4.4 Article

Earth System Model Analysis of How Astronomical Forcing Is Imprinted Onto the Marine Geological Record: The Role of the Inorganic (Carbonate) Carbon Cycle and Feedbacks

期刊

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2020PA004090

关键词

astronomical forcing; carbon cycling; early Cenozoic; earth system modeling; feedbacks; greenhouse climate

资金

  1. Heising-Simons Foundation
  2. NSF [1702913, 1658024]
  3. ERC
  4. Directorate For Geosciences [1702913] Funding Source: National Science Foundation
  5. Directorate For Geosciences
  6. Division Of Ocean Sciences [1658024] Funding Source: National Science Foundation
  7. Division Of Ocean Sciences [1702913] Funding Source: National Science Foundation

向作者/读者索取更多资源

Astronomical cycles play a significant role in marine geological records, providing insights into Earth system dynamics and aiding in the construction of age models. Through simulations, it has been shown that astronomical modulation impacts model variables differently, particularly with regards to carbon and nutrient cycling in the ocean. Further research is needed to fully understand the Earth system's response to astronomical forcing.
Astronomical cycles are strongly expressed in marine geological records, providing important insights into Earth system dynamics and an invaluable means of constructing age models. However, how various astronomical periods are filtered by the Earth system and the mechanisms by which carbon reservoirs and climate components respond, particularly in absence of dynamic ice sheets, is unclear. Using an Earth system model that includes feedbacks between climate, ocean circulation, and inorganic (carbonate) carbon cycling relevant to geological timescales, we systematically explore the impact of astronomically modulated insolation forcing and its expression in model variables most comparable to key paleoceanographic proxies (temperature, the delta C-13 of inorganic carbon, and sedimentary carbonate content). Temperature predominately responds to short and long eccentricity and is little influenced by the modeled carbon cycle feedbacks. In contrast, the cycling of nutrients and carbon in the ocean generates significant precession power in atmospheric CO2, benthic ocean delta C-13, and sedimentary wt% CaCO3, while inclusion of marine sedimentary and weathering processes shifts power to the long eccentricity period. Our simulations produce reduced pCO(2) and dissolved inorganic carbon (DIC) delta C-13 at long eccentricity maxima and, contrary to early Cenozoic marine records, CaCO3 preservation in the model is enhanced during eccentricity-modulated warmth. Additionally, the magnitude of delta C-13 variability simulated in our model underestimates marine proxy records. These model-data discrepancies hint at the possibility that the Paleogene silicate weathering feedback was weaker than modeled here and that additional organic carbon cycle feedbacks are necessary to explain the full response of the Earth system to astronomical forcing.

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