低質量星に対するCME のUV 放射量供給による生命存在領域の拡大

• 大石, 碧

• 渡邉, 恭子

• 釜谷, 秀幸

書誌事項

タイトル別名

• テイシツリョウセイ ニ タイスル CME ノ UV ホウシャリョウ キョウキュウ ニ ヨル セイメイ ソンザイ リョウイキ ノ カクダイ
• Expansion of Habitable Zone around Low Mass Stars by the Supply of UV Radiation from CME

抄録

It is very important to consider the amount of UV (ultra-violet) radiation for life existence and evolution because moderate UV radiation is necessary for the synthesis of biological compounds. Recently, life on the low mass stars has been suggested because of their long lifespan. However, these stars are out of ‘‘common region’’ between HZ (habitable zone) and UV-HZ, where the persistent life existence is expected because of lack of UV radiation. Then, this paper considers UV-HZ with the intensive supply of UV radiation from Coronal Mass Ejection (CME) and explores to increase the range of the common region around low mass stars. Then, we find the common region doesn’t always spread so much because CME size is proportion to the distance from a host star and the peak of UV luminosity depends on evolutionary phase of main sequence stars.

identifier:0385-7301

identifier:http://nda-repository.nda.ac.jp/dspace/handle/11605/101

収録刊行物

• 防衛大学校　　理工学研究報告

  防衛大学校　　理工学研究報告 第55巻 (第1号), 9-16, 2017-09

  防衛大学校

キーワード

• Habitable Zone
• UV Habitable Zone
• Low Mass Sars
• Coronal Mass Ejection

詳細情報

• CRID: 1050564287590864768
• NII論文ID: 120006358374
• NII書誌ID: AN00224173
• ISSN: 03857301
• NDL書誌ID: 028604383
• Web Site: http://hdl.handle.net/11605/101
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I028604383
• 本文言語コード: ja
• 資料種別: departmental bulletin paper
• データソース種別:
  • IRDB
  • NDL
  • CiNii Articles