This analysis reveals the MPT's sensitivity to initial state in the Earth system, suggesting orbital forcing drives this transition.
The Middle Pleistocene Transition (MPT), i.e., the “fast” transition from ~41- to ~100-kyr rhythmicity that occurred about 1 Myr ago, remains one of the most intriguing phenomena of the past climate. The cause of this period shift is generally thought to be a change within the Earth System, since the orbital insolation forcing does not change its pattern through the MPT. Using a dynamical model rooted in ocean chemistry, we advance three novel concepts here: (a) the MPT could be a dominant-period relaxation process that is strongly dependent on the initial state of the system, (b) this sensitivity to the initial state is enabled by the orbital forcing, and (c) depending on the amplitude of the orbital forcing and initial values, the MPT could have been not just of the 40 – 80 kyr type, as we observe in the available data, but also of a 20 – 40, 80 – 100, 40 – 120, or even 80 – 40 kyr type.
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Verbitsky et al. (2025) studied this question.
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