A climatic control on the accretion of meteoric and super-chondritic iridium-platinum to the Antarctic ice cap
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- A climatic control on the accretion of meteoric and super-chondritic iridium-platinum to the Antarctic ice cap
- Other Titles
- 남극빙상으로 축적되는 외계기원 및 화산기원 이리듐과 플래티늄의 기후적 조절
- J. Plane
- Geochemistry & Geophysics
- Antarctica; ice; iridium; meteoric smoke; platinum
- Issue Date
- J. Plane, et al. 2006. "A climatic control on the accretion of meteoric and super-chondritic iridium-platinum to the Antarctic ice cap". EARTH AND PLANETARY SCIENCE LETTERS, 250(3-4): 459-469.
- Meteoric smoke particles (MSPs) form through the vaporization of meteoroids and the subsequent re-condensation of metallic species in the mesosphere. Recently, iridium and platinum enrichments have been identified in Greenland ice layers and attributed to the fallout of MSPs supplying polar latitudes with cosmic matter during the Holocene. However, the MSP fallout to Antarctica during the Earth's climatic history remains essentially unknown. We have determined iridium and platinum in deep Antarctic ice from Dome C and Vostok dated back to 240 kyrs BP. We find high super-chondritic fluxes during warm periods and low meteoric accretion during glacial times, a pattern that is opposite to any known climatic variation in dust fallout to polar regions. The proposed explanation of this accretion regime is a weaker polar vortex during warm periods, allowing peripheral air masses enriched in volcanic iridium and platinum to penetrate inland to Antarctica. The MSP signal emerges only during cold phases and is four times lower than in the Greenland ice cap where more snow accumulates. This suggests that wet deposition is an important route of cosmic material to the Earth's surface.
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