Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits☆

@article{Vasavada1999NearSurfaceTO,
  title={Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits☆},
  author={A. Vasavada and D. Paige and S. Wood},
  journal={Icarus},
  year={1999},
  volume={141},
  pages={179-193}
}
  • A. Vasavada, D. Paige, S. Wood
  • Published 1999
  • Physics
  • Icarus
  • Abstract In order to assess the thermal stability of polar ice deposits, we present model calculated temperatures of flat surfaces and surfaces within bowl-shaped and flat-floored polar impact craters on Mercury and the Moon. Our model includes appropriate insolation cycles, realistic crater shapes, multiple scattering of sunlight and infrared radiation, and depth- and temperature-dependent regolith thermophysical properties. Unshaded water ice deposits on the surface of either body are rapidly… CONTINUE READING
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    • 65
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    References

    SHOWING 1-10 OF 56 REFERENCES
    The Thermal Stability of Water Ice at the Poles of Mercury
    • 95
    • PDF
    Lunar cold traps and their influence on argon-40
    • 28
    • Highly Influential
    The migration of volatiles on the surfaces of Mercury and the Moon
    • 113
    • Highly Influential
    Thermophysics of the planet Mercury
    • 57