![]() ![]() You can see the metal shining on a broken surface. Most meteorites contain at least some iron metal (actually an alloy of iron and nickel). Ordinary chondrites and stony meteorites like the one at left have smooth surfaces or regmaglypts. Most iron meteorites, like the example at right, have well-developed regmaglypts all over their surface. ![]() The surface of a meteorite is generally very smooth and featureless, but often has shallow depressions and deep cavities resembling clearly visible thumbprints in wet clay or Play-Doh. This web page has some good examples of desert varnish. Usually, but not always, you will be able to see the same kind of varnish on lots of rocks in the same area. This develops due to microbial activity on the rock. In desert areas, rocks often develop a shiny, black exterior called desert varnish. In the image to the right, the fusion crust is the thin, black coating on the outside of the meteorite. However, this crust weathers to a rusty brown color after several years of exposure on the Earth's surface and will eventually disappear altogether. It is often black and looks like an eggshell coating the rock. This thin crust is called a fusion crust. When a meteorite falls through the Earth's atmosphere a very thin layer on the outer surface melts. Meteorites which have fallen recently may have a black "ash-like" crust on their surface. Since detailed analyses take time and money, look for the easy characteristics first. Sometimes, detailed chemical analyses need to be done, but only on rocks that meet all these characteristics. Usually, meteorites have all or most of these characteristics. You can use this list to guide you through them. Meteorites have several distinguishing characteristics that make them different from terrestrial (Earth) rocks. Several booms may be succeeded by irregular sputtering sounds, comparable to an automobile backfiring. Because the fireballs are traveling at high speeds, they sometimes produce a sonic boom or whistling heard 30 miles or more from where the meteorite lands. A smoke or dust trail is produced in the sky by the fireball caused by the removal of material from the surface of the meteorite. When a meteor enters the Earth's atmosphere the resulting fireball produces light, due to the friction between its surface and the air. Meteorites fall to Earth all the time and are distributed over the entire planet, so you could even find one in your own backyard! They are rocks that are similar in many ways to Earth rocks, but it is exciting to find a piece of another planet here on Earth. Meteorites are pieces of asteroids and other bodies like the moon and Mars that travel through space and fall to the earth. ![]() Nature 267, 414–415 (1977).Do You Think You May Have Found a Meteorite? Handbook of Iron Meteorites (University of California Press, 1975).Īxon, H. Arizona's Meteorite Crater (American Meteorite Museum, Arizona, 1956). Here we present the metallographic and X-ray diffraction data on which this conclusion is based. The shock event that produced these high pressure phases, therefore, must have taken place on its parent body or have been associated with the disruption of that body. It seems, therefore, that the diamond and lonsdaleite were present in the meteoroid before its final ablative passage through the atmosphere and soft landing on the ground. Virtually identical diamond–lonsdaleite-containing material in ALHA77283 occurs in a meteorite specimen with a well developed heat-altered zone produced by atmospheric ablation. The suggestion 7 that formation was by high gravitational pressure has not been accepted. The Canyon Diablo, Arizona, meteorite, the excavator of Meteor Crater, is the only other iron meteorite known to contain these high-pressure minerals, and their occurrence in that meteorite has been explained as the result of shock-induced transformation of graphite, most probably at the moment of terrestrial impact and disintegration of the projectile during crater formation 3–6. One of these, ALHA77283, contains troilite(FeS)–graphite(C)–schreibersite((Fe,Ni) 3P)–cohenite(Fe 3C) inclusions rich in the carbonado-type diamond–lonsdaleite ‘nodules’ previously described from the Canyon Diablo meteorite 1,2. Of the many meteorites recovered so far from the Allan Hills, Antarctica, only nine have been irons. ![]()
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