Dallas H. Abbott, Dee Breger, Pierre E. Biscaye, John A. Barron, Robert A. Juhl and Patrick McCafferty
What caused terrestrial dust loading and climate downturns between A.D. 533 and 540? (in Volcanism, impacts, and mass extinctions; causes and effects )
Special Paper - Geological Society of America(September 2014), 505:421-438
Index Terms/Descriptors: aerosols; algae; asteroids; atmosphere; carbon; causes; Cenozoic; chondrites; climate change; climate forcing; comets; composition; condensation; cosmic dust; data processing; diatoms; ecology; Eta Aquarid meteor shower; experimental studies; extraterrestrial debris; GISP2; global change; global dimming; Halley's Comet; history; Holocene; ice cores; interplanetary dust; Invertebrata; laboratory studies; marine environment; marine sediments; mass extinctions; metals; meteor showers; meteorite flux; meteorites; microfossils; models; near-Earth objects; nickel; orbital forcing; orbits; particles; Plantae; Protista; provenance; Quaternary; seasonal variations; sediments; SEM data; Silicoflagellata; simulation; spectra; stony meteorites; time scales; tin; Tunguska event; upper Holocene; volatile elements; volcanism; X-ray spectra
Latitude & LongitudeN72°36'00'' - N72°36'00'' and W38°30'00'' - W38°30'00''
Sn-rich particles, Ni-rich particles, and cosmic spherules are found together at four discrete stratigraphic levels within the 362-360 m depth interval of the Greenland Ice Sheet Project 2 (GISP2) ice core (72.6 degrees N, 38.5 degrees W, elevation: 3203 m). Using a previously derived calendar-year time scale, these particles span a time of increased dust loading of Earth's atmosphere between A.D. 533 and 540. The Sn-rich and Ni-rich particles contain an average of 10-11 wt% C. Their high C contents coupled with local enrichments in the volatile elements I, Zn, Cu, and Xe suggest a cometary source for the dust. The late spring timing of extraterrestrial input best matches the Eta Aquarid meteor shower associated with comet 1P/Halley. An increased flux of cometary dust might explain a modest climate downturn in A.D. 533. Both cometary dust and volcanic sulfate probably contributed to the profound global dimming during A.D. 536 and 537 but may be insufficient sources of fine aerosols. We found tropical marine microfossils and aerosol-sized CaCO 3 particles at the end A.D. 535-start A.D. 536 level that we attribute to a low-latitude explosion in the ocean. This additional source of dust is probably needed to explain the solar dimming during A.D. 536 and 537. Although there has been no extinction documented at A.D. 536, our results are relevant because mass extinctions may also have multiple drivers. Detailed examinations of fine particles at and near extinction horizons can help to determine the relative contributions of cosmic and volcanic drivers to mass extinctions.