Finding a Rock that Knocked
Found within the crater's impact melt sheet about 770 meters (half a mile) down a drilling borehole, the hefty meteorite's existence would seem improbable given its low chance of surviving the high shock pressures and temperatures normally associated with large impact events. Its unusual composition could mean it is a sample from a previously unknown part of the LL chondrite parent body. Or maybe it is from an entirely different asteroid population than other known meteorites.
The Morokweng crater is at the edge of the Kalahari Desert in northern South Africa. It has a diameter of at least 70 kilometers and is one of the largest terrestrial impact craters known today. Worn by erosion and obscured by sediments and Kalahari sands, the crater is unrecognizable on the surface. It was discovered by Marco Andreoli as a circular pattern of magnetic anomalies during early-1990s mining explorations.
In 1997, researchers from the University of the Witwatersrand and their colleagues reported that boreholes drilled into the center of the crater hit an impact melt sheet at least 870 meters thick. The melt sheet is rock at the base of the crater that was liquified by heat of the impact, and it has high abundances of chromium, nickel, cobalt, and the platinum-group elements.
The age of the crater was determined by isotopic age dating of zircons plucked from the impact melt rock. Ion microprobe analyses for uranium-thorium-lead isotopic compositions place the age of the crater at 146.2 ± 1.5 million years--the same age as a major geological boundary, the Jurassic-Cretaceous.
The Morokweng melt sheet is out of the ordinary for a few reasons. First, it contains more meteorite fragments than melt sheets of most other impact craters--fragments thought to be relicts of the impactor that created the crater. In Morokweng the fragments are pebble-sized (<1 centimeter) and represent 5 to 6 percent chondritic contamination of the melt sheet. That percentage is so high, only one other crater's melt sheet -- the Clearwater East crater in Quebec, Canada -- has come close to that figure. Second, the impact melt is unusually rich in nickel (up to 0.25% NiO in pyroxene) and chromium (up to 0.35% Cr2O3 in the orthopyroxene, and 0.69% in clinopyroxene).
Maier and his colleagues report that the Morokweng meteorite is chemically unaltered except for a thin (1 millimeter) coating of brown alteration minerals. Their laboratory analyses show that the meteorite has chondritic chromium isotope ratios and identical platinum-group element ratios to the bulk impact melt.
The research team found diagnostic features of a highly equilibrated chondrite breccia, including well-preserved chondrules of various textures: porphyritic, excentroradial (see images), and barred. These textures are produced by different degrees of melting and are typical of chondrules in chondrites. Olivines with 120o triple junctions indicate that recrystalization occurred in the parent asteroid as the result of thermal metamorphism. Maier and coauthors report that the fossil meteorite resembles an LL6 chondrite breccia, yet its atypical composition and texture do not fit exactly into any of the known chondrite groups. The platinum-group element contents of the Morokweng meteorite are lower than in normal LL chondrites. It contains unusually iron-rich silicates and iron-nickel sulfide, but does not have troilite (an iron sulfide) and there is no metal, which would be expected in this type of meteorite. It seems they have found some thing a little different.
The Morokweng fossil meteorite is a rare find. It is a surviving remnant of a much larger projectile that blasted out the crater. Its existence challenges the accepted idea that large bodies hit with such energy that they are melted or vaporized within seconds of impact. Laboratory modeling experiments and numerical simulations of the cratering process support this idea. For example, at high impact angles (close to vertical), the predicted peak shock pressures are 200-500 GPa. Predicted temperatures exceed 2,000K (1,700 oC). If any bits survived, they would be melted and chemically altered.
The discovery of the Morokweng fossil meteorite is a new piece of information that may help us better understand the bombardment history in the inner solar system. The unusual composition of Morokweng might suggest that the nature of meteorites may have changed through time -- types of impactors hitting Earth 145 million years ago were not the same as bodies hitting more recently. Morokweng may represent a sample of a different asteroid population from any other meteorite collected so far.
Maier and colleagues state that they found no evidence to suggest that the absence of metal and abundance of sulfide are the result of contamination from interaction with the impact melt. They attribute the mineralogy to metamorphism in the parent body. If the mineralogy reflects metamorphism in the parent body, then the Morokweng fossil meteorite could have come from a previously unknown interior portion of the LL chondrite parent body.