Fullerenes and Interplanetary Dust at the Permian-Triassic Boundary

Details Fullerenes and Interplanetary Dust at the Permian-Triassic Boundary Fullerenes and Interplanetary Dust at the Permian-Triassic Boundary

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asbio...3...75p&link_type=abstract

Astrobiology, Volume 3, Issue 1, pp. 75-90.

Biology

10

Fullerene-Interplanetary, Dust, Particles-Permian-Triassic, Boundary-Mass Extinctions

Scientific paper

We recently presented new evidence that an impact occurred ~250 million years ago at the Permian-Triassic boundary (PTB), triggering the most severe mass extinction in the history of life on Earth. We used a new extraterrestrial tracer, fullerene, a third carbon carrier of noble gases besides diamond and graphite. By exploiting the unique properties of this molecule to trap noble gases inside of its caged structure (helium, neon, argon), the origin of the fullerenes can be determined. Here, we present new evidence for fullerenes with extraterrestrial noble gases in the PTB at Graphite Peak, Antarctica, similar to PTB fullerenes from Meishan, China and Sasayama, Japan. In addition, we isolated a 3He-rich magnetic carrier phase in three fractions from the Graphite Peak section. The noble gases in this magnetic fraction were similar to zero-age deep-sea interplanetary dust particles (IDPs) and some magnetic grains isolated from the Cretaceous-Tertiary boundary. The helium and neon isotopic compositions for both the bulk Graphite Peak sediments and an isolated magnetic fraction from the bulk material are consistent with solar-type gases measured in zero-age deep-sea sediments and point to a common source, namely, the flux of IDPs to the Earth's surface. In this instance, the IDP noble gas signature for the bulk sediment can be uniquely decoupled from fullerene, demonstrating that two separate tracers are present (direct flux of IDPs for 3He vs. giant impact for fullerene).

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