ExoMol line lists - XXXVIII. High-temperature molecular line list of silicon dioxide (SiO2)
Abstract
Silicon dioxide (SiO2) is expected to occur in the atmospheres of hot rocky super-Earth exoplanets but a lack of spectroscopic data is hampering its possible detection. Here, we present the first, comprehensive molecular line list for SiO2. The line list, named OYT3, covers the wavenumber range 0 - 6000 cm-1 (wavelengths λ > 1.67 μm) and is suitable for temperatures up to T = 3000 K. Almost 33 billion transitions involving 5.69 million rotation-vibration states with rotational excitation up to J = 255 have been computed using robust first-principles methodologies. The OYT3 line list is available from the ExoMol data base at www.exomol.com.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2020
- DOI:
- 10.1093/mnras/staa1287
- arXiv:
- arXiv:2005.13586
- Bibcode:
- 2020MNRAS.495.1927O
- Keywords:
-
- molecular data;
- opacity;
- planets and satellites: atmospheres;
- stars: atmospheres;
- ISM: molecules;
- Astrophysics - Earth and Planetary Astrophysics;
- Physics - Chemical Physics
- E-Print:
- doi:10.1093/mnras/staa1287