Ramme Lennart, Ilyina Tatiana, Marotzke Jochem
Max Planck Institute for Meteorology, Hamburg, Germany.
International Max Planck Research School on Earth System Modelling, Hamburg, Germany.
Nat Commun. 2024 Apr 26;15(1):3571. doi: 10.1038/s41467-024-47873-6.
When the Marinoan snowball Earth deglaciated in response to high atmospheric carbon dioxide (CO) concentrations, the planet warmed rapidly. It is commonly hypothesized that the ensuing supergreenhouse climate then declined slowly over hundreds of thousands of years through continental weathering. However, how the ocean affected atmospheric CO in the snowball Earth aftermath has never been quantified. Here we show that the ocean's carbon cycle drives the supergreenhouse climate evolution via a set of different mechanisms, triggering scenarios ranging from a rapid decline to an intensification of the supergreenhouse climate. We further identify the rapid formation of carbonate sediments from pre-existing ocean alkalinity as a possible explanation for the enigmatic origin of Marinoan cap dolostones. This work demonstrates that a moderate and relatively short-lived supergreenhouse climate following the Marinoan snowball Earth is a plausible scenario that is in accordance with geological data, challenging the previous hypothesis.
当 Marinoan 雪球地球因大气中高浓度二氧化碳(CO)而发生冰消作用时,地球迅速变暖。人们普遍推测,随后的超级温室气候在数十万年的时间里通过大陆风化作用而缓慢衰退。然而,在雪球地球事件之后,海洋如何影响大气中的 CO 从未被量化过。在此我们表明,海洋碳循环通过一系列不同机制驱动超级温室气候演变,引发了从超级温室气候迅速衰退到强化等不同情景。我们进一步确定,由先前海洋碱度快速形成碳酸盐沉积物,可能是 Marinoan 盖帽白云岩神秘成因的一种解释。这项研究表明,Marinoan 雪球地球事件之后出现适度且相对短暂的超级温室气候是一种符合地质数据的合理情景,这对先前的假设提出了挑战。