Problem of nature of inert gases in lunar surface material

Details Problem of nature of inert gases in lunar surface material Problem of nature of inert gases in lunar surface material

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974lssf.nasa..348l&link_type=abstract

"In its Lunar soil from the Sea of Fertility (NASA-TT-F-15881) p 348-357 (SEE N75-11814 02-91) Transl. into ENGLISH from the bo

Computer Science

Cosmic Gases, Lunar Maria, Lunar Soil, Rare Gases, Argon, Helium, Isotopes, Krypton, Lunar Surface, Lunik 16 Lunar Probe, Neon, Solar Wind, Xenon

Scientific paper

The origin of isotopes of inert gases in lunar surface material was investigated from the standpoint of the isotopic two-component status of inert gases in the solar system. Helium and neon represent the solar wind component, while krypton and xenon are planetary gases. Type A gases are trapped by the material of the regolith in the early stages of the existence of the solar system and were brought to the lunar surface together with dust. The material of the regolith therefore cannot be considered as the product of the erosion of the crystalline rocks of the moon and in this sense are extralunar. The regolith material containing type A gases must be identified with the high temperature minerals of the carbonaceous chondrites.

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