By Lashay Breedlove
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Additional resources for A Comprehensive Book on Lunar Science
1007/s11038-010-9365-0 October 2010). Chapter- 7 Transient Lunar Phenomenon This map, based on a survey of 300 TLPs by Barbara Middlehurst and Patrick Moore, shows the approximate distribution of observed events. Red-hued events are in red; the remainder are in yellow. A transient lunar phenomenon (TLP), or lunar transient phenomenon (LTP), is a short-lived light, color, or change in appearance on the lunar surface. Claims of short-lived phenomena go back at least 1,000 years, with some having been observed independently by multiple witnesses or reputable scientists.
India's Moon Impact Probe and NASA's LCROSS. Impact events leave a visible scar on the surface, and these could be detected by analyzing before and after photos of sufficiently high resolution. No impact craters having formed between the Apollo-era, Clementine (global resolution 100 metre, selected areas 7-20 metre) and SMART-1 (resolution 50 metre) missions have been identified. Electrostatic phenomena Eight individual frames taken from a video of the lunar crater Clavius showing the effect of the Earth's atmosphere on astronomical images It has been suggested that effects related to either electrostatic charging or discharging might be able to account for some of the transient lunar phenomena.
False color image of the Moon taken by the Galileo orbiter showing geological features. NASA photo. The same image in normal color. The geology of the Moon (sometimes called selenology, although the latter term can refer more generally to "lunar science") is quite different from that of the Earth. The Moon lacks a significant atmosphere and any bodies of water, which eliminates erosion due to weather; it does not possess any form of plate tectonics, it has a lower gravity, and because of its small size, it cools more rapidly.
A Comprehensive Book on Lunar Science by Lashay Breedlove