Habitable zones of host stars during the post-MS phase
文献类型：期刊论文
| 作者 | Guo JP(郭建坡)1,2,3 ; Zhang FH(张奉辉)1,2; Han ZW(韩占文)1,2
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| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
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| 出版日期 | 2010-06 |
| 卷号 | 327期号:2页码:233-238 |
| 关键词 | Stars: horizontal branch Planets: moons Astrobiology |
| ISSN号 | 0004-640X |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Guo, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | 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. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | EXTRASOLAR PLANETARY SYSTEMS ; STELLAR EVOLUTION ; BRANCH STARS ; LIFE ; OPACITIES ; MODEL ; MASS |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1007%2Fs10509-010-0321-2 |
| 语种 | 英语 |
| WOS记录号 | WOS:000277165200007 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/4500]  |
| 专题 | 云南天文台_大样本恒星演化研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
| 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 |
| 推荐引用方式 GB/T 7714 | Guo JP,Zhang FH,Han ZW. 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.(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. |
入库方式： OAI收割
来源：云南天文台
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