globalchange  > 全球变化的国际研究计划
DOI: 10.1089/ast.2018.1942
WOS记录号: WOS:000480330100001
论文题名:
Intrinsic Climate Cooling
作者: Waltham, David
通讯作者: Waltham, David
刊名: ASTROBIOLOGY
ISSN: 1531-1074
EISSN: 1557-8070
出版年: 2019
语种: 英语
英文关键词: Habitability ; Faint Young Sun ; Red dwarfs ; Climate
WOS关键词: INITIAL MASS FUNCTION ; PLATE-TECTONICS ; CARBON-DIOXIDE ; SUPER-EARTHS ; SENSITIVITY ; OXYGEN ; CONSTRAINTS ; ATMOSPHERE ; PLANETS ; CO2
WOS学科分类: Astronomy & Astrophysics ; Biology ; Geosciences, Multidisciplinary
WOS研究方向: Astronomy & Astrophysics ; Life Sciences & Biomedicine - Other Topics ; Geology
英文摘要:

Lower heating of our planet by the young Sun was compensated by higher warming from factors such as greater greenhouse gas concentrations or reduced albedo. Earth's climate history has therefore been one of increasing solar forcing through time roughly cancelled by decreasing forcing due to geological and biological processes. The current generation of coupled carbon-cycle/climate models suggests that decreasing geological forcing-due to falling rates of outgassing, continent growth, and plate spreading-can account for much of Earth's climate history. If Earth-like planets orbiting in the habitable zone of red dwarfs experience a similar history of decreasing geological forcing, their climates will cool at a faster rate than is compensated for by the relatively slow evolution of their smaller stars. As a result, they will become globally glaciated within a few billion years. The results of this paper therefore suggest that coupled carbon-cycle/climate models account, parsimoniously, for both the faint young Sun paradox and the puzzle of why Earth orbits a relatively rare and short-lived star-type.


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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/145249
Appears in Collections:全球变化的国际研究计划

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作者单位: Royal Holloway Univ London, Dept Earth Sci, Egham, Surrey, England

Recommended Citation:
Waltham, David. Intrinsic Climate Cooling[J]. ASTROBIOLOGY,2019-01-01
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