用于行星土壤模拟物反射光谱分析的实验室设备--Exoland 模拟器:设计与模拟

Marco Dionigi, Silvia Logozzo, M. C. Valigi, Paola Comodi, Alessandro Pisello, Diego Perugini, M. Fastelli
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引用次数: 0

摘要

在行星科学中,可见光(Vis)和近红外(NIR)反射光谱可以通过比较遥感获取的数据和实验室参考数据来破译天体表面的化学/矿物成分。本文介绍了名为 "Exoland 模拟器 "的自动测试平台的设计,该平台配备了两台反射光谱仪,波长范围为 0.38-2.2 微米。它的设计目的是收集实验室制备的天然/合成岩石和矿物的数据,模拟行星表面的组成。测试台的结构设计为笛卡尔机器人,以实现自动采集。还通过模拟一些项目轨迹对测试装置进行了测试,并根据其再现编程轨迹的能力提供了测试结果。此外,还展示了初步的光谱数据,以说明土壤模拟物的光谱如何能够对材料进行准确的远程识别,从而能够创建库来研究多种化学物理成分变化对单个光谱带的影响。尽管 Exoland 的主要应用范围很广,但它也可用于摩擦学目的,通过分析磨损痕迹,将土壤和材料的磨损行为与其成分联系起来。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Exoland Simulator, a Laboratory Device for Reflectance Spectral Analyses of Planetary Soil Analogs: Design and Simulation
In planetary science, visible (Vis) and near-infrared (NIR) reflectance spectra allow deciphering the chemical/mineralogical composition of celestial bodies’ surfaces by comparison between remotely acquired data and laboratory references. This paper presents the design of an automated test rig named Exoland Simulator equipped with two reflectance spectrometers covering the 0.38–2.2 µm range. It is designed to collect data of natural/synthetic rocks and minerals prepared in the laboratory that simulate the composition of planetary surfaces. The structure of the test rig is conceived as a Cartesian robot to automatize the acquisition. The test rig is also tested by simulating some project trajectories, and results are presented in terms of its ability to reproduce the programmed trajectories. Furthermore, preliminary spectral data are shown to demonstrate how the soil analogs’ spectra could allow an accurate remote identification of materials, enabling the creation of libraries to study the effect of multiple chemical–physical component variations on individual spectral bands. Despite the primary scope of Exoland, it can be advantageously used also for tribological purposes, to correlate the wear behavior of soils and materials with their composition by also analyzing the wear scars.
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