Asteroids Get 'Sunburned' Quickly

Heather Catchpole, ABC Science Online
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April 28, 2009 -- Asteroids become redder the longer they stay out in the sun, a finding that could help determine our planetary origins, say U.S. and European researchers.

The research, which appears in the latest edition of Nature, found that the fresh surface of asteroid fragments redden in less than a million years, much faster than previously thought.

"Asteroids seem to get a sun tan very quickly," said research lead author Pierre Vernazza from the European Southern Observatory (ESO). "The charged, fast moving particles in the solar wind damage the asteroid's surface at an amazing rate."

It has long been known that asteroid surfaces change appearance over time, but the actual processes behind this weathering and the time involved were controversial.

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Using the ESO's New Technology Telescope and the Very Large Telescope in Chile, as well as telescopes in Spain and Hawaii, they analyzed the surfaces of S-type, stony asteroids, and Q-type asteroids, rich in the minerals pyroxene and olivine. These asteroids were formed by collisions as recently as one million years ago.

By comparing the age of the asteroids and their color, they determined solar wind was the culprit.

Solar wind, which consists of highly energetic particles released by the sun, is different from ultraviolet radiation, which is responsible for tanning human skin.

The finding is significant, as it will allow astronomers to better determine the origin of meteorites -- asteroid fragments that fall to Earth.

"Meteorites are time capsules from the beginning of the solar system," said Vernazza. "The value of their record of the earliest epoch of planetary formation is, with a few exceptions, compromised by the lack of precision with which we can pinpoint the location of their parent bodies."


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