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Milankovitch Cycle Evolution and Uncertainty
Dave Waltham
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Outline Croll-Milankovitch cycles Application to cyclostratigraphy
Earth-Moon system evolution The time-varying drag problem Time-evolution of CM cycles and their (big) uncertainties Beware!
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Croll-Milankovitch Cycles
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Cyclostratigraphy Wu et al, Time-calibrated Milankovitch cycles for the late Permian, Nature Communications
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Earth-Moon System Evolution
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Earth-Moon System Evolution
da/dt = f a-5.5
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Earth-Moon System Evolution
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Earth-Moon System Evolution
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Time Varying Drag f = 2.01±0.03 x 1038 m6.5 s-1
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Time-Varying Drag f = 6.85±0.08 x 1037 m6.5 s-1 = (0.344±0.004) f0
Don Dixon
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Time-Varying Drag OR
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Time-Varying Drag Stochastic Variation Log-normal variation
f = exp( m + s 2/2 ) Secular Increase Resonance in oceans is predicted to peak when day length ~ 27 hours (Webb, 1982)
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Time-Varying Drag Stochastic variation Monte-Carlo Simulation
Secular increase Exponential approximation
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Time-Varying Drag Geological Constraints Tidal Rhythmites
Only really good ones are from Elatina/Reynella (Williams, 1989, 2000; Deubner, 1990) 620±20 Ma f = (0.51±0.02) f0
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Time-Varying Drag
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Time-Varying Obliquity
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Time-Varying Obliquity
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Web-based Tool
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Beware!
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