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深海中断记录揭示了轨道步伐为2.4 Myr的离心率大周期
Adriana Dutkiewicz1, Slah Boulila2,3, R Dietmar Müller4
1EarthByte Group, School of Geosciences, The University of Sydney, Sydney, NSW, 2006, Australia. adriana.dutkiewicz@sydney.edu.au.
Nature communications
|March 13, 2024
概括
天文学周期在数百万年内影响地球的气候. 这项研究揭示了深海记录中的~2.4 Myr离心率信号,可能与太阳系混乱有关,在古世 - 世热极限期间.
科学领域:
- 古气候学 古气候学
- 地质物理学 地质物理学
- 天文学 天文学
背景情况:
- 地球的气候受天文周期的影响,包括米兰科维奇周期 (10^4-10^5年) 和更长期的大周期.
- 在气候代理记录中检测长期的天文调制具有挑战性.
研究的目的:
- 通过使用深海间隙,研究气候变异的长期天文强迫.
- 为了识别和描述调节中新生代气候的主要周期.
主要方法:
- 频谱分析应用于Cenozoic深海间隙的数据集.
- 确定周期与天文学解决方案和主要地质事件的相关性.
主要成果:
- 在中断记录中检测到一个显著的~2.4 Myr离心率信号.
- 这种信号会定期被构造力强迫的事件所破坏.
- 一个主要的破坏恰逢古世 - 世热极限 (PETM) 和潜在的太阳系混乱.
结论:
- 深海间隙记录了长期的天文强迫,特别是一个~2.4 Myr的异心周期.
- 间隙最大值可能代表了与轨道偏心相关的深水循环加剧的时期.
- PETM的周期性干扰表明,地球气候与太阳系轨道动态之间存在潜在的联系.
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