Modeling of the spectral properties of the dwarf planet Makemake

  • T. A. Hromakina
  • L.  V. Starukhina Institute of Astronomy of V.N. Karazin Kharkiv National University
  • I.  N. Belskaya Institute of Astronomy of V.N. Karazin Kharkiv National University
  • V.  V. Korokhin Institute of Astronomy of V.N. Karazin Kharkiv National University
Keywords: small Solar system bodies, planetary surfaces, spectral modeling

Abstract

We present the results of spectral modeling for dwarf planet Makemake in the visible and near infrared ranges. The spectral modeling of surface properties suggests the presence of both large and small (~1 μm) grains of methane ice on the top surface, and possible presence of ethane ice and other long-chain hydrocarbons.

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Published
2015-07-01
How to Cite
Hromakina, T. A., Starukhina, L. V., Belskaya, I. N., & Korokhin, V. V. (2015). Modeling of the spectral properties of the dwarf planet Makemake. Journal of V. N. Karazin Kharkiv National University. Series Physics, 1158(22), 10-12. Retrieved from https://periodicals.karazin.ua/physics/article/view/7792
Section
Articles