IMCA Insights – August 2007 This is the second part of Our Favorite Iron Meteorites, introducing you to some more great samples that have a very special place in the hearts and in the collections of the IMCA Board Members. Enjoy! Christian Anger: Silicated irons are very beautiful and amazing when watched under the microscope. The silicated iron meteorite Udei Station has, IMHO, the most beautiful silicate inclusions of all silicated irons. Especially the wonderful green chromian-diopside crystals are marvellous. Chromian-diopside Crystals in the Udei Station, IAB Iron Meteorite Udei Station is a witnessed iron meteorite fall, so it is a very fresh meteorite. A 103 kg mass fell in spring 1927 near the Benue River in Nigeria. It is a IAB medium octahedrite and represents the so called "Udei Station grouplet" in the IAB complex. The silicate sizes range from single grains up to 8 cm. Udei Station contains oxidized as well as reduced phases of Cr and P (i.e. chromian-diopside, chromite-daubreelite, and phosphate-phosphides) in addition to a most oxidized silicate mineralogy. The clasts in which these minerals occur are particularly interesting since they are depleted in high-Ca pyroxene and plagioclase and are probably an olivine-rich residue formed at relatively high temperature. Chromite is scattered throughout the inclusions. Phosphates can be found completely within the inclusions, but they also occur on the edges of the inclusions, in contact with the metallic matrix. A 239g Full Slice of
the Udei Station, IAB Iron Meteorite, My collection piece is an etched 239 g slice containing some green chromian-diopside crystals and the big silicate inclusion in the middle of the slice measures 65x35mm. Norbert Classen: I usually don't collect iron meteorites, but I have my favorite, anyway: the anomalous, silicate-rich IVA iron Steinbach. This historic German find consists of nearly equal parts of a IVA nickel-iron matrix and reddish silicates. These silicates are a mixture of pyroxenes and the rare mineral tridymite. It is still heavily debated whether this beautiful silicated iron represents a IVA analog to the pallasites, those true stony-iron meteorites that formed at the core/mantle boundary of their parent body, or if Steinbach is just a secondary product, formed during the reaccretion of the IVA parent body following a disrupting impact. A Slice of the Steinbach Iron; former Norbert Classen Coll. Sample Recent research suggests that the IVA irons formed in the core of a small, differentiated asteroid that was disrupted by a major impact shortly after its formation. After the asteroid was reaccreted, it was again disrupted about 450 million years ago. What an exciting history! Andrzej S. Pilski: Every iron is my
favourite except those totally weathered ones. However, I am allowed to
pick one only. So my best choice is the only iron I could find myself in
the field. The iron I could cut and etch so many specimens of. The iron
in which I could see tiny green crystals of cosmochlore, the Na-Cr
silicate. The Morasko IAB-MG iron. A Full Slice of Morasko from a 28kg Find, Coll. Andrzej S. Pilski The photo above shows a
full slice of Morasko, cut from a 28 kg find. Notice a large inclusion
of troilite (lower right), with a rim of graphite (black), schreibersite
and cohenite. Adam C. Hupé: My favorite iron
meteorite is Sikhote Alin, an Octahedrite type iron meteorite
that fell February 12th, 1947 in the Maritime Territory, Russia,
specifically the variety with thumb-printing (regmaglypts). To me,
Sikhote Alin represents what one would expect a meteorite to look like.
I find it interesting that the larger the individual, the larger the
regmaglypts. Conversely, I have observed near microscopic regmaglypts in
very small individuals. The thin black magnetite coating (crust) and
features like flow-lines make almost every individual Sikhote Alin a
wonder to observe with or without magnification. A Really Neat Sculptural Sikhote with Hole, Coll. Adam Hupé Oriented, note the flow-lines that encircle the leading edge. This is the best example of an X-Y oriented individual that I have seen meaning that it not only stabilized during flight but rotated as well: A Sikhote with Circular Flow-Lines, Coll. Adam Hupé Excellent example of a crater formed when another meteoroid struck it during its brief flight through the atmosphere. Note the raised rim: A Sikhote with an Impact Crater, Coll. Adam Hupé Pierre-Marie Pelé: Let me tell you the
story of my favorite iron meteorite, Mont-Dieu: Late June 1994,
during the Sainte-Marie-aux-Mines mineral show, Alain Carion had a stand
as usual. On the last day of the Show, a young couple stopped by at
Carion’s table and got a black metal piece from a plastic bag, measuring
about 4 cm, relatively light and very oxydized. They explained that they
got this piece from a man who had found a 40kg specimen with a metal
detector, underground. Slice of the IIE Mont-Dieu Iron, Photo Courtesy Eric Twelker Ten days later, Mr. C.
called Alain Carion: “I went back to the strewnfield with a friend, we
searched day and night and found more fragments, a total of 140kg. The
biggest weighs 95kg. I can sell them to you for the same price as the
first piece. You have a week to think about it or I'll sell to someone
else.” •
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