Papers presented at the sessions.
Inferences From the Optical Properties of the Moon Concerning the Nature and Evolution of the Lunar Surface
Article first published online: 7 DEC 2012
Copyright 1970 by the American Geophysical Union.
Volume 5, Issue 2, pages 293–299, February 1970
How to Cite
1970), Inferences From the Optical Properties of the Moon Concerning the Nature and Evolution of the Lunar Surface, Radio Sci., 5(2), 293–299, doi:10.1029/RS005i002p00293.(
- Issue published online: 7 DEC 2012
- Article first published online: 7 DEC 2012
- Manuscript Received: 9 SEP 1969
The unusual optical properties of the moon are summarized. They imply that the fine-grained, compressible material observed by the Surveyor television cameras is representative of the entire lunar surface and very probably of the surfaces of Mercury, Mars, and the asteroids also. The soil is the result of repeated meteorite impacts and is not an ash flow. Evidence for darkening is examined, and it is concluded that a process is acting on the lunar surface to alter the albedo and color of the rock powder. Materials of chondritic or granitic composition are not prevalent on the moon. Differences in the optical properties of the maria and the highlands imply that the soil cover is thicker in the highlands than in the maria and that the high-land soils are laterally more homogeneous than are those of the maria.