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NUMBER 19 109<br />
FIGURE 5.—Coarse silicate texture, inclusion 8: a, transmitted light (black areas are graphite),<br />
note graphite "nibbling" at silicate grains; b, reflected light, crossed polarizers.<br />
quently of the silicates is rather constant. It is<br />
interesting that the amount of silicates in these<br />
three inclusions of 75.9%, 77.3%, and 74.5% is<br />
quite close to the average silicate portion of Hchondrites,<br />
which is 76% (Table 7). The silicate<br />
portion of two of the three inclusions analyzed<br />
chemically is higher, but this does not give the true<br />
silicate amount, as coarse metal particles were<br />
removed prior to analysis.<br />
In addition to the main minerals listed in Tables<br />
1 and 2, the following accessory minerals were<br />
found: schreibersite and cohenite (at the border to<br />
the metal host), apatite, chromite, and sphalerite.<br />
The apatite is a chlorapatite; the microprobe<br />
analysis of 11 grains in different sections gave an<br />
average (in weight percent) of CaO, 52.6; P2O5;<br />
41.1; Cl, 6.00; FeO, 0.30; MgO, 0.11; Na2O, 0.46;<br />
F is not determined, sum 99.2 (corrected for<br />
Cl = 0). This is smiliar to the composition of the<br />
Campo del Cielo apatite published by Bunch, Keil,<br />
and Olsen (1970). The silicates often contain small<br />
inclusions, mostly troilite or metal. Veining with<br />
iron oxides formed by terrestrial weathering is<br />
found in most specimens.<br />
Mineral Composition<br />
In Table 2 the orthopyroxene, olivine, diopside,<br />
plagioclase, and K-feldspar compositions are given<br />
for one inclusion as determined by standard procedures<br />
with an ARL SEMQ microprobe. The<br />
results were corrected by the method of Bence and<br />
Albee (1968). During the study of these inclusions<br />
it was found that small differences in the Fe/