-JCJC-0102-01, ANR-NT05-4-44463]
- CNES
- European Research Council/European Community [239953]
- Fundacao para a Ciencia e a Tecnologia (FCT)
- FCT/MCTES (Portugal) [PTDC/CTE-AST/66643/2006, PTDC/CTE-AST/098528/2008]
- Fundação para a Ciência e a Tecnologia [PTDC/CTE-AST/66643/2006] Funding Source: FCT
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We observed the transit of the HAT-P-6b exoplanet across its host star with the SOPHIE spectrograph (OHP, France). The resulting stellar radial velocities display the Rossiter-McLaughlin anomaly and reveal a retrograde orbit: the planetary orbital spin and the stellar rotational spin point in approximately opposite directions. A fit to the anomaly measures a sky-projected angle lambda = 166 degrees +/- 10 degrees between these two spin axes. All seven known retrograde planets are hot Jupiters with masses M-p < 3 M-Jup. About two thirds of the planets in this mass range, however, are prograde and aligned (lambda similar or equal to 0 degrees). In contrast, most of the more massive planets (M-p > 4 M-Jup) are prograde but misaligned. Different mechanisms may therefore be responsible for planetary obliquities above and below similar to 3.5 M-Jup.
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