Ab. Verchovsky et al., C, N, AND NOBLE-GAS ISOTOPES IN GRAIN-SIZE SEPARATES OF PRESOLAR DIAMONDS FROM EFREMOVKA, Science, 281(5380), 1998, pp. 1165-1168
Nanometer-size presolar diamonds from the Efremovka CV3 chondrite were
physically separated into several grain size fractions by uttracentri
fugation. The coarsest size fraction is the most enriched in carbon-12
; the others have broadly similar carbon isotopic compositions. Measur
ement of noble gases shows that their concentration decreases with dec
reasing grain size. This effect is attributed to ion implantation, Suc
h an episode could occur in the envelope of a supernova that produced
the diamonds, or in interstellar space; in either case, ions with ener
gies above a certain threshold pass completely through the smaller dia
mond grains without being captured. Concentrations of nitrogen show on
ly minor variations with grain size, indicating a different mechanism
of incorporation into the diamonds.