All posts tagged: carbonaceous chondrites

The asteroid that killed the dinosaurs was more odd than expected

The asteroid that killed the dinosaurs was more odd than expected

The asteroid that ended the age of dinosaurs may have been far rarer, drier and less sulfur-rich than scientists once thought. Traces buried in clay now point toward an unusual meteorite with roots in a distant part of the solar system. Nickel isotopes preserved at the boundary between the Cretaceous and Paleogene periods indicate that the Chicxulub impactor probably resembled a carbonaceous chondrite of the Ornans class, known as a CO chondrite. The findings came from researchers working in Paris, Brussels, Vienna and at the University of British Columbia. The team analyzed samples collected from impact clay layers in Denmark, Spain and Italy. CO chondrites represent a tiny fraction of meteorites recovered on Earth. They also contain fewer volatile substances, including carbon, zinc, water and sulfur, than several meteorite groups previously proposed as the Chicxulub projectile. Dr. Philippe Claeys, a visiting professor at the University of British Columbia, in front of an exhibit at the Pacific Museum of Earth. (CREDIT: University of British Columbia) “Carbonaceous chondrites of the Ornans class are definitely not like the …

Mysterious dust ring beyond Jupiter formed many of our Solar System’s earliest worlds

Mysterious dust ring beyond Jupiter formed many of our Solar System’s earliest worlds

In the young Solar System, a dust trap beyond Jupiter may have built wildly different meteorite parent bodies over two million years. New simulations suggest the same ring-shaped region sorted and recycled material by time, helping explain why carbonaceous chondrites differ so sharply. When Jupiter finished clearing out its neighborhood, it may have done more than carve a gap in the young Solar System. Just beyond that gap, according to new simulations, a ring of dust and gas became one of the most productive nurseries for early planetary building blocks, and one of the most versatile. The new work argues that this region outside Jupiter’s orbit did not produce just one kind of planetesimal. Over roughly two million years, it may have generated several distinct families, each with different mixtures of fine-grained dust and tougher, heat-processed solids. Those differences matter because many meteorites that land on Earth are fragments of these long-lost bodies, preserving a record of how the Solar System assembled itself. Researchers at the Max Planck Institute for Solar System Research in Germany …