http://media-newswire.com/release_1083611.html

(Media-Newswire.com) - COLLEGE PARK, Md. - Two rare meteorites found in 
Antarctica two years ago are from a previously unknown, ancient asteroid with 
an outer layer or crust similar in composition to the crust of Earth's 
continents, reports a research team primarily composed of geochemists from the 
University of Maryland. 

Published in the January 8 issue of the journal Nature, this is the first ever 
finding of material from an asteroid with a crust like Earth's. The discovery 
also represents the oldest example of rock with this composition ever found. 

These meteorites point "to previously unrecognized diversity" of materials 
formed early in the history of the Solar System, write authors James Day, 
Richard Ash, Jeremy Bellucci, William McDonough and Richard Walker of the 
University of Maryland; Yang Liu and Lawrence Taylor of the University of 
Tennessee and Douglas Rumble III of the Carnegie Institution for Science. 

James Day looking at a portion of the meteorite in the University of Maryland's 
isotope geochemistry lab. In the background is a mass spectrometer used to 
analyze the meteorite samples. Prof. James Day looking at a portion of the 
meteorite in the University of Maryland's isotope geochemistry lab. In the 
background is a mass spectrometer used to analyze the meteorite samples. 

"What is most unusual about these rocks is that they have compositions similar 
to Earth's andesite continental crust -- what the rock beneath our feet is made 
of," said first author Day, who is a research scientist in Maryland's 
department of geology. "No meteorites like this have ever been seen before." 

Day explained that his team focused their investigations on how such different 
Solar System bodies could have crusts with such similar compositions. "We show 
that this occurred because of limited melting of the asteroid, and thus 
illustrate that the formation of andesite crust has occurred in our solar 
system by processes other than plate tectonics, which is the generally accepted 
process that created the crust of Earth." 

The two meteorites (numbered GRA 06128 and GRA 06129) were discovered in the 
Graves Nunatak Icefield during the US Antarctic Search for Meteorites (ANSMET) 
2006/2007 field season. Day and his colleagues immediately recognized that 
these meteorites were unusual because of elevated contents of a light-colored 
feldspar mineral called oligoclase. "Our age results point to these rocks being 
over 4.52 billion years old and that they formed during the birth of the Solar 
System. Combined with the oxygen isotope data, this age points to their origin 
from an asteroid rather than a planet," he said. 

There are a number of asteroids in the asteroid belt that may have properties 
like the GRA 06128 and GRA 06129 meteorites including the asteroid (2867) 
Steins, which was studied by the European Space Agency's Rosetta spacecraft 
during a flyby this past September. These so-called E-type asteroids reflect 
the Sun's light very brightly, as would be predicted for a body with a crust 
made of feldspar. 

According to Day and his colleagues, finding pieces of meteorites with andesite 
compositions is important because they not only point to a previously 
unrecognized diversity of Solar System materials, but also to a new mechanism 
to generate andesite crust. On the present-day Earth, this occurs dominantly 
through plates colliding and subduction - where one plate slides beneath 
another. Subduction forces water back into the mantle aiding melting and 
generating arc volcanoes, such as the Pacific Rim of Fire - in this way new 
crust is formed. 

"Our studies of the GRA meteorites suggest similar crust compositions may be 
formed via melting of materials in planets that are initially volatile- and 
possibly water-rich, like the Earth probably was when if first formed" said 
Day." A major uncertainty is how evolved crust formed in the early Solar System 
and these meteorites are a piece in the puzzle to understanding these 
processes." 

This research was funded by the NASA cosmochemistry program. 




      
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