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Finding a lunar meteorite's home.


Scientists have for the first time pinpointed the source of a meteorite meteorite, meteor that survives the intense heat of atmospheric friction and reaches the earth's surface. Because of the destructive effects of this friction, only the very largest meteors become meteorites.  that came from the moon. By measuring the rock's age, the researchers have precisely dated the rock's lunar home, the Imbrium impact basin, which is the youngest of the moon's large impact craters. That crater's age may have special significance because Imbrium's formation marks the end of an era in which space debris Space debris or orbital debris, also called space junk and space waste, are the objects in orbit around Earth created by humans, that no longer serve any useful purpose.  walloped the inner solar system solar system, the sun and the surrounding planets, natural satellites, dwarf planets, asteroids, meteoroids, and comets that are bound by its gravity. The sun is by far the most massive part of the solar system, containing almost 99.9% of the system's total mass. . Researchers have long argued that life on Earth couldn't have evolved until after that bombardment.

Found in the desert of Oman in 2002, the 7-ounce stone has a greenish hue mixed with bits of white. That appearance is typical of lunar rocks, but this meteorite turns out to be exceptional.

Edwin Gnos of the University of Bern The University of Bern is a university in the Swiss capital of Bern. It was founded in 1834. As one of the German-speaking universities in Switzerland its official name is Universität Bern, although it is frequently referred to in the French form, Université de Berne.  in Switzerland and his colleagues found that relative to other rocks from the moon, the stone contains high concentrations of uranium, thorium thorium (thôr`ēəm) [from Thor], radioactive chemical element; symbol Th; at. no. 90; at. wt. 232.0381; m.p. about 1,750°C;; b.p. about 4,790°C;; sp. gr. 11.7 at 20°C;; valence +4. , and potassium. The ratios of these elements to each other match those of only one group of lunar rocks, located in the Imbrium impact basin on the moon's near side.

Gnos' team determined the meteorite's age by radioactive dating radioactive dating: see dating. . The group describes the turbulent history of the meteorite, dubbed Sayh al Uhaymir (SaU) 169, in the July 30 Science.

According to the researchers, the 1,160-kilometer-wide Imbrium basin, along with the main rock in the meteorite, formed when an asteroid struck the moon 3.909 billion years ago. Two other impacts--2.8 billion years ago and 200 million years ago--brought the material close to the moon's surface. Finally, less than 340,000 years ago, another impact dislodged SaU 169 from the moon. The meteorite struck Earth 9,700 years ago.

Suffering at least five impacts in nearly 4 billion years, "SaU 169 is a rock which demonstrates impressively how rocks can travel, like a ping-pong-ball, from one body to another," the researchers note.--R.C.
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Title Annotation:Astronomy
Publication:Science News
Article Type:Brief Article
Geographic Code:1USA
Date:Aug 21, 2004
Words:314
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