Physics
Scientific paper
Oct 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sci...286...90b&link_type=abstract
Science, Vol. 286, No. 5437, p. 90 - 94
Physics
47
Meteorites: Mars, Meteorites: Ages
Scientific paper
The age of secondary carbonate mineralization in the martian meteorite ALH84001 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 high-graded carbonate (visually estimated as ≡5 percent), whitlockite (trace), and orthopyroxene (≡95 percent). The carbonate formation age is contemporaneous with a period in martian history when the surface is thought to have had flowing water, but also was undergoing heavy bombardment by meteorites. Therefore, this age does not distinguish between aqueous and impact origins for the carbonates.
Borg Lars E.
Connelly James N.
Nyquist Larry E.
Reese Young
Shih Chia-You
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