Mid-Proterozoic day length stalled by tidal resonance

被引:6
|
作者
Mitchell, Ross N. [1 ,2 ]
Kirscher, Uwe [3 ,4 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, State Key Lab Lithospher Evolut, Beijing, Peoples R China
[2] Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
[3] Univ Tubingen, Dept Geosci, Tubingen, Germany
[4] Curtin Univ, Inst Geosci Res, Sch Earth & Planetary Sci, Earth Dynam Res Grp, Perth, Australia
基金
中国国家自然科学基金;
关键词
ROCK MAGNETIC CYCLOSTRATIGRAPHY; DOUSHANTUO FORMATION; SOUTH CHINA; MOON; CONSTRAINTS; DISSIPATION; DURATION; DYNAMICS; PLATFORM; HISTORY;
D O I
10.1038/s41561-023-01202-6
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present statistical analysis of a compilation of observational constraints on the Precambrian length of day and find that the day length stalled at about 19 h for about 1 billion years during the mid-Proterozoic. We suggest that the accelerative torque of atmospheric thermal tides from solar energy balanced the decelerative torque of lunar oceanic tides, temporarily stabilizing Earth's rotation. This stalling coincides with a period of relatively limited biological evolution known as the boring billion.
引用
收藏
页码:567 / +
页数:7
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