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Moonrock tells of little-known lunar layers.


Moonrock tells of little-known lunar layer

"It's wonderful," says Ursula B. Marvin, "that after all these years For the film, see .

"After All These Years" is the fifth and final single released by rock band Silverchair from their fourth album, Diorama, which was released in 2002, while "After All These Years" was released in 2003.
 one can still find a completely new rock type on the moon." According to Marvin, a space scientist at the Harvard-Smithsonian Center for Astrophysics The Harvard-Smithsonian Center for Astrophysics (CfA) is located in Cambridge, Massachusetts. It consists of the Harvard College Observatory and the Smithsonian Astrophysical Observatory. The Center is located at 60 Garden Street.  in Cambridge, Mass., the tiny fragment provides information about a little-sampled layer of the lunar crust.

Included among the samples brought back by the Apollo 15 astronauts in 1971, the unusual rock was pointed out to Marvin by Marilyn M. Lindstrom, who was working with the moon-rocks at the NASA NASA: see National Aeronautics and Space Administration.
NASA
 in full National Aeronautics and Space Administration

Independent U.S.
 Johnson Space Center in Houston. Marvin describes the rare bit, only about 1.5 millimeters across, as "white glass with two bright red spinels in it." Spinel spinel, magnesium aluminum oxide, MgAl2O4, a mineral crystallizing in the isometric system, usually as octahedrons. It occurs as an accessory mineral in basic igneous rocks, in aluminum-rich metamorphic rocks, and in contact-metamorphosed  is a crystalline mineral that exists in various colors, and although researchers might have broken up a larger chunk for different kinds of tests, Marvin says Lindstrom called this one "too small to split but too beautiful to pass up."

What makes it significant is that it contains tiny grains of a magnesium-rich mineral called cordierite cor·di·er·ite  
n.
A dichroic violet-blue to gray mineral silicate of magnesium, aluminum, and sometimes iron. Also called dichroite.



[French, after Pierre L.
, together with an olivine mineral called forsterite forsterite  

See under olivine.
. According to J. William Carey of Harvard University, the maximum pressure at which this combination could form is equal to that about 30 miles below the lunar surface, about 6 miles above the moon's crust-mantle boundary. A few Apollo moonrocks appear to have formed at greater depths, and some came from closer to the surface, but the Apollo 15 sample represents an intermediate level. The high magnesium content suggests it came from deeper than about 16 miles, Marvin says, while the cordierite means it was probably no more than 30 miles deep.

The researchers report in the Feb. 17 SCIENCE that the rarity of this combination, called a cordierite-spinel troctolite Troctolite is a rare ultramafic intrusive rock type. It consists essentially of variable amounts of olivine and calcic plagioclase along with variable minor pyroxene. It thus is midway between peridotite and anorthosite. , among the Apollo moonrock samples suggests it probably formed far enough down that only a major cataclysm, such as a meteorite impact, could have exposed it to view. The astronauts collected their samples near the moon's huge Imbrium basin, and the researchers suggest the cordierite bit was "excavated" by the same impact that formed Imbrium.
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Publication:Science News
Date:Feb 25, 1989
Words:346
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