diogenite
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Piece of a diogenitite that fell near Johnstown,
Colorado. It is brecciated and contains large orthopyroxene grains
in a groundmass of crushed and broken orthopyroxene. The specimen
is about 13 cm long. Photo by D. Ball, ASU.
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A type of achondrite and a member of the HED
group for which the parent body is believed to be the asteroid 2 Vesta.
Diogenites are named for the Greek philosopher Diogenes of Apollonia who,
in the fifth century B.C., was the first to suggest
that meteorites come from space (a realization that was subsequently forgotten
for the next 2,000 years).
Diogenites consist mostly of magnesium-rich orthopyroxene,
with smaller amounts of olivine and plagioclase.
The pyroxene is often in the form of sizeable crystals, indicating that
it cooled slowly, presumably within magma chambers deep within the crust
of Vesta.
The Tatahouine meteorite, a unique diogenite
that fell in small fragments Tunisia in 1931, is famous for its green, centimeter-sized
pyroxene crystals. Related category
METEORS
AND METEORITES
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