posted August 26, 2004
Meteorite Shower in Park Forest, Illinois
Written by Linda M. V. Martel
Its chemical and mineralogical compositions establish the Park Forest meteorite as an L5 chondrite, one of the most primitive groups of known meteorites. It is a strongly shocked monomict breccia (a term applied to a breccia made of one kind of rock) with light-colored clasts in a very dark matrix. The team measured cosmic radionuclides in Park Forest and found nearly zero 56Co and high 60Co, values that indicate a large preatmospheric mass. They estimate the meteoroid was at least 900 kilograms and possibly as large as 7000 kilograms before it broke apart in the atmosphere, of which only about 30 kilograms of fragments have been recovered.
Asteroids Don't Usually Drop on Neighborhoods
Most meteorites are samples of asteroids and most are recovered from one of the world's cold or hot deserts (eg. Antarctica, north Africa, Oman) a long time after striking ground. [See, for example, PSRD article Searching Antarctic Ice for Meteorites.] Witnessed falls, on the other hand, have a better chance of being recovered and transferred quickly into the laboratory for analyses while still in relatively fresh, uncontaminated condition. About 33% of the meteorites in the world's collections are witnessed falls, but not necessarily in heavily populated areas. Allende (Mexico, 1969), Murchison (Australia, 1969), and Tagish Lake (British Columbia, Canada, 2000) are examples of observed falls that have greatly expanded our understanding of the solar system's formation. [See PSRD article Tagish Lake -- A Meteorite from the Far Reaches of the Asteroid Belt.]
The Park Forest meteorite [Data link from Meteoritical Database] is one of the most recent observed falls in the United States. And it happened to land in the midst of a group of highly talented and busy cosmochemists--men and women who specialize in the study of meteorites. Talk about a lucky break! The newly established Chicago Center for Cosmochemistry is one example of how the cosmochemistry communities at the University of Chicago, Argonne National Laboratory, and the Field Museum have combined their expertise and facilities to study solar system science.
The fireball approached from the southwest and was visible from parts of Illinois, Indiana, Michigan, and Missouri. The subsequent meteorite shower hit the southern suburbs of Chicago at approximately 11:50 p.m. on March 26, 2003. Hundreds of meteorite fragments ranging from a few grams to 5.26 kilograms were recovered from the elongate strewnfield (approximately 8 x 3 kilometers), which spread by strong westerly winds over residential neighborhoods and a forest preserve (see the map below). The smallest pieces were deflected the furthest eastward and the largest pieces, carrying more momentum, were deflected the least.
The center of the strewnfield is Park Forest, about 40 kilometers south of Chicago. "I don't know of any other time when a meteoriticist was in the middle of a strewnfield," quipped co-author Lawrence Grossman (University of Chicago) referring to colleague Steven Simon's residence, which is marked with a star on the map shown above. The colored dots show the locations where meteorites were recovered. The colors represent different sizes of individual stones. A total of three kilograms are now in the meteorite collection at the Field Museum in Chicago, including the type specimen, a 545-gram fragment recovered from the Park Forest fire station (see photos below).
Classification of the Park Forest Meteorite
Park Forest is a breccia with light gray clasts in a very dark matrix, referred to as the light and dark lithologies, respectively. Most of the recovered meteorite fragments, especially the larger ones, are dominated by the light lithology. Olivine ((Mg, Fe)2)SiO4), pyroxene ((Ca, Mg, Fe)2Si2O6), metal (FeNi), sulfide (FeS) and chromite (FeCr2O4) grains are present in both lithologies, though only the dark lithology has a pervasive network of fine sulfide veins, which are opaque. They prevent light from penetrating into the rock, giving it a very dark appearance. Both lithologies contain chondrules with diameters ranging from ~600 microns to 1.3 millimeters. Olivine chondrules are the most abundant followed by olivine-free, pyroxene chondrules.
|This 232-gram sample of the Park Forest meteorite shows the light-colored angular clasts in the dark matrix. This piece was recovered the night of the shower and was used to measure cosmogenic radionuclides. The small divisions on the scale bar are millimeters.|
Average olivine, low-Ca pyroxene, and bulk oxygen-isotopic compositions show that Park Forest is an L chondrite (see plots below). The researchers further classified the meteorite as petrologic type 5 based on their observations that ferromagnesian minerals are well equilibrated (they are the same composition everywhere in the rock), the chondrules are easily recognized, and maskelynite (a glass formed from plagioclase feldspar by high shock pressures) is relatively fine grained (mostly less than or equal to 50 microns across).
|This plot shows olivine and pyroxene compositions in the light and dark lithologies of Park Forest compared with typical ranges in ordinary chondrites. Higher values reflect higher concentrations of iron in each mineral. Park Forest plots in the L chondrite field.||Oxygen isotopic compositions of the light (PF Light) and dark (PD Dark) lithologies in Park Forest are similar to each other and to the average of L chondrites (L fall avg).|
The conversion of plagioclase to maskelynite in Park Forest is one indication that it was strongly shocked. Other shock features in the meteorite include mosaicism and planar deformation in olivine, undulatory extinction in pyroxene, and glassy veins. Simon and his colleagues classify it as shock stage S5. [See PSRD article Asteroid Heating: A Shocking View for a good summary of the shock stages in chondrites, including movies of shocked and unshocked olivine grains rotated in polarized light using a petrographic microscope.]
About half the meteorites that fall today are L chondrites and many of them were shocked 465±15 million years ago, presumably when the parent asteroid body was smashed to pieces in a huge collision. Though the age of the Park Forest meteorite is yet unknown, its shock stage of S5 is consistent with the idea that it derived from the break-up of the L chondrite parent body. Some scientists consider the Flora family of S-type asteroids to be more remnants of the L chondrite parent body.
How Big was the Meteoroid?
One way of estimating the probable size range of a meteoroid before its breakup in the atmosphere (preatmospheric mass) is by measuring the concentrations (also called activities) of cosmogenic radionuclides in the meteorite. These are radioactive isotopes formed as a result of exposure to high-energy cosmic rays in space. Some of these, such as cobalt-56 (56Co), can only form at the surface of a body, while others, such as cobalt-60 (60Co), require some shielding and increase with depth in the parent body. If an object is too small, the cosmic rays will just pass through it and not make 60Co.
Simon and colleagues used a fragment of the Park Forest meteorite recovered the night of the shower (pictured above) and began their measurements less than 72 hours after the fall. They found very low (essentially zero) 56Co activity and high 60Co activity, consistent with a large preatmospheric mass for Park Forest. When they compared these observed radionuclide activities with calculated production rates in chondrites they determined that the sample they measured came from a depth of about 40 centimeters and could have been from an object that was at least 900 kilograms and possibly as large as 7000 kilograms. Other ways of estimating the original size of the object, based on work by Peter Brown of the University of Western Ontario and his colleagues of the energy released (seismic, light, sound) give an even higher range of 8000-11000 kilograms. The hundreds of fragments of the Park Forest meteorite that have been officially documented total about 18 kilograms. The authors estimate that at least 30 kilograms in all were probably recovered. Assuming that some of the fragments simply burned up during atmospheric entry, that still leaves plenty of extraterrestrial material out there to be found.
LINKS OPEN IN A NEW WINDOW
[ About PSRD |
[ Glossary | General Resources | Comments | Top of page ]