Space Nomads: Meteorites in Sky, Field, and Laboratory — John Shaqi
Space Nomads: Meteorites in Sky, Field, and LaboratoryLaPaz, Lincoln
Science
Space Nomads: Meteorites in Sky, Field, and Laboratory
LaPaz, Lincoln
Meteorites
At the other end of the size-range, investigators have recovered
meteoritic masses weighing no more than a small fraction of a gram. From
a stone shower that occurred at Holbrook, Arizona, field searchers have
found some of the very smallest specimens in anthills. The insects had
carried these tiny meteorites along with sand and garnet grains in
building their hills!
[Illustration: COURTESY OF AMERICAN MUSEUM OF NATURAL HISTORY
The Willamette iron, famous for its great size and weight (14
tons), on exhibit at the Hayden Planetarium, New York City. See pp.
36, 39.]
The only sure way to determine whether or not an object _is_ a meteorite
is to have a small piece of it (say, a fragment the size of an egg)
tested chemically and microscopically by an expert on meteorites.
Nevertheless, there are several questions whose answers will help you to
decide whether or not you are on the right track in suspecting that a
“rock” you have found may be a meteorite:
Is your specimen especially heavy?
Does your specimen show a thin blackish or brownish crust on its outer
surface?
Does your “rock” have shallow, oval pits on its outer surface?
If the specimen has a corner knocked off, do you see specks and grains
of metal on the broken surface?
Is your specimen especially heavy? The iron and stony-iron meteorites
are very heavy. A 1-inch cube of iron meteorite weighs approximately 8
times as much as a 1-inch cube of ice. Even the stones, which are only
about half as dense as the irons, are much heavier than ordinary rocks.
Does your specimen show a thin blackish or brownish crust on its outer
surfaces? You will recall that specimens of both the Ussuri and Norton
meteorites showed a “glaze” of fused material which we call fusion
crust. Most freshly-fallen meteorites are covered with such a crust. To
illustrate how this crust forms, consider a snowball that you bravely
hold in your freezing hand until the outer surface melts. If you then
were to leave the snowball outside overnight, the melted outer surface
would freeze into a hard crust.
[Illustration: Piezoglyphs (oval pits resembling thumb-prints) in a
stone meteorite, found at Belly River, Canada. See p. 132.]
In similar fashion, the surface of a meteorite melts during the
blazing-hot part of its flight through the air, only to “freeze” into a
hard, firm coating in the lower, cooler portions of its path. This
hardened coating, the fusion crust, is of much importance. Its presence
is one of the best indications that a “rock” is really a meteorite. From
the character of the fusion crust, experts can piece together a good
deal about what happened to a meteorite on its way down to earth. If you
should be lucky enough to find a meteorite, don’t break off the fusion
crust. A whole encrusted specimen in the hand is worth 200 crustless
fragments scattered at your feet!
Public-domain text, read in full here on John Shaqi.
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