Jupiter's Formation in the Vicinity of the Amorphous Ice Snowline
Mousis, Olivier1; Ronnet, Thomas2; Lunine, Jonathan I.3
2019-04-10
发表期刊ASTROPHYSICAL JOURNAL
ISSN0004-637X
EISSN1538-4357
卷号875期号:1
摘要Argon, krypton, xenon, carbon, nitrogen, sulfur, and phosphorus have all been measured and found to be enriched by a quasi uniform factor in the 2-4 range, compared to their protosolar values, in the atmosphere of Jupiter. To elucidate the origin of these volatile enrichments, we investigate the possibility of an inward drift of particles made of amorphous ice and adsorbed volatiles, and their ability to enrich in heavy elements the gas phase of the protosolar nebula, once they cross the amorphous-to-crystalline ice transition zone, following the original idea formulated by Monga & Desch. To do so, we use a simple accretion disk model coupled to modules depicting the radial evolution of icy particles and vapors, assuming growth, fragmentation, and crystallization of amorphous grains. We show that it is possible to accrete supersolar gas from the nebula onto proto-Jupiter's core to form its envelope, and allowing it to match the observed volatile enrichments. Our calculations suggest that nebular gas, with a metallicity similar to that measured in Jupiter, can be accreted by its envelope if the planet is formed in the similar to 0.5-2 Myr time range and in the 0.5-20 au distance range from the Sun, depending on the adopted viscosity parameter of the disk. These values match a wide range of Jupiter's formation scenarios, including in situ formation and migration/formation models.
关键词planets and satellites: composition planets and satellites: formation planets and satellites: gaseous planets protoplanetary disks stars: formation
DOI10.3847/1538-4357/ab0a72
收录类别SCI
语种英语
WOS关键词Astronomy & Astrophysics
WOS研究方向Science & Technology
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000468788900009
出版者IOP PUBLISHING LTD
引用统计
文献类型期刊论文
专题任务一_子任务一
循证社会科学证据集成
任务一
作者单位1.Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
2.Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
3.Lund Univ, Dept Astron & Theoret Phys, Lund Observ, Box 43, SE-22100 Lund, Sweden
推荐引用方式
GB/T 7714
Mousis, Olivier,Ronnet, Thomas,Lunine, Jonathan I.. Jupiter's Formation in the Vicinity of the Amorphous Ice Snowline[J]. ASTROPHYSICAL JOURNAL,2019,875(1).
APA Mousis, Olivier,Ronnet, Thomas,&Lunine, Jonathan I..(2019).Jupiter's Formation in the Vicinity of the Amorphous Ice Snowline.ASTROPHYSICAL JOURNAL,875(1).
MLA Mousis, Olivier,et al."Jupiter's Formation in the Vicinity of the Amorphous Ice Snowline".ASTROPHYSICAL JOURNAL 875.1(2019).
条目包含的文件
条目无相关文件。
个性服务
查看访问统计
谷歌学术
谷歌学术中相似的文章
[Mousis, Olivier]的文章
[Ronnet, Thomas]的文章
[Lunine, Jonathan I.]的文章
百度学术
百度学术中相似的文章
[Mousis, Olivier]的文章
[Ronnet, Thomas]的文章
[Lunine, Jonathan I.]的文章
必应学术
必应学术中相似的文章
[Mousis, Olivier]的文章
[Ronnet, Thomas]的文章
[Lunine, Jonathan I.]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。

元出版是什么?

元出版是融合预印本出版、数据出版、结构化信息出版等当前开放出版实践与理念为一体的开放出版新模式,旨在提供一个科学工作者完全融入的泛在沉浸式开放知识交流机制。

MetaPub团队

  • 关于我们
  • 编委会
  • 审稿专家
  • 编辑部

开放研究

  • 学科领域
  • 入驻期刊
  • 入驻会议
  • 开放数据集

帮助

  • 元作品投稿流程
  • 元作品写作要求
  • 元作品出版声明
  • 元作品出版标准
  • 审稿注意事项
地址:四川天府新区群贤南街289号 邮编:610299 电子邮箱:liucj@clas.ac.cn
版权所有 蜀ICP备05003827号