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Effect of orbital parameters on the habitability on planets

Effect of orbital parameters on the habitability on planets
轨道参数对行星宜居性的影响
批准号:
13640435
负责人:
ABE Yutaka
金额:
$2.11万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
2001
资助国家:
日本
项目状态:
已结题
起止时间:
2001 至 2002

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中文摘要
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英文摘要
The condition for the occurrence of a completely frozen state (a "snow-ball" state) is investigated with a general circulation model for both a land planet case (a wet planet without fixed ocean) and an aqua planet (a planet entirely covered by an ocean) with a particular reference to the obliquity. Results : 1. A land planet shows stronger resistance to the com-plete freezing than an aqua planet. 2. Both land and aqua planets in an oblique regime show stronger resis-tance to the complete freezing than those in an upright regime. However, the dependence on the obliquity is not clear within the upright regime. 3. On a land planet in an oblique regime, low latitude area is more suscep-tible to freezing than the mid latitude area. Thus, there is a good chance of low-latitude-only freezing (freezing of low latitude without freezing the entire planet) of a land planet. 4. On an aqua planet with high obliquity, low latitude freezing occurs at lower solar constant than on a land planet with h … More igh obliquity. The range of the solar constant that yields low-latitude-only freezing is much narrower on an aqua planet than that on a land planet. Thus, low-latitude-only freezing is unlikely on an aqua planet. Implications for the paleo-Mars : 1. In order to keep a wet ground at the low latitude area of paleo-Mars, the planet must be in the oblique regime, or with oceans. Under such conditions, however, the low latitude is relatively easily covered by permanent snow. Thus, it is more difficult to keep unfrozen wet surface on low latitude than to keep Mars from the completely frozen state under the condition of the present obliquity. 2. If the obliquity changed significantly while Martian water cycle was active and the average temperature was de-creasing steadily, there must have been a period while only the low latitude area is covered by permanent snow. It is an interesting question whether we can find such evidence from geological records. Implication for the Habitability on a Planet : 1. A water rich aqua planet may not be the best place for life, and a land planet with some water may be better than an aqua planet, because an aqua planet easily falls in a completely frozen state. 2. It is a difficult question whether high obliquity or low obliquity planet is prefer-able. A high obliquity planet is resistive to the complete freezing, but experiences severe seasonal change. The calmest climate is found on 45° obliquity aqua planet. Less
期刊论文(9)
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Kimura, H., Y.Abe, A.Abe-Ouchi: "Role of ocean on planetary climate : an implication for ancient-mars"Lunar and Planetary Science (CD-ROM). XXXIII. 1731 (2002)
Kimura, H.、Y.Abe、A.Abe-Ouchi:“海洋对行星气候的作用:对古代火星的影响”月球与行星科学(CD-ROM)。
DOI: --
发表时间:
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影响因子: --
作者: []
通讯作者:
Abe, Y., A.Abe-Ouchi: "The effect of obliquity and surface condition on the freezing condition of a planet : implications for paleo-mars climate and habitable condition"Lunar and Planetary Science. XXXIV(CD-ROM). 1617 (2003)
Abe,Y.,A.Abe-Ouchi:“倾斜度和表面条件对行星冻结条件的影响:对古火星气候和宜居条件的影响”月球与行星科学。
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通讯作者:
Yutaka Abe, Ayako Abe-Ouchi: "The freezing condition of a land planet : effect of obliquity"Proceedings of the ISAS Lunar and Planetary Symposium. 35. 21-24 (2002)
Yutaka Abe、Ayako Abe-Ouchi:“陆地行星的冻结条件:倾角的影响”ISAS 月球和行星研讨会论文集。
DOI: --
发表时间:
期刊:
影响因子: --
作者: []
通讯作者:
Kimura, H., Y.Abe, A.Abe-Ouchi: "Role of ocean on planetary climate : an implication for ancient-mars"Lunar and Planetary Science. XXXIII(CD-ROM). 1731 (2002)
Kimura, H.、Y.Abe、A.Abe-Ouchi:“海洋对行星气候的作用:对古代火星的影响”月球与行星科学。
DOI: --
发表时间:
期刊:
影响因子: --
作者: []
通讯作者:
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