| Habitable zones of host stars during the post-MS phase | |
Guo JP(郭建坡)1,2,3 ; Zhang FH(张奉辉)1,2; Han ZW(韩占文)1,2; Guo, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
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| 发表期刊 | ASTROPHYSICS AND SPACE SCIENCE
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| 2010-06 | |
| 卷号 | 327期号:2页码:233-238 |
| DOI | 10.1007/s10509-010-0321-2 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 关键词 | Stars: Horizontal Branch Planets: Moons Astrobiology |
| 摘要 | A star will become brighter and brighter with stellar evolution, and the distance of its habitable zone will become larger and larger. Some planets outside the habitable zone of a host star during the main sequence phase may enter the habitable zone of the host star during other evolutionary phases. A terrestrial planet within the habitable zone of its host star is generally thought to be suitable for the existence of life. Furthermore, a rocky moon around a giant planet may be also suitable for life to survive, provided that the planet-moon system is within the habitable zone of its host star. Using Eggleton's code and the boundary flux of the habitable zone, we calculate the habitable zone of our Solar system after the main sequence phase. It is found that Mars' orbit and Jupiter's orbit will enter the habitable zone of the Solar system during the subgiant branch phase and the red giant branch phase, respectively. And the orbit of Saturn will enter the habitable zone of Solar during the He-burning phase for about 137 million years. Life is unlikely at any time on Saturn, as it is a giant gaseous planet. However, Titan, the rocky moon of Saturn, may be suitable for biological evolution and become another Earth during that time. For low-mass stars, there are similar habitable zones during the He-burning phase as our Solar, because there are similar core masses and luminosities for these stars during that phase. |
| 项目资助者 | National Natural Science Foundation of China [10773026, 10821061, 2007CB815406] ; Chinese Academy of Sciences [KJCX2-YW-T24] ; Yunnan Natural Science Foundation [06GJ061001] |
| 语种 | 英语 |
| 学科领域 | Astronomy & Astrophysics |
| 文章类型 | Article |
| ISSN | 0004-640X |
| URL | 查看原文 |
| 归档日期 | 2010-06-04 |
| WOS记录号 | WOS:000277165200007 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | EXTRASOLAR PLANETARY SYSTEMS ; STELLAR EVOLUTION ; BRANCH STARS ; LIFE ; OPACITIES ; MODEL ; MASS |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4500 |
| 专题 | 大样本恒星演化研究组 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Guo, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
| 作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P.R. China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650011, P.R. China 3.Graduate School of the Chinese Academy of Sciences, Beijing, 100049, P.R. China |
| 第一作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Guo JP,Zhang FH,Han ZW,et al. Habitable zones of host stars during the post-MS phase[J]. ASTROPHYSICS AND SPACE SCIENCE,2010,327(2):233-238. |
| APA | Guo JP,Zhang FH,Han ZW,&Guo, JP .(2010).Habitable zones of host stars during the post-MS phase.ASTROPHYSICS AND SPACE SCIENCE,327(2),233-238. |
| MLA | Guo JP,et al."Habitable zones of host stars during the post-MS phase".ASTROPHYSICS AND SPACE SCIENCE 327.2(2010):233-238. |
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| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| Habitable zones of h（735KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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