Volume 547, November 2012
|Number of page(s)||8|
|Section||Planets and planetary systems|
|Published online||22 October 2012|
Hint of a transiting extended atmosphere on 55 Cancri b⋆
Observatoire astronomique de l’Université de Genève,
2 UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), UMR 5274, Grenoble, France
3 Institut d’astrophysique de Paris, Université Pierre & Marie Curie, CNRS (UMR 7095), Paris, France
4 Observatoire de Haute-Provence, CNRS (USR 2217), Saint-Michel-l’Observatoire, France
5 Astrophysics Group, School of Physics, University of Exeter, Exeter, UK
6 Department of Physics, University of Warwick, Coventry, UK
7 Laboratoire d’astrophysique de Marseille, Université de Provence, CNRS (UMR 6110), Marseille, France
Received: 10 July 2012
Accepted: 28 September 2012
The naked-eye star 55 Cancri hosts a planetary system with five known planets, including a hot super-Earth (55 Cnc e) extremely close to its star and a farther out giant planet (55 Cnc b), found in milder irradiation conditions with respect to other known hot Jupiters. This system raises important questions on the evolution of atmospheres for close-in exoplanets, and the dependence with planetary mass and irradiation. These questions can be addressed by Lyman-α transit observations of the extended hydrogen planetary atmospheres, complemented by contemporaneous measurements of the stellar X-ray flux. In fact, planet “e” has been detected in transit, suggesting the system is seen nearly edge-on. Yet, planet “b” has not been observed in transit so far. Here, we report on Hubble Space Telescope STIS Lyα and Chandra ACIS-S X-ray observations of 55 Cnc. These simultaneous observations cover two transits of 55 Cnc e and two inferior conjunctions of 55 Cnc b. They reveal the star as a bright Lyα target and a variable X-ray source. While no significant signal is detected during the transits of 55 Cnc e, we detect a surprising Lyα absorption of 7.5 ± 1.8% (4.2σ) at inferior conjunctions of 55 Cnc b. The absorption is only detected over the range of Doppler velocities where the stellar radiation repels hydrogen atoms towards the observer. We calculate a false-alarm probability of 4.4%, which takes the a-priori unknown transit parameters into account. This result suggests the possibility that 55 Cnc b has an extended upper H i atmosphere, which undergoes partial transits when the planet grazes the stellar disc. If confirmed, it would show that planets cooler than hot Jupiters can also have extended atmospheres.
Key words: planetary systems / planets and satellites: atmospheres / stars: individual: 55 Cancri / techniques: spectroscopic
Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with GO/DD programme #12681.
© ESO, 2012
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