Diurnal Temperature Regime in the Regolith Surface Layer of the Lagado Planitia Region on Phobos: Model Predictions for Different Seasons


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The paper contains the data on the thermal and physical characteristic of the surface regolith of the Martian satellite Phobos obtained from the spaceborne remote sensing (with the Mariner 9, Viking, and Mars Global Surveyor orbiters and the Phobos-2 spacecraft) and the results of the numerical modeling of the thermal regime in the surface regolith (on diurnal and seasonal scales) performed for the prospective landing site in the Lagado Planitia region located in the anti-Martian hemisphere of Phobos.

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R. Kuzmin

Vernadsky Institute of Geochemistry and Analytical Chemistry; Space Research Institute

编辑信件的主要联系方式.
Email: rok@geokhi.ru
俄罗斯联邦, Moscow, 119991; Moscow, 117997

E. Zabalueva

Vernadsky Institute of Geochemistry and Analytical Chemistry

Email: rok@geokhi.ru
俄罗斯联邦, Moscow, 119991

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