Trajectory estimation for fresh impacts on Mars

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Contributions of the Astronomical Observatory Skalnate Pleso Pub Date : 2021-12-01 DOI:10.31577/caosp.2021.51.3.241
E. Podobnaya, O. Popova, D. Glazachev
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引用次数: 0

Abstract

Exploration of small craters and craters clusters on Mars allows one to study meteoroid fragmentation details that cannot be detected in terrestrial conditions. It was suggested earlier that the description of a cluster with a scattering ellipse allows one to estimate the meteoroids’ trajectory, which is connected with orbital parameters of the impactor. Independent construction of scattering ellipses and comparison with crater ejecta demonstrate the accuracy and find out some problems of this approach.
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火星新一轮撞击的轨迹估计
探索火星上的小陨石坑和陨石坑群可以研究在陆地条件下无法探测到的流星体碎片细节。早些时候有人提出,对具有散射椭圆的星团的描述可以估计流星体的轨迹,这与撞击器的轨道参数有关。独立构造散射椭圆并与火山口喷出物进行比较,证明了该方法的准确性,并发现了该方法存在的一些问题。
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来源期刊
CiteScore
1.10
自引率
20.00%
发文量
4
审稿时长
>12 weeks
期刊介绍: Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.
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