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Explicitly modelled deep-time tidal dissipation and its implication for Lunar history

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

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Explicitly modelled deep-time tidal dissipation and its implication for Lunar history. / Green, Mattias; Huber, Matthew; Waltham, David et al.
Yn: Earth and Planetary Science Letters, Cyfrol 461, 01.03.2017, t. 46–53.

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

HarvardHarvard

Green, M, Huber, M, Waltham, D, Buzan, J & Wells, M 2017, 'Explicitly modelled deep-time tidal dissipation and its implication for Lunar history', Earth and Planetary Science Letters, cyfrol. 461, tt. 46–53. https://doi.org/10.1016/j.epsl.2016.12.038

APA

Green, M., Huber, M., Waltham, D., Buzan, J., & Wells, M. (2017). Explicitly modelled deep-time tidal dissipation and its implication for Lunar history. Earth and Planetary Science Letters, 461, 46–53. https://doi.org/10.1016/j.epsl.2016.12.038

CBE

Green M, Huber M, Waltham D, Buzan J, Wells M. 2017. Explicitly modelled deep-time tidal dissipation and its implication for Lunar history. Earth and Planetary Science Letters. 461:46–53. https://doi.org/10.1016/j.epsl.2016.12.038

MLA

Green, Mattias et al. "Explicitly modelled deep-time tidal dissipation and its implication for Lunar history". Earth and Planetary Science Letters. 2017, 461. 46–53. https://doi.org/10.1016/j.epsl.2016.12.038

VancouverVancouver

Green M, Huber M, Waltham D, Buzan J, Wells M. Explicitly modelled deep-time tidal dissipation and its implication for Lunar history. Earth and Planetary Science Letters. 2017 Maw 1;461:46–53. Epub 2017 Ion 6. doi: 10.1016/j.epsl.2016.12.038

Author

Green, Mattias ; Huber, Matthew ; Waltham, David et al. / Explicitly modelled deep-time tidal dissipation and its implication for Lunar history. Yn: Earth and Planetary Science Letters. 2017 ; Cyfrol 461. tt. 46–53.

RIS

TY - JOUR

T1 - Explicitly modelled deep-time tidal dissipation and its implication for Lunar history

AU - Green, Mattias

AU - Huber, Matthew

AU - Waltham, David

AU - Buzan, Jonathan

AU - Wells, Martin

PY - 2017/3/1

Y1 - 2017/3/1

N2 - Dissipation of tidal energy causes the moon to recede away from the Earth. The currently measured rate of recession implies that the moon is about 1,500Ma, but the moon is known to be ~4,500Ma old. Consequently, it has been proposed that tidal energy dissipation was weaker in the Earth's past, but explicit numerical calculations are missing for such long time intervals. Here, for the first time, numerical tidal model simulations linked to climate model output are conducted for a range of paleogeographic configurations over the last 252Ma. We find that the present is a poor guide to the past in terms of tidal dissipation: the total dissipation rates for most of the past 252Ma were far below present levels. This confirms the old-age moon theory, and the lower dissipation allow refinement of orbitally-derived age models by shifting ages by an entire precession cycle.

AB - Dissipation of tidal energy causes the moon to recede away from the Earth. The currently measured rate of recession implies that the moon is about 1,500Ma, but the moon is known to be ~4,500Ma old. Consequently, it has been proposed that tidal energy dissipation was weaker in the Earth's past, but explicit numerical calculations are missing for such long time intervals. Here, for the first time, numerical tidal model simulations linked to climate model output are conducted for a range of paleogeographic configurations over the last 252Ma. We find that the present is a poor guide to the past in terms of tidal dissipation: the total dissipation rates for most of the past 252Ma were far below present levels. This confirms the old-age moon theory, and the lower dissipation allow refinement of orbitally-derived age models by shifting ages by an entire precession cycle.

U2 - 10.1016/j.epsl.2016.12.038

DO - 10.1016/j.epsl.2016.12.038

M3 - Article

VL - 461

SP - 46

EP - 53

JO - Earth and Planetary Science Letters

JF - Earth and Planetary Science Letters

SN - 0012-821X

ER -