spacer
 
Advanced Search
Astrobiology Magazine Facebook  Astrobiology Magazine Twitter
  
Hot Topic Solar System Meteorites, Comets and Asteroids Finding a Rock that Knocked
 
Finding a Rock that Knocked
based on an PSRD release
print PDF
Meteorites, Comets and Asteroids
Posted:   06/18/06

Summary: Scientists have found a chunk of a meteorite that made an enormous impact crater in South Africa 146 million years ago. Found half a mile down, the chrondritic meteorite somehow survived the shock pressures and temperatures of the immense impact. Fossil meteorites have previously been found in craters.


The olivines and orthopyroxenes in the Morokweng meteorite (plotted as the star symbol) have higher iron contents than most other LL, L, and H chondrites. Axes are labeled Fs and Fa. Fs (ferrosilite, FeSiO3) is the iron-rich end-member of the enstatite-ferrosilite solid-solution series. Fa (fayalite, Fe2SiO4) is the iron-rich end-member of the olivine solid-solution series.)
Credit: Maier, et al. 2006. Nature, v.441, p.205.
A team of scientists report in the journal Nature the discovery of a 25-centimeter-wide chondritic meteorite unearthed from the 145-million-year-old Morokweng impact crater in South Africa.

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).

Photomicrograph taken in polarized transmitted light of chondrules in the Morokweng meteorite showing porphyritic orthopyroxene.
Credit: Wolfgang Maier, University of Quebec
Third, and unique to Morokweng's melt sheet is the new discovery reported by Wolf Maier and colleagues of a large (25-cm) fossil meteorite. Never before has such a boulder-sized chuck of the impactor been found within a large crater. Previously, researchers have found fossil meteorites in crater ejecta deposits, but finding a large fragment inside a huge crater had been deemed nearly impossible.

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.

Photomicrograph taken in polarized transmitted light of chondrules in the Morokweng meteorite showing excentroradial orthopyroxene.
Credit: Wolfgang Maier, University of Quebec
Does This Challenge Our Ideas of Impact Cratering?

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.

ESA Envisat MERIS mosaic of Africa
Until now craters larger than four kilometers in diameter have not yielded any large remnant meteorites. In these cases, the composition of the original impacting body is usually determined indirectly by analyzing chemical tracers of metals, such as nickel, cobalt, and the platinum-group elements. What were the special conditions that made it possible to preserve this unaltered meteorite in the Morokweng melt sheet? Was it slower than the normal 15-20 kilometers/second (maybe Earth's escape velocity of 11 kilometers/second)? Was it an asteroid rubble pile, hence weak? Running more cratering experiments and finding similar fossil meteorites on Earth in large impact craters, particularly those with melt sheets that contain an elevated dissolved platinum-group element component, would help to answer such questions. Perhaps future explorers will find projectile pieces in the impact melts of large lunar craters.

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.


Related Stories

Asteroid Riddling
Cold Case Crater
What Happened at Meteor Crater?
2029 A Near Miss Odyssey
The Great Impact Debate
Contemplating Craters

About Us
Contact Us
Links
Sitemap
Podcast Rss Feed
Daily News Story RSS Feed
Latest News Story RSS Feed
Learn more about RSS
Chief Editor & Executive Producer: Helen Matsos
Copyright © 2014, Astrobio.net