Do icy dust aggregates break up when they pass the snow line?

IF 3 2区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Icarus Pub Date : 2025-03-15 Epub Date: 2024-12-18 DOI:10.1016/j.icarus.2024.116430
Sin-iti Sirono
{"title":"Do icy dust aggregates break up when they pass the snow line?","authors":"Sin-iti Sirono","doi":"10.1016/j.icarus.2024.116430","DOIUrl":null,"url":null,"abstract":"<div><div>Icy dust aggregates can break up when they pass the snow line or when a heating event occurs because of the sublimation of H<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>O ice. However, the original aggregate may absorb the fragment conducting the Brownian motion because the thickness of the icy mantle of a grain is less than the typical grain radius of <span><math><mrow><mo>∼</mo><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mo>−</mo><mn>5</mn></mrow></msup><mspace></mspace></mrow></math></span>cm. On the other hand, the vapor pressure caused by the sublimated H<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>O molecules accelerates the fragment to escape. Rotation of the aggregate and electrostatic repulsion may also promote the escape of the fragment aggregate. Here, I determined a lower bound of the escaping fragment radius, including the effects of the vapor pressure, rotation, and electrostatic repulsion. It has been found that the breakup to the single grain does not occur, and the fragment radius strongly depends on the thickness of the icy mantle. The vapor pressure and the rotation produce fragments from large aggregates. The fragments escape from small aggregates by the electrostatic repulsion. Possible consequences of the breakup are discussed.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"429 ","pages":"Article 116430"},"PeriodicalIF":3.0000,"publicationDate":"2025-03-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Icarus","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0019103524004901","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2024/12/18 0:00:00","PubModel":"Epub","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Icy dust aggregates can break up when they pass the snow line or when a heating event occurs because of the sublimation of H2O ice. However, the original aggregate may absorb the fragment conducting the Brownian motion because the thickness of the icy mantle of a grain is less than the typical grain radius of 105cm. On the other hand, the vapor pressure caused by the sublimated H2O molecules accelerates the fragment to escape. Rotation of the aggregate and electrostatic repulsion may also promote the escape of the fragment aggregate. Here, I determined a lower bound of the escaping fragment radius, including the effects of the vapor pressure, rotation, and electrostatic repulsion. It has been found that the breakup to the single grain does not occur, and the fragment radius strongly depends on the thickness of the icy mantle. The vapor pressure and the rotation produce fragments from large aggregates. The fragments escape from small aggregates by the electrostatic repulsion. Possible consequences of the breakup are discussed.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
冰尘聚集物经过雪线时会破裂吗?
由于水冰的升华,冰冷的尘埃聚集体在经过雪线或发生加热事件时可能会破裂。然而,原始聚集体可能会吸收进行布朗运动的碎片,因为颗粒的冰地幔厚度小于典型的颗粒半径(~ 10−5cm)。另一方面,升华的水分子产生的蒸汽压加速了碎片的逃逸。聚集体的旋转和静电斥力也可能促进碎片聚集体的逃逸。在这里,我确定了逃逸碎片半径的下限,包括蒸汽压,旋转和静电排斥的影响。研究发现,不发生单粒碎裂,碎裂半径强烈依赖于冰地幔的厚度。蒸气压和旋转使大块的聚集体产生碎片。碎片通过静电斥力从小聚集体中逸出。讨论了分手可能产生的后果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Icarus
Icarus 地学天文-天文与天体物理
CiteScore
6.30
自引率
18.80%
发文量
356
审稿时长
2-4 weeks
期刊介绍: Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.
期刊最新文献
Investigation of the performance and influencing factors of imaging asteroid interiors by 2-D full-waveform inversion of quasi-monostatic radar data Infalling ring material produce layers of charged dust in the ionosphere of Saturn A systematic survey of von Zeipel–Lidov–Kozai resonances among trans-Neptunian objects: Empirical confirmation of the coupling with mean motion resonances Re-evaluation of meteor showers listed in the IAU Meteor Data Center The Material Point Method (MPM) for simulating hypervelocity impact on asteroids
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1