An absolute sodium abundance for a cloud-free 'hot Saturn' exoplanet
Abstract
Broad absorption signatures from alkali metals, such as the sodium (Na i) and potassium (K i) resonance doublets, have long been predicted in the optical atmospheric spectra of cloud-free irradiated gas giant exoplanets1,2,3. However, observations have revealed only the narrow cores of these features rather than the full pressure-broadened profiles4,5,6. Cloud and haze opacity at the day–night planetary terminator are considered to be responsible for obscuring the absorption-line wings, which hinders constraints on absolute atmospheric abundances7,8,9. Here we report an optical transmission spectrum for the ‘hot Saturn’ exoplanet WASP-96b obtained with the Very Large Telescope, which exhibits the complete pressure-broadened profile of the sodium absorption feature. The spectrum is in excellent agreement with cloud-free, solar-abundance models assuming chemical equilibrium. We are able to measure a precise, absolute sodium abundance of logεNa = 6.9+0.6−0.4, and use it as a proxy for the planet’s atmospheric metallicity relative to the solar value (Zp/Zʘ = 2.3+8.9−1.7). This result is consistent with the mass–metallicity trend observed for Solar System planets and exoplanets10,11,12.
Citation
Nikolov , N , Sing , D K , Fortney , J J , Goyal , J M , Drummond , B , Evans , T M , Gibson , N P , De Mooj , E J W , Rustamkulov , Z , Wakeford , H R , Smalley , B , Burgasser , A J , Hellier , C , Helling , C , Mayne , N J , Madhusudhan , N , Kataria , T , Baines , J , Carter , A L , Ballester , G E , Barstow , J K , McCleery , J & Spake , J J 2018 , ' An absolute sodium abundance for a cloud-free 'hot Saturn' exoplanet ' , Nature , vol. 557 , no. 7706 , pp. 526-529 . https://doi.org/10.1038/s41586-018-0101-7
Publication
Nature
Status
Peer reviewed
ISSN
0028-0836Type
Journal article
Rights
© 2018 Macmillan Publishers Limited, part of Springer Nature. All rights reserved. This work has been made available online in accordance with the publisher’s policies. This is the author created accepted version manuscript following peer review and as such may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1038/s41586-018-0101-7
Description
The research leading to these results received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement number 336792. A.J.B. is a US/UK Fulbright Scholar. J.M.G. and N.J.M. acknowledge support from a Leverhulme Trust Research Project Grant. J.K.B. is a Royal Astronomical Society Research Fellow.Collections
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