The age of secondary carbonate mineralization in the martian meteorite ALH8
4001 was determined to be 3.90 +/- 0.04 billion years by rubidium-strontium
(Rb-Sr) dating and 4.04 +/- 0.10 billion years by Lead-Lead (Pb-Pb) dating
. The Rb-Sr and Pb-Pb isochrons are defined by Leachates of a mixture of hi
gh-graded carbonate (visually estimated as similar to 5 percent). whitlocki
te (trace), and orthopyroxene (similar to 95 percent). The carbonate format
ion age is contemporaneous with a period in martian history when the surfac
e is thought to have had flowing water, but also was undergoing heavy bomba
rdment by meteorites. Therefore, this age does not distinguish between aque
ous and impact origins for the carbonates.