[meteorite-list] Tschermak and Chladnites
From: bernd.pauli_at_paulinet.de <bernd.pauli_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:13 2004 Message-ID: <DIIE.0000003A00001E42_at_paulinet.de> TSCHERMAK G. (1885) Die mikroskopische Beschaffenheit der Meteoriten (Stuttgart E. Schweizerbart'sche Verlagshandlung, E. Koch, 23 pp.). English Translation: The Microscopic Properties of Meteorites, Vol. 4, No. 6 (Smithsonian Contributions to Astrophysics, Washington, D.C., 1964). Translation by J.A. Wood and E.M. Wood Chladnites This combination of minerals has been found in only one meteorite, Bishopville. The stone is coarse-grained and consists mostly of friable snow-white enstatite. Rose observed other white grains, but could not identify them. I find these to be plagioclase. The third constituent is pyrrhotite. The stone's crust has a marbled appearance, being partly colorless, partly black, white, bluish, and gray. Enstatite occurs in large and small grains, mostly large. I observed distinct crystal boundaries on one of the small grains ...The grains are cut by many fine, irregular cracks (in addition to the cracks that were produced during preparation of the thin- section). Inclusions are rare and consist of opaque grains, less often of black needles. Plagioclase is usually attached to the small enstatite grains. I have not found plaogioclase with a regular crystal boundary. Its outlines are rounded, lobate, or elongated. In polarized light a very distinct twin structure is sometimes seen, consisting either of alternating wide and narrow lamellae, or entirely of extremely narrow lamellae having a finely-ruled appear- ance between crossed Nicols. Most untwinned plagioclase grains show undulose extinction; many are aggregates of several small grains. The identification of this mineral as plagioclase is based on its behavior in polarized light. An attempt to separate individual grains from the stone for further tests was unsuccessful, not only because of their small size but also because they could not be distinguished by color or luster from the enstatite. In places, the plagioclase shows streaks and slight cloudiness and is brownish by transmitted light. Small opaque inclusions are rare, but larger, often spindle-shaped, bronzite inclusions are abundant. Pyrrhotite forms large and small grains; in the specimen studied these grains are surrounded by brown areas, the result of reaction with the atmosphere. The analysis of Rammelsberg (1861), which found Al2O3, CaO, and alkalis in small amounts, in addition to the ingredients of enstatite, is in full agreement with the microscopic description just given. Rose also reports small amounts of nickel--iron and a black mineral that sometimes fills fine cracks. Breaking the stone along such cracks, I observed a shiny material, similar to that in meteorites to be described later, in which the veins consist of iron, pyrrhotite, and silicate glass. Received on Sat 10 Apr 2004 03:46:15 PM PDT |
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