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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/

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