Space Weathering Change of Grain Surfaces using Meteorite Tests and Related Possible Consequences on Asteroid Properties

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. Kereszturi, I. Gyollai, S. Biri, Z. Juhász, Cs. Király, R. Rácz, D. Rezes, B. Sulik, M. Szabó, Z. Szalai, P. Szávai
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Abstract

Compositional and structural understanding of asteroids, especially the moderately small (and frequent) Near Earth Asteroids is important not only for science but also for possible mitigation against their any future impact. However, space weathering substantially modifies the surface infrared spectra, making it difficult to identify their composition. Laboratory tests of artificial weathering by simulated solar wind on meteorites were conducted and reviewed in this study. During the simulations, an increase in the iron content, amorphization, water loss and other structural changes were observed, which usually decreases the mechanical hardness of the very thin surface layer. Using these results, the question was formulated and evaluated here: could such surface changes influence the joint behavior of grain groups when effects driven by YORP forces modify the global shape of asteroids. Based on the evaluation, 10–100 million years of time scale changes are expected to occur both mineral structure and global asteroid shape. The related theoretical consequences and research questions are summarized here.

Abstract Image

利用陨石试验研究颗粒表面的空间风化变化及其对小行星特性的可能影响
了解小行星的成分和结构,特别是中等大小(和频繁)的近地小行星,不仅对科学很重要,而且对可能减轻它们未来的影响也很重要。然而,空间风化极大地改变了表面红外光谱,使其难以确定其组成。本文进行了模拟太阳风对陨石进行人工风化的室内试验,并进行了综述。在模拟过程中,观察到铁含量增加、非晶化、失水和其他结构变化,这些变化通常会降低极薄表面层的机械硬度。利用这些结果,在这里提出并评估了一个问题:当YORP力驱动的效应改变了小行星的整体形状时,这种表面变化是否会影响颗粒群的联合行为?根据评估,预计矿物结构和全球小行星形状将发生1000万年至1亿年的时间尺度变化。本文总结了相关的理论结果和研究问题。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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