Early Cretaceous Terrestrial Milankovitch Cycles in the Luanping Basin, North China and Time Constraints on Early Stage Jehol Biota Evolution

被引:17
|
作者
Liu, Wei [1 ,2 ]
Wu, Huaichun [1 ,2 ]
Hinnov, Linda A. [3 ]
Xi, Dangpeng [1 ]
He, Huaiyu [4 ]
Zhang, Shihong [1 ]
Yang, Tianshui [1 ]
机构
[1] China Univ Geosci Beijing, State Key Lab Biogeol & Environm Geol, Beijing, Peoples R China
[2] China Univ Geosci, Sch Ocean Sci, Beijing, Peoples R China
[3] George Mason Univ, Dept Atmospher Ocean & Earth Sci, Fairfax, VA 22030 USA
[4] Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
基金
中国国家自然科学基金; 国家重点研发计划;
关键词
Early Cretaceous; Dabeigou Formation; magnetic susceptibility; astrochronology; Jehol Biota; Weissert Event; SONGLIAO BASIN; FEATHERED DINOSAURS; PALEOCLIMATE CHANGE; ISOTOPE EVENT; AGE; ASTROCHRONOLOGY; WEISSERT; CYCLOSTRATIGRAPHY; SEDIMENTATION; CALIBRATION;
D O I
10.3389/feart.2020.00178
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This research analyzes the cyclostratigraphy of the lacustrine Dabeigou Formation (DBG) of early Jehol Biota age (similar to 130-135 Ma) in the Luanping Basin, northern China. A high-resolution (2 cm interval), 117.82-m-long magnetic susceptibility (MS) stratigraphic series was measured along the Yushuxia section. MS is positively correlated with thorium, potassium and uranium concentrations associated with gamma ray intensity, and represents a proxy for detrital influx to the Luanping Basin. Power spectral analysis identifies a hierarchy of sedimentary cycles with wavelengths of 16.38 m, 5.85-3.28 m, 1.88-1.33 m, and 0.98-0.7 m, which are interpreted to represent Earth's orbital eccentricity, obliquity and precession index cycles. Objective testing of the MS series supports the interpretation of Milankovitch cycles, indicating an average sedimentation rate of 4.642-4.723 cm/kyr. A floating astronomical time scale with a duration of 2478 kyr is established from interpreted 405 kyr long orbital eccentricity cycles along the MS series. The 405-kyr tuned DBG MS time series closely matches the predicted orbital eccentricity of the La2004 astronomical solution from 130.787 to 133.265 Ma, providing independent temporal constraints on early stage Jehol Biota evolution. Finally, this estimated time interval for the DBG MS time series indicates that it occurred entirely within the Weissert Event.
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页数:15
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