Published December 22, 1972 | Version public
Journal Article

Is the Moon Hot or Cold?

Abstract

Baldwin (1) has summarized some of the evidence for the early and present internal thermal states of the moon. He argued that the interior of the moon, below about 200 to 300 kilometers, is presently "hot," that is, has interior temperatures close to or exceeding the lunar solidus curve. The evidence for a rapid differentiation of the moon about 4.6 X 10^9 on years ago, the extensive igneous episode resulting in mare formation 3.7 X 10^9 to 2.8 X 10^9 years ago, the depletion of the moon in volatiles and its enrichment in calcium, aluminum, and the trace refractory elements all argue for a hot origin and high initial temperatures. A straightforward consequence of the lunar thermal inertia is that if the interior of the moon were ever hot it would remain hot to the present. The high surface concentrations of uranium, thorium, and potassium, and the Apollo 15 heat flow value of 33 ergs per square centimeter per second (2), indicate high present-day temperatures in the lunar interior (3).

Additional Information

© 1972 American Association for the Advancement of Science. Supported by NASA grant NGL 05-002-069. Contribution No. 2188, Division of Geological and Planetary Sciences, California Institute of Technology.

Additional details

Identifiers

Eprint ID
62054
DOI
10.1126/science.178.4067.1245
Resolver ID
CaltechAUTHORS:20151111-100012443

Related works

Funding

NASA
NGL 05-002-069

Dates

Created
2015-11-11
Created from EPrint's datestamp field
Updated
2021-11-10
Created from EPrint's last_modified field

Caltech Custom Metadata

Other Numbering System Name
Caltech Division of Geological and Planetary Sciences
Other Numbering System Identifier
2188