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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Kombayashi–Ingersoll limit ： ウィキペディア英語版 Kombayashi–Ingersoll limit In planetary science, the Kombayashi–Ingersoll limit represents the maximum solar flux a planet can handle without a runaway greenhouse effect setting in.〔Raymond T. Pierrehumbert. Principles of Planetary Climate. Cambridge University Press. 2010〕 For planets with temperature-dependent sources of greenhouse gases such as liquid water and optically thin atmospheres the outgoing longwave radiation curve (which indicates how fast energy can be radiated away by the planet) flattens at high temperatures, reaching a horizontal asymptote - the Kombayashi–Ingersoll limit itself. Since the equilibrium temperature is the intersection of this curve and a horizontal line representing solar flux, for fluxes above this point the planet heats up indefinitely.〔http://www.skepticalscience.com/print.php?r=262〕 Kasting estimated the limit for Earth to 320 Watts per square meter. The limit is relevant for estimating the inner edge of the circumstellar habitable zone. However, the limit also depends on the surface gravity of the planet, making heavy worlds somewhat more resistant to the runaway effect.〔 ==References== 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Kombayashi–Ingersoll limit」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.