The Relationship between Cone Penetration Resistance and Wheel-Soil Interactions in Lunar Gravity

Adriana Daca, D. Tremblay, K. Skonieczny
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引用次数: 2

Abstract

One of the major challenges faced by planetary exploration rovers today is the negotiation of difficult terrain, such as fine granular regolith commonly found on the Moon and Mars. Typical Earth-based testing methods cannot accurately predict rover mobility in reduced gravity environments (i.e. the Moon and Mars) as they fail to account for the effect of reduced gravity on the soil itself. Preliminary efforts have been made to account for effects of gravity on granular materials, at least indirectly, through simulant design. The soil simulant GRC-1 is designed to produce cone penetrometer readings comparable to those collected on the Moon (i.e. in lunar gravity) during Apollo. The assumption is that replicating the mechanical properties of lunar soil in terms of cone penetration resistance will also replicate the response to vehicle loading in terms of traction. The present research was designed to thoroughly characterize this assumption by exploring the relationship between rover mobility and cone penetration resistance experimentally in lunar gravity (1/6-g) and terrestrial gravity (1-g). The cone penetrometer response of GRC-1 was measured at relative densities (DR'S) of 46%,63%, and 69 % in both 1-g and 1/6-g aboard parabolic flights producing effective lunar gravitational accelerations. Cone index gradient (G) values measured in 1/6-g were 4 x lower on average than those measured in 1-g, indicating a significant decrease in shear strength in lunar-g. Wheel-soil interactions between a smooth rigid wheel and G R C-1 were also characterized at 69% DR in 1/6-g. The wheel experiments measured wheel-soil interaction data at controlled slip values of 20 % and 70 %. Wheel-soil interaction data collected include subsurface soil imaging, force/torque sensor data, wheel sinkage, and motor current, with drawbar pull (DP) and sinkage data reported here. Average DP/W values observed at 20% slip and 70% slip were 0.11 ± 0.02 and 0.32 ± 0.03, respectively, and maximum observed sinkage was 9.0 ± 1.9 mm and 16.2 ± 2.1 mm at 20% and 70 % slip, respectively. These results will be compared to 1-g experiments in a lower-density soil that produces an equivalent cone penetrometer response in order to test the hypothesis that equivalent wheel performance will be observed in soil with equal G values across differing gravity levels.
月球重力下锥体穿透阻力与轮土相互作用的关系
如今,行星探测漫游者面临的主要挑战之一是通过困难的地形,比如在月球和火星上常见的细颗粒风化层。典型的基于地球的测试方法无法准确预测月球车在失重环境(即月球和火星)下的机动性,因为它们无法考虑失重对土壤本身的影响。通过模拟设计,已经做出了初步的努力来解释重力对颗粒材料的影响,至少是间接的。土壤模拟GRC-1的设计目的是产生与阿波罗期间在月球上收集的(即月球重力)相媲美的锥贯仪读数。我们的假设是,复制月球土壤在锥体穿透阻力方面的力学特性,也将复制车辆加载在牵引力方面的反应。本研究旨在通过在月球重力(1/6-g)和地球重力(1-g)下实验探索月球车机动性与锥体穿透阻力之间的关系,彻底表征这一假设。在产生有效月球重力加速度的抛物线飞行中,在相对密度为46%、63%和69%的情况下,测量了GRC-1的锥形穿透仪响应。在1/6-g中测得的锥指数梯度(G)值比在1-g中测得的值平均低4倍,表明在月球- G中抗剪强度显著降低。光滑刚性车轮与G R C-1之间的轮-土相互作用在1/6 G中也具有69%的DR。车轮试验在控制滑移值为20%和70%时测量了轮-土相互作用数据。收集的车轮-土壤相互作用数据包括地下土壤成像、力/扭矩传感器数据、车轮下沉和电机电流,并报告了牵引力(DP)和下沉数据。滑移率为20%和70%时的平均DP/W分别为0.11±0.02和0.32±0.03,滑移率为20%和70%时的最大沉降分别为9.0±1.9 mm和16.2±2.1 mm。这些结果将与在低密度土壤中进行的1-g实验进行比较,该实验产生等效锥体穿透仪响应,以验证在不同重力水平下具有相同G值的土壤中观察到等效车轮性能的假设。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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