Published January 16, 2021 | Version v1

Exoplanet Aerosol Transmission Spectra

  • 1. University of California, Santa Cruz
  • 2. University of Bristol
  • 3. Johns Hopkins University
  • 4. University of Oxford

Description

Aerosol transmission spectra for a variety of proposed cloud and haze species computed assuming monodisperse 0.1 micron particles distributed with a constant mass mixing ratio profile in the atmosphere. The first column is wavelength in microns, the second is planet radius in km, and third column is atmospheric molecular weight. Optical constants for tholins are taken from Khare et al. (1984); those for soots are from Lavvas and Koskinen (2017); those for KCl, ZnS, Na2S, MnS, and Cr are from Morley et al. (2012); those for NaCl are from Eldridge and Palik (1985) and Querry (1987); those for Mg2SiO4, Fe, and Al2O3 are from Wakeford and Sing (2015); and those for TiO2 are from Posch et al. (2003) and Zeidler et al. (2011).

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Additional details

References

  • Khare, B. N., Sagan, C., Arakawa, K. T., Suits, F., Callcott, T. A., & Williams, M. W. (1984) Optical constants of organic tholins produced in a simulated titanian atmosphere: From soft x-ray to microwave frequencies. Icarus, 60, 127–137.
  • Lavvas, P., & Koskinen, T. (2017) Aerosol Properties of the Atmospheres of Extrasolar Giant Planets. The Astrophysical Journal, 847, 32.
  • Morley, C. V., Fortney, J. J., Marley, M. S., Visscher, C., Saumon, D., & Leggett, S. K. (2012) Neglected Clouds in T and Y Dwarf Atmospheres. The Astrophysical Journal, 756 (2), 172.
  • Eldridge, J., & Palik, E. D. (1985) Sodium chloride (nacl). In E. D. Palik (Ed.), Handbook of optical constants of solids (p. 775 - 793). Boston: Academic Press.
  • Querry, M. R. (1987) Optical constants of minerals and other materials from the millimeter to the ultraviolet. U.S. Army Armament, Munitions Chemical Research, Dover, New Jersey, USA.
  • Wakeford, H. R., & Sing, D. K. (2015) Transmission spectral properties of clouds for hot Jupiter exoplanets. Astronomy & Astrophysics, 573, A122.
  • Posch, T., Kerschbaum, F., Fabian, D., Mutschke, H., Dorschner, J., Tamanai, A., & Henning, T. (2003) Infrared Properties of Solid Titanium Oxides: Exploring Potential Primary Dust Condensates. The Astrophysical Journal Supplement Series, 149 (2), 437-445.
  • Zeidler, S., Posch, T., Mutschke, H., Richter, H., & Wehrhan, O. (2011) Near-infrared absorption properties of oxygen-rich stardust analogs. The influence of coloring metal ions. Astronomy & Astrophysics, 526, A68.