The surface dynamics and geophysical environment of asteroid (3200) Phaethon

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-04-01 DOI:10.1051/0004-6361/202453408
Hangbin Jo, Masateru Ishiguro, Derek C. Richardson, Sean E. Marshall, Tomoko Arai, Ko Ishibashi
{"title":"The surface dynamics and geophysical environment of asteroid (3200) Phaethon","authors":"Hangbin Jo, Masateru Ishiguro, Derek C. Richardson, Sean E. Marshall, Tomoko Arai, Ko Ishibashi","doi":"10.1051/0004-6361/202453408","DOIUrl":null,"url":null,"abstract":"<i>Context<i/>. (3200) Phaethon is a ∼5-kilometer-diameter near-Earth asteroid with a small perihelion distance of 0.14 au. It is the parent body of the Geminids. JAXA’s DESTINY<sup>+<sup/> mission will fly by Phaethon in the near future.<i>Aims<i/>. To support the preflight planning for the DESTINY<sup>+<sup/> mission, we performed a geophysical analysis of Phaethon’s surface and near-surface environment utilizing the latest shape model, which is based on numerous observations.<i>Methods<i/>. We employed the soft-sphere discrete element method code PKDGRAV to construct a “mascon” model of Phaethon and determine its gravity. We then computed the geopotential on Phaethon and derived various physical quantities related to its surface and near-surface dynamics.<i>Results<i/>. We calculated geophysical quantities for the surface, including surface acceleration and slope. To assess whether surface objects could be launched off the surface, we computed the escape speed, return speed, Jacobi speed, and the location and stability of equilibrium points around Phaethon, and conducted a simple dynamical simulation of launched particles.<i>Conclusions<i/>. Our results suggest that a large depression feature in the northern hemisphere could harbor exposed subsurface material and the freshest material on Phaethon. We propose that this depression be considered a key area for observation by the DESTINY<sup>+<sup/> mission.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"33 1","pages":""},"PeriodicalIF":5.8000,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202453408","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Context. (3200) Phaethon is a ∼5-kilometer-diameter near-Earth asteroid with a small perihelion distance of 0.14 au. It is the parent body of the Geminids. JAXA’s DESTINY+ mission will fly by Phaethon in the near future.Aims. To support the preflight planning for the DESTINY+ mission, we performed a geophysical analysis of Phaethon’s surface and near-surface environment utilizing the latest shape model, which is based on numerous observations.Methods. We employed the soft-sphere discrete element method code PKDGRAV to construct a “mascon” model of Phaethon and determine its gravity. We then computed the geopotential on Phaethon and derived various physical quantities related to its surface and near-surface dynamics.Results. We calculated geophysical quantities for the surface, including surface acceleration and slope. To assess whether surface objects could be launched off the surface, we computed the escape speed, return speed, Jacobi speed, and the location and stability of equilibrium points around Phaethon, and conducted a simple dynamical simulation of launched particles.Conclusions. Our results suggest that a large depression feature in the northern hemisphere could harbor exposed subsurface material and the freshest material on Phaethon. We propose that this depression be considered a key area for observation by the DESTINY+ mission.
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
小行星(3200)Phaethon的地表动力学和地球物理环境
上下文。(3200) Phaethon是一颗直径约5公里的近地小行星,近日点距离很小,为0.14 au。它是双子座的母体。JAXA的命运+任务将在不久的将来通过Phaethon飞行。为了支持DESTINY+任务的飞行前规划,我们利用基于大量观测的最新形状模型对Phaethon的表面和近表面环境进行了地球物理分析。采用软球离散元方法PKDGRAV建立了Phaethon的“mascon”模型并确定了其重力。然后,我们计算了法厄同的位势,并推导了与其表面和近表面动力学相关的各种物理量。我们计算了地表的地球物理量,包括地表加速度和坡度。为了评估表面物体是否可以被发射出表面,我们计算了逃逸速度、返回速度、雅可比速度以及Phaethon周围平衡点的位置和稳定性,并对发射粒子进行了简单的动力学模拟。我们的研究结果表明,北半球的一个大洼地特征可能包含在法厄同上暴露的地下物质和最新鲜的物质。我们建议将这个洼地视为命运+号任务观测的关键区域。
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
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
期刊最新文献
More power on large scales Exploring the origins of high-velocity features in SNe Ia with the spectral synthesis code TARDIS Lyman continuum escaping from in situ formed stars in a tidal bridge at z = 3 Data-driven magnetohydrodynamic simulation of the initiation of a coronal mass ejection with multiple stages eROSITA selection of new period-bounce cataclysmic variables
×
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
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