From: University of Hawaii
Posted: Friday, May 21, 2004
In an article published today in the journal Nature, a team led by Robert Jedicke of the University of Hawaii's Institute for Astronomy provides convincing evidence that asteroids change color as they age.
David Nesvorny, a team member from the Southwest Research Institute in Boulder, CO, used a variety of methods to estimate asteroid ages that range from 6 million up to 3 billion years. Accurate color measurements for over 100,000 asteroids were obtained by the Sloan Digital Sky Survey (SDSS), and catalogued by team members Zeljko Ivezic from the University of Washington and Mario Juric from Princeton University.
Robert Whiteley, a team member from the USAF Space and Missile Systems Center in Los Angeles, points out that "the age-color correlation we found explains a long-standing discrepancy between the colors of the most numerous meteorites known as ordinary chondrites (OC) and their presumed asteroid progenitors." Meteorites are chips of asteroids and comets that have fallen to Earth's surface.
According to Jedicke, "If you were given a piece of rock from the Grand Canyon, you might expect that it would be red, like the colorful pictures in travel magazines. You'd be forgiven for questioning its origin if the rock had a bluish color. But if you were then told that the rocks turn from blue to Grand Canyon red because of the effects of weather, then everything might make sense. Your gift is simply a fresh piece of exposed rock, whereas the pictures you've seen show weathered cliff faces millions of years old."
Nesvorny explains that this is similar to the situation experienced by asteroid astronomers. "The meteorites are gifts of the solar system to scientists on Earth - pieces of asteroids delivered to their own backyard. The mystery is that the OC meteorites have a bluish color relative to the reddish color of the asteroids from which they were supposedly released." Jedicke asks, "How could they possibly be related?"
About thirty years ago, a "space weathering" effect was proposed to explain the color change. Meteorites, whose surface is affected by their fall through Earth's atmosphere, are usually studied in laboratories by observing their freshly cut and exposed interiors. Billions of years of exposure of the same material on the surface of an asteroid to solar and cosmic radiation and the heating effect of impacts of tiny asteroids might alter the surface color of asteroids in exactly the manner required to match the color of asteroids.
Jedicke said that they found that "asteroids get more red with time in exactly the right manner and at the right rate to explain the mystery of the color difference between them and OC meteorites." He added, "Even though we have found a link between the two types of objects, we still don't know what causes space weathering."
Once these researchers refine their analysis by obtaining more colors of the youngest-known asteroid surfaces, it will be possible to determine the age of any asteroid from its surface color. They are currently searching for a space weathering effect on other types of asteroids in the solar system.
The Institute for Astronomy at the University of Hawaii conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakala and Mauna Kea. Refer to http://www.ifa.hawaii.edu/ for more information about the Institute.
Funding for the creation and distribution of the SDSS Archive has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the U.S. Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society. The SDSS Web site is
The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The Participating Institutions are The University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, University of Pittsburgh, Princeton University, the United States Naval Observatory, and the University of Washington.
This enhanced false color image of Ida with its small satellite Dactyl to the right gives a vivid example of the effect of space weathering on asteroids. Blue regions on the asteroid tend to be associated with fresh young craters where subsurface material has been recently exposed to space. There are also blue regions associated with ridges and steep hills where surface material falls down during small "asteroid-quakes" to expose fresh surfaces. Red regions on the surface correspond to old craters and flat surfaces that have not been disturbed in a very long time. By measuring the rate of space weathering on asteroids Jedicke and his collaborators can now estimate the ages of the various colored regions on the surface of asteroids like Ida. Photo courtesy of NASA/JPL.
Note to Editors:
A high-resolution photograph of Dr. Jedicke is available at http://www.ifa.hawaii.edu/info/press-releases/jedicke.cmyk.300dpi.tif
Nature's Web site is http://www.nature.com/.
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