Testing the snowball Earth hypothesis for the Ediacaran

被引:8
|
作者
Ivanov, Alexei V. [1 ]
Mazukabzov, Anatoly M. [1 ]
Stanevich, Arkady M. [1 ]
Palesskiy, Stanislav V. [2 ]
Kozmenko, Olga A. [2 ]
机构
[1] Russian Acad Sci, Inst Earths Crust, Siberian Branch, Irkutsk 664033, Russia
[2] Russian Acad Sci, Inst Geol & Mineral, Siberian Branch, Novosibirsk 630090, Russia
关键词
CRETACEOUS-TERTIARY BOUNDARY; SOUTH-AUSTRALIA; BAIKAL GROUP; CONSTRAINTS; SEDIMENTS; ISOTOPES; HISTORY; IMPACT; BASIN; IR;
D O I
10.1130/G34345.1
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
Ediacaran Siberia was at tropical paleolatitudes when the glacigenic strata of the Goloustnaya Formation (Baikal Group, Siberia) were deposited at sea level. The presence of such deposits (at tropical latitudes) is at the core of the snowball Earth hypothesis, which is generally accepted for the previous Cryogenian glaciations. To test this hypothesis for the Ediacaran Period, we determined concentrations of platinum group elements (PGE) in the transitional unit between glacigenic conglomerates and postglacial cap carbonates of the Goloustnaya Formation. We speculate that if oceans were completely covered by ice during the glaciation, the ice prevented accumulation of PGE-rich cosmic dust and micrometeorites during that period, i.e., the snowball Earth stage. Such particles would have accumulated rapidly on the ocean floor at the ice-melting event, providing a geochemical signal; however, unlike the previous Cryogenian glaciations, this signal is at a background level, and we conclude that either the Ediacaran glaciation did not reach the snowball stage, or it was of very short duration.
引用
收藏
页码:787 / 790
页数:4
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