Lunar science: An overview

Autor: Stuart Ross Taylor
Rok vydání: 2005
Předmět:
Zdroj: Journal of Earth System Science. 114:587-591
ISSN: 0973-774X
0253-4126
DOI: 10.1007/bf02715941
Popis: Before spacecraft exploration, facts about the Moon were restricted to information about the lunar orbit, angular momentum and density. Speculations about composition and origin were unconstrained. Naked eye and telescope observations revealed two major terrains, the old heavily cratered highlands and the younger mostly circular, lightly cratered maria. The lunar highlands were thought to be composed of granite or covered with volcanic ash-flows. The maria were thought to be sediments, or were full of dust, and possibly only a few million years old. A few perceptive observers such as Ralph Baldwin (Baldwin 1949) concluded that the maria were filled with volcanic lavas, but the absence of terrestrial-type central volcanoes like Hawaii was a puzzle.
Databáze: OpenAIRE