小相位角下高浓度月球岩石三维模拟物的光散射

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Mingyeong Lee, Minsup Jeong, Young-Jun Choi
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引用次数: 0

摘要

月球碎屑由未固结的颗粒组成,具有高孔隙率,被称为 "仙女城堡结构"。它与月球反相效应密切相关,即当相角接近 0° ${}^{\circ}$ 时亮度急剧增加的效应。然而,由于地球引力的原因,在实验室中很难再现月球仙堡结构来研究其物理特性。我们设计了一种月球仙女城堡结构模型,用于三维打印。这些模型具有高孔隙率,并被简化为树状。我们考虑了表面的各种多孔条件,以树的数量、最大树干长度和最大树枝角度来表示。在本研究中,我们进行了一次实验室实验,在 1.4 ° ${}^{\circ}$ 到 5.0 ° ${}^{\circ}$ 的小相位角范围内测量了具有童话城堡结构的模拟物的反射率。结果分析了样品孔隙率与反射率 S ( α ) $(\α )$ 的切线斜率,后者表示对立效应的强度。此外,研究结果还与月球观测数据进行了比较。多孔样品的 S ( α ) $(\alpha )$ 值相对较大。在这项研究中,枝条长度和附着角度的影响非常微弱。孔隙度在 0.78 和 0.82 之间的样品代表了与月球观测数据相似的 S ( α ) $(\alpha )$ 值,即月球碎屑岩的平均孔隙度。总之,我们的研究结果表明,印刷样品中的孔隙度与对立效应之间存在潜在的相关性,为理解月球对立效应提出了一种新的研究方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Light Scattering From High-Porosity 3D Simulants of the Lunar Regolith at Small Phase Angles

Lunar regolith consists of unconsolidated grains with high porosity, called the fairy castle structure. It is closely linked to the lunar opposition effect, which is the effect where brightness sharply increases as the phase angle approaches 0 ° ${}^{\circ}$ . However, owing to the Earth's gravity, it is difficult to reproduce the structure to study the physical characteristics of the lunar fairy castle structure in the laboratory. We designed a lunar fairy castle structure model for 3D printing. These models had high porosity and were simplified to tree-like shapes. Various porous conditions of the surface were considered, represented by the number of trees, maximum trunk length, and maximum branch angle. In this study, a laboratory experiment was conducted to measure the reflectance of simulants with a fairy castle structure within a small phase angle range from 1.4 ° ${}^{\circ}$ to 5.0 ° ${}^{\circ}$ . The result is analyzed for the sample porosity with the tangential slope of the reflectance S ( α ) $(\alpha )$ , which denotes the strength of the opposition effect. In addition, the results of this study were compared with lunar observation data. The porous samples exhibited a relatively large S ( α ) $(\alpha )$ value. The influence of branch length and attachment angle was very weak in this study. Samples with a porosity between 0.78 and 0.82 represent the similar S ( α ) $(\alpha )$ values to the lunar observation data, a mean porosity of lunar regolith. In conclusion, our findings suggest a potential correlation between porosity and the opposition effect in printed samples, proposing a new research approach for understanding the lunar opposition effect.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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