Fact sheet
12015 is an olivine vitrophyre with skeletal and dendritic olivine and pyroxene phenocrysts. Microphenocrysts of chromite are also an early phase. These phenocrysts are set in a nearly opaque fine-grained matrix of dendritic pyroxene, plagioclase, filamental ilmenite, chromite, cristobalite, troilite, metallic iron and glass. The bulk composition of 12015 (and 12009) is thought to represent the original magma composition of Apollo 12 mare basalts.
The sample weighed 191.2 grams before analysis. It has not been dated.
Further details of this and other Apollo samples are here: http://curator.jsc.nasa.gov/lunar/
Apollo 12 returned 34 kilograms of samples, including 45 rocks, samples of lunar 'soil', and several core tubes that included material from as much as 40 centimetres below the lunar surface.
Apollo 12 rocks were almost all basalts, with only two breccias in the returned samples. The basalts at the Apollo 12 site formed 3.1 to 3.3 billion years ago, roughly 500 million years later than the Apollo 11 basalts. Overall, there is much less of the element titanium in the Apollo 12 samples than in the Apollo 11 samples, which explains the more reddish colour of this region. The differences in age and chemical composition between the Apollo 11 and Apollo 12 samples demonstrate that mare volcanism did not occur as a single, Moon-wide melting event.
Apollo 12 was launched on 14 November 1969.