A. Bischoff et al., MINERALOGY, CHEMISTRY, AND NOBLE-GAS CONTENTS OF ADZHI-BOGDO - AN LL3-6 CHONDRITIC BRECCIA WITH L-CHONDRITIC AND GRANITOIDAL CLASTS, Meteoritics, 28(4), 1993, pp. 570-578
Adzhi-Bogdo is an ordinary chondrite regolith breccia (LL3-6) which fe
ll on 1949 October 30 in Gobi Altay, Mongolia. The rock consists of su
bmm- to cm-sized fragments embedded in a fine-grained clastic matrix T
he polymict breccia contains various types of clasts, some of which mu
st be of foreign origin. Components of the breccia include chondrules,
melt rock clasts (some of which are K-rich), highly recrystallized ro
ck fragments (''granulites''), breccia clasts, pyroxene-rich fragments
with achondritic textures, and alkali-granitoids. The composition of
olivine in most fragments is in the range of LL-chondrites. However, o
livine in some components has significantly lower fayalite contents, c
haracteristic of L-chondrites. The bulk meteorite is very weakly shock
ed (S2). Based on the bulk chemical composition, Adzhi-Bogdo is an ord
inary chondrite. The concentrations of Fe and Ni are somewhat intermed
iate between L- and LL-chondrites. The contents of solar gases indicat
e that Adzhi-Bogdo is a regolith breccia. Most of the solar He and pro
bably a part of the solar Ne of Adzhi-Bogdo has been lost. It is sugge
sted that Adzhi-Bogdo experienced an (impact-induced) thermal event ea
rly in its history, because most of the radiogenic Ar-40 is retained.