Lunar Transient Phenomena (LTP) have been reported for at least 450 years.
The events range from bright flashes, to reddish or bluish glows, to obscur
ations. Gaseous spectra and photometric measurements of the events have bee
n obtained. Several theories have been offered as explanations for LTP, inc
luding residual volcanic activity or outgassing, bombardment by energetic p
articles, and piezoelectric effects. As the first set of digital multispect
ral images of the entire Moon, the Clementine data offer a unique opportuni
ty to couple inferences of compositional relationships with lunar geomorpho
logy in the regions of LTP. We have selected 11 regions from which numerous
reliable historical reports of LTP exist. Our analysis of the Clementine m
ultispectral images shows that many events occur in regions of bright, spec
trally reddish deposits, which may be characteristic of volcanic ejecta. Th
e events may be associated with outgassing of volatiles collected in or ben
eath mare basalt flows, We find that LTP tend to occur near the edges of ma
ria, in agreement with a suggestion originally made by Cameron (1972, Icaru
s 16, 339-387), and in other regions of crustal weakness. We also find that
some of the reported events tend to be in craters with rims of distinctly
different (bluer) composition. This compositional difference may result fro
m recent slumping of the rim, accompanied by the appearance of fresher unde
rlying material. In some cases, slumping may be triggered by the release of
pockets of volatiles; in turn the slumping events may cause additional poc
kets of trapped material to be released.
There are four instances in which Clementine multispectral images were acqu
ired both before and after an event that was reported by a terrestrial team
of amateur astronomers mobilized to observe the Moon during the mapping ph
ase of Clementine. None of these four sets of images shows clear changes th
at could be attributed to the reported LTP. (C) 2000 Academic Press.