Astronomical tuning of the end-Permian extinction and the Early Triassic Epoch of South China and Germany

被引:137
作者
Li, Mingsong [1 ,2 ]
Ogg, James [1 ,3 ]
Zhang, Yang [1 ,3 ]
Huang, Chunju [1 ]
Hinnov, Linda [2 ,4 ]
Chen, Zhong-Qiang [1 ]
Zou, Zhuoyan [1 ]
机构
[1] China Univ Geosci, Sch Earth Sci, State Key Lab Biogeol & Environm Geol, Wuhan 430074, Hubei, Peoples R China
[2] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA
[3] Purdue Univ, Dept Earth Atmospher & Planetary Sci, 550 Stadium Mall Dr, W Lafayette, IN 47907 USA
[4] George Mason Univ, Dept Atmospher Ocean & Earth Sci, Fairfax, VA 22030 USA
基金
中国国家自然科学基金;
关键词
Triassic time scale; cyclostratigraphy; magnetostratigraphy; mass extinction; recovery; end-Permian; U-PB AGES; NANPANJIANG BASIN; MILANKOVITCH CYCLES; CARBON-CYCLE; BOUNDARY; MAGNETOSTRATIGRAPHY; CYCLOSTRATIGRAPHY; RECOVERY; SECTION; PERTURBATIONS;
D O I
10.1016/j.epsl.2016.02.017
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The timing of the end-Permian mass extinction and subsequent prolonged recovery during the Early Triassic Epoch can be established from astronomically controlled climate cycles recorded in continuous marine sedimentary sections. Astronomical-cycle tuning of spectral gamma-ray logs from biostratigraphically-constrained cyclic stratigraphy through marine sections at Meishan, Chaohu, Daxiakou and Guandao in South China yields an integrated time scale for the Early Triassic, which is consistent with scaling of magnetostratigraphy from climatic cycles in continental deposits of the Germanic Basin. The main marine mass extinction interval at Meishan is constrained to less than 40% of a 100-kyr (kilo year) cycle (i.e., <40 kyr) and the sharp negative excursion in delta C-13 is estimated to have lasted <6 kyr. The sharp positive shift in delta C-13 from -2 parts per thousand to 4 parts per thousand across the Smithian-Spathian boundary at Chaohu was completed in 50 kyr. The earliest marine reptiles in the Mesozoic at Chaohu that are considered to represent a significant recovery of marine ecosystems did not appear until 4.7 myr (million years) after the end-Permian extinction. The durations of the Griesbachian, Dienerian, Smithian and Spathian substages, including the uncertainty in placement of widely used conodont biostratigraphic datums for their boundaries, are 1.41 +/- 0.1, 0.61 +/- 0.1, 1.7 +/- 0.1 and 1.41 +/- 0.1 myr, implying a total span for the Early Triassic of 5.1 +/- 0.1 myr. Therefore, relative to an assigned 251.902 +/- 0.024 Ma for the Permian-Triassic boundary from the Meishan GSSP, the ages for these substage boundaries are 250.5 +/- 0.1 Ma for base Dienerian, 249.9 +/- 0.1 Ma for base Smithian (base of Olenekian stage), 248.2 +/- 0.1 Ma for base Spathian, and 246.8 +/- 0.1 Ma for the base of the Anisian Stage. This astronomical-calibrated timescale provides rates for the recurrent carbon isotope excursions and for trends in sedimentation accumulation through the Early Triassic of studied sections in South China. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:10 / 25
页数:16
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