ADSORPTIVE MECHANISM FOR LOSS OF THE MOON'S ATMOSPHERE,

Abstract

The thermal dissipation of gases cannot explain the practically complete absence of an atmosphere on the Moon. Therefore other mechanisms are invoked to account for it: the ionizing action of the solar ultraviolet radiation; energy transfer to lunar surface molecules from particles of the solar corpuscular radiation (solar wind); the formation, at a certain height above the lunar surface, of an ionized layer similar to the terrestrial exosphere, with a temperature of 1000-1500C. It seems that to explain the absence of an atmosphere on the Moon one must take into account the process of gas adsorption by the lunar surface. The adsorptive powers of the lunar surface must be considerable, because of its high porosity.

Document Details

Document Type
Technical Report
Publication Date
May 01, 1969
Accession Number
AD0689798

Entities

People

  • A. M. Gutkin
  • M. S. Markov
  • M. V. Slonimskaya
  • Ts. M. Raitburd

Tags

Communities of Interest

  • Materials and Manufacturing Processes

DTIC Thesaurus Topics

  • Atmospheres
  • Corpuscular Radiation
  • Electromagnetic Radiation
  • Energy Transfer
  • Radiation
  • Solar Ultraviolet Radiation
  • Solar Wind
  • Ultraviolet Radiation

Fields of Study

  • Physics

Readers

  • Electrochemical Engineering/ Fuel Cell Technologies
  • Plasma Physics / Magnetohydrodynamics
  • Space Exploration and Orbital Mechanics.

Technology Areas

  • Space
  • Space - Hall-Effect Thruster
  • Space - Orbital Debris