Tennyson, J;
Yurchenko, SN;
(2017)
Laboratory spectra of hot molecules: Data needs for hot super-Earth exoplanets.
Molecular Astrophysics
, 8
pp. 1-18.
10.1016/j.molap.2017.05.002.
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Abstract
The majority of stars are now thought to support exoplanets. Many of those exoplanets discovered thus far are categorized as rocky objects with an atmosphere. Most of these objects are however hot due to their short orbital period. Models suggest that water is the dominant species in their atmospheres. The hot temperatures are expected to turn these atmospheres into a (high pressure) steam bath containing remains of melted rock. The spectroscopy of these hot rocky objects will be very different from that of cooler objects or hot gas giants. Molecules suggested to be important for the spectroscopy of these objects are reviewed together with the current status of the corresponding spectroscopic data. Perspectives of building a comprehensive database of linelist/cross sections applicable for atmospheric models of rocky super-Earths as part of the ExoMol project are discussed. The quantum-mechanical approaches used in linelist productions and their challenges are summarized.
Type: | Article |
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Title: | Laboratory spectra of hot molecules: Data needs for hot super-Earth exoplanets |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1016/j.molap.2017.05.002 |
Publisher version: | http://dx.doi.org/10.1016/j.molap.2017.05.002 |
Language: | English |
Additional information: | Copyright © 2017 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license. (http://creativecommons.org/licenses/by/4.0/) |
Keywords: | Super-Earth, Lava-planets, Absorption Intensities, FTIR spectroscopy, Line lists, Transit spectroscopy, Exoplanets |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/1557861 |
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