More Wrinkles in Earth’s Climate History

2021 ◽  
pp. 57-79
2017 ◽  
Vol 114 (25) ◽  
pp. 6474-6479 ◽  
Author(s):  
William H. Amidon ◽  
G. Burch Fisher ◽  
Douglas W. Burbank ◽  
Patricia L. Ciccioli ◽  
Ricardo N. Alonso ◽  
...  

Although Earth’s climate history is best known through marine records, the corresponding continental climatic conditions drive the evolution of terrestrial life. Continental conditions during the latest Miocene are of particular interest because global faunal turnover is roughly synchronous with a period of global glaciation from ∼6.2–5.5 Ma and with the Messinian Salinity Crisis from ∼6.0–5.3 Ma. Despite the climatic and ecological significance of this period, the continental climatic conditions associated with it remain unclear. We address this question using erosion rates of ancient watersheds to constrain Mio-Pliocene climatic conditions in the south-central Andes near 30° S. Our results show two slowdowns in erosion rate, one from ∼6.1–5.2 Ma and another from 3.6 to 3.3 Ma, which we attribute to periods of continental aridity. This view is supported by synchrony with other regional proxies for aridity and with the timing of glacial ‟cold” periods as recorded by marine proxies, such as the M2 isotope excursion. We thus conclude that aridity in the south-central Andes is associated with cold periods at high southern latitudes, perhaps due to a northward migration of the Southern Hemisphere westerlies, which disrupted the South American Low Level Jet that delivers moisture to southeastern South America. Colder glacial periods, and possibly associated reductions in atmospheric CO2, thus seem to be an important driver of Mio-Pliocene ecological transitions in the central Andes. Finally, this study demonstrates that paleo-erosion rates can be a powerful proxy for ancient continental climates that lie beyond the reach of most lacustrine and glacial archives.


Elements ◽  
2021 ◽  
Vol 17 (2) ◽  
pp. 87-92 ◽  
Author(s):  
Kathleen A. Wendt ◽  
Xianglei Li ◽  
R. Lawrence Edwards

Speleothems are important timekeepers of Earth’s climate history. A key advantage of speleothems is that they can be dated using U–Th techniques. Mass spectrometric methods for measuring U and Th isotopes has led to vast improvements in measurement precision and a dramatic reduction in sample size. As a result, the timing of past climate, environment, and Earth system changes can be investigated at exceptional temporal precision. In this review, we summarize the principles and history of U–Th dating of speleothems. Finally, we highlight three studies that use U–Th dated speleothems to investigate past changes to the Asian monsoon, constrain the timing of sociopolitical change in ancient civilizations, and develop a speleothem-based calibration of the 14C timescale.


Author(s):  
Jan Zalasiewicz ◽  
Mark Williams

What is the future for the planet, and for climate? Gazing into crystal balls is a pastime that humans have a fascination for. It is also one in which they have a dismal record. A generation or two ago, there were predictions of cities made of glass or plastic, clothes of aluminium or asbestos, flying cars, the fall of nationalism and the rise of world government, the demise of religion, and robots taking over our tasks and ushering in an age of universal leisure for all. So much for all that. When we move, then, to the almost limitless complexities and intersecting feedbacks of Earth’s climate system, one might be forgiven for throwing in the towel straight away. This is a system, we must eternally remember, of which we have only partial understanding, even as we see today’s weather patterns spin off from it. Go back into the deep past, and that climate and those long-vanished weather patterns leave only traces in strata that are, in large part, invisible to the naked eye. And of the future, of course, we have no samples, no deep boreholes, no fossils: the canvas is blank—indeed, as yet there is no canvas at all. Yet, from those ancient stratal traces we can construct a picture of events that is both vivid and (within our levels of uncertainty) true. There is no reasonable doubt that 20,000 years ago massive ice sheets spread out from the poles—or, that 125,000 years ago there was a climate on Earth as temperate, within a degree or so, as the one we enjoy today. So, there are patterns, real patterns that we can use as guides to help us try, with the utmost caution and scepticism, to create pictures, scenarios, sketches of the climate of the future. One might imagine alternative futures—or create them—particularly with the help of those elapsed realities. For instance, one might take that striking five-million year slice of climate history put together by Lorraine Lisiecki and Maureen Raymo (see Ch. 8 ).


Author(s):  
Andrew P. Ingersoll

This clear and concise introduction to planetary climates explains the global physical and chemical processes that determine climate on any planet or major planetary satellite—from Mercury to Neptune and even large moons such as Saturn's Titan. The book presents a tour of our solar system's diverse planetary atmospheres, providing a rich foundation on their structure, composition, circulation, climate, and long-term evolution. Although the climates of other worlds are extremely diverse, the chemical and physical processes that shape their dynamics are the same. As this book makes clear, the better we can understand how various planetary climates formed and evolved, the better we can understand Earth's climate history and future. Explaining current knowledge, physical and chemical mechanisms, and unanswered questions, the book brings the reader to the cutting edge of this field.


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