首页> 外文会议>International Astronautical Congress >SPACE EXPLORATION SYMPOSIUM (A3) Moon Exploration - Poster session (2D):A NEW MODEL TO PREDICT THE WORN SURFACES OF LUNAR EXPLORERS CAUSED BY PARTICLE COLLISION IN SPACE ENVIRONMENT
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SPACE EXPLORATION SYMPOSIUM (A3) Moon Exploration - Poster session (2D):A NEW MODEL TO PREDICT THE WORN SURFACES OF LUNAR EXPLORERS CAUSED BY PARTICLE COLLISION IN SPACE ENVIRONMENT

机译:太空勘探研讨会(A3)月亮探索 - 海报会话(2D):预测空间环境中的粒子碰撞引起的月探险勘探器磨损的新模型

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When lunar explorers working on the moon, wear caused by frequent collision of the particles such as settled dust, regolith and gravel on the machine surfaces always exist. Usually, the energy consumed by the particle collision is considered as a factor heavily determining the volume of material peeled off. So a new model is proposed in this paper to formulate the relationship between the collision energy and the worn volume of the machine surfaces based on the discrete element method (DEM) which can precisely detect contacts and calculate the collision energy between individual particles and surfaces. When the surfaces of the CAD model of an explorer are partitioned into rigid triangles linked with each other through their vertices, the wear prediction model can applied to each triangle. The collision energy dissipated in a triangle can be used to compute the worn volume on this triangle and further to know its change to height on the wearing direction. Through recalculating the positions according to the new heights of triangles and surface fitting for all triangles, the geometries of the worn surfaces can be visually presented. In order to verify this prediction model, a lugged wheel of the lunar exploration rover is selected as the worn component to interact with the lunar regolith simulant of spherical particles in microgravity. From the comparison between the simulation results and the photos of a real worn wheel of a test rover, one can see that the proposed model is able to effectively predict the main geometrical characteristics of the worn surfaces of explorers on the moon.
机译:当农历探险家在月球上工作时,磨损造成的颗粒频繁碰撞,如机械表面上的沉降灰尘,石头和砾石总是存在。通常,颗粒碰撞所消耗的能量被认为是严重确定剥离的材料体积的因素。因此,在本文中提出了一种新模型,以基于可以精确地检测接触并计算各个颗粒和表面之间的碰撞能量的离散元件方法(DEM)来制定碰撞能量和机器表面的磨损体积之间的关系。当探险器的CAD模型的表面被划分为通过其顶点彼此连接的刚性三角形时,磨损预测模型可以应用于每个三角形。在三角形中消散的碰撞能量可用于计算在该三角形上的磨损体积,并进一步知道其在磨损方向上的高度变化。通过根据所有三角形的三角形和表面配件的新高度重新计算位置,可以在视觉上呈现磨损表面的几何形状。为了验证这种预测模型,选择了月球探测器的镂空轮作为磨损的组分,以与微匍匐度的球形颗粒的月球颗粒模拟物相互作用。从模拟结果与真正磨损轮的照片之间的比较来看,可以看到所提出的模型能够有效地预测月球上探险探险器的磨损表面的主要几何特征。

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