An ultrahot gas-giant exoplanet with a stratosphere

作者:Evans, Thomas M.*; Sing, David K.; Kataria, Tiffany; Oyal, Jayesh G.; Nikolov, Nikolay; Wakeford, Hannah R.; Deming, Drake; Marley, Mark S.; Amundsen, David S.; Ballester, Gilda E.; Barstow, Joanna K.; Ben-Jaffel, Lotfi; Bourrier, Vincent; Buchhave, Lars A.; Cohen, Ofer; Ehrenreich, David; Munoz, Antonio Garcia; Henry, Gregory W.; Knutson, Heather; Lavvas, Panayotis; des Etangs, Alain Lecavelier; Lewis, Nikole K.; Lopez-Morales, Mercedes; Mandell, Avi M.; Sanz-Forcada, Jorge
来源:Nature, 2017, 548(7665): 58-+.
DOI:10.1038/nature23266

摘要

Infrared radiation emitted from a planet contains information about the chemical composition and vertical temperature profile of its atmosphere(1-3). If upper layers are cooler than lower layers, molecular gases will produce absorption features in the planetary thermal spectrum(4,5). Conversely, if there is a stratosphere-where temperature increases with altitude-these molecular features will be observed in emission(6-8). It has been suggested that stratospheres could form in highly irradiated exoplanets(9,10), but the extent to which this occurs is unresolved both theoretically(11,12) and observationally(3,13-15). A previous claim for the presence of a stratosphere(14) remains open to question, owing to the challenges posed by the highly variable host star and the low spectral resolution of the measurements(3). Here we report a near-infrared thermal spectrum for the ultrahot gas giant WASP-121b, which has an equilibrium temperature of approximately 2,500 kelvin. Water is resolved in emission, providing a detection of an exoplanet stratosphere at 5 sigma confidence. These observations imply that a substantial fraction of incident stellar radiation is retained at high altitudes in the atmosphere, possibly by absorbing chemical species such as gaseous vanadium oxide and titanium oxide.

  • 出版日期2017-8-3
  • 单位中国地震局