Published April 1974
| Version v1
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Regolith history from cosmic-ray-produced isotopes
Description
A statistical model is given for soil development relating meteoroid impacts on the moon to cosmic-ray-produced isotopes in the soil. By means of this model, the average lunar mass loss rate during the past 14 aeons is determined to be 170 g/sq cm aeon and the soil mixing rate to be approximately 200 cm/aeon from the gadolinium isotope data for the Apollo 15 and 16 drill stems. The isotope data also restrict the time variation of the meteoroid flux during the past 14 aeons. (U.S.)
Availability note (English)
MF available from INIS under the Report Number.
Files
Additional details
Additional titles
- Augmented title (English)
- Statistical model
Publishing Information
- Imprint Pagination
- 16 p.
- Report number
- N--74-26277
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6205821
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; GADOLINIUM; ISOTOPES; LOSSES; MASS; METEOROIDS; MOON; SOILS; STATISTICS; TIME DEPENDENCE
- Descriptors DEC
- ELEMENTS; IONIZING RADIATIONS; MATHEMATICS; METALS; RADIATIONS; RARE EARTHS; SATELLITES
Optional Information
- Secondary number(s)
- NASA-CR--134261; SAO--404-069.