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The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation

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

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The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation. / Way, Michael; Davies, Hannah; Duarte, Joao et al.
Yn: Geochemistry, Geophysics, Geosystems, Cyfrol 22, Rhif 8, e2021GC009983, 08.2021.

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

HarvardHarvard

Way, M, Davies, H, Duarte, J & Green, M 2021, 'The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation', Geochemistry, Geophysics, Geosystems, cyfrol. 22, rhif 8, e2021GC009983. https://doi.org/10.1029/2021GC009983

APA

Way, M., Davies, H., Duarte, J., & Green, M. (2021). The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation. Geochemistry, Geophysics, Geosystems, 22(8), Erthygl e2021GC009983. https://doi.org/10.1029/2021GC009983

CBE

Way M, Davies H, Duarte J, Green M. 2021. The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation. Geochemistry, Geophysics, Geosystems. 22(8):Article e2021GC009983. https://doi.org/10.1029/2021GC009983

MLA

Way, Michael et al. "The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation". Geochemistry, Geophysics, Geosystems. 2021. 22(8). https://doi.org/10.1029/2021GC009983

VancouverVancouver

Way M, Davies H, Duarte J, Green M. The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation. Geochemistry, Geophysics, Geosystems. 2021 Awst;22(8):e2021GC009983. Epub 2021 Gor 19. doi: 10.1029/2021GC009983

Author

Way, Michael ; Davies, Hannah ; Duarte, Joao et al. / The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation. Yn: Geochemistry, Geophysics, Geosystems. 2021 ; Cyfrol 22, Rhif 8.

RIS

TY - JOUR

T1 - The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation

AU - Way, Michael

AU - Davies, Hannah

AU - Duarte, Joao

AU - Green, Mattias

PY - 2021/8

Y1 - 2021/8

N2 - We explore two possible Earth climate scenarios, 200 and 250 million years into the future, using projections of the evolution of plate tectonics, solar luminosity, and rotation rate. In one scenario, a supercontinent forms at low latitudes, whereas in the other it forms at high northern latitudes with an Antarctic subcontinent remaining at the south pole. The climates between these two end points are quite stark, with differences in mean surface temperatures approaching several degrees. The main factor in these differences is related to the topographic height of the high latitude supercontinents where higher elevations promote snowfall and subsequent higher planetary albedos. These results demonstrate the need to consider multiple boundary conditions when simulating Earth-like exoplanetary climates.

AB - We explore two possible Earth climate scenarios, 200 and 250 million years into the future, using projections of the evolution of plate tectonics, solar luminosity, and rotation rate. In one scenario, a supercontinent forms at low latitudes, whereas in the other it forms at high northern latitudes with an Antarctic subcontinent remaining at the south pole. The climates between these two end points are quite stark, with differences in mean surface temperatures approaching several degrees. The main factor in these differences is related to the topographic height of the high latitude supercontinents where higher elevations promote snowfall and subsequent higher planetary albedos. These results demonstrate the need to consider multiple boundary conditions when simulating Earth-like exoplanetary climates.

U2 - 10.1029/2021GC009983

DO - 10.1029/2021GC009983

M3 - Article

VL - 22

JO - Geochemistry, Geophysics, Geosystems

JF - Geochemistry, Geophysics, Geosystems

SN - 1525-2027

IS - 8

M1 - e2021GC009983

ER -