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Shape of (101955) Bennu indicative of a rubble pile with internal stiffness

机译:(101955)Bennu表示具有内刚度的瓦砾桩

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The shapes of asteroids reflect interplay between their interior properties and the processes responsible for their formation and evolution as they journey through the Solar System. Prior to the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) mission, Earth-based radar imaging gave an overview of (101955) Bennu's shape. Here we construct a high-resolution shape model from OSIRIS-REx images. We find that Bennu's top-like shape, considerable macroporosity and prominent surface boulders suggest that it is a rubble pile. High-standing, north-south ridges that extend from pole to pole, many long grooves and surface mass wasting indicate some low levels of internal friction and/or cohesion. Our shape model indicates that, similar to other top-shaped asteroids, Bennu formed by reaccumulation and underwent past periods of fast spin, which led to its current shape. Today, Bennu might follow a different evolutionary pathway, with an interior stiffness that permits surface cracking and mass wasting.
机译:小行星的形状反映了它们的内部性质与负责它们的形成和演进的过程之间的相互作用。在Osiris-rex(起源,光谱解释,资源识别和安全regolith Explorer)之前,基于地球的雷达成像概述了(101955)Bennu形状。在这里,我们从Osiris-rex图像构造一个高分辨率形状模型。我们发现Bennu的顶部形状,相当大的宏观度和突出的表面巨石表明它是一种瓦砾堆。高位北方南部沿杆延伸到杆,许多长的凹槽和表面质量浪费表示一些低水平的内部摩擦和/或内聚力。我们的形状模型表明,类似于其他顶形的小行星,通过ReaCrumulation形成的Bennu,并且经历了过去的快速旋转时段,导致其当前的形状。如今,Bennu可能遵循不同的进化途径,内部刚度允许表面开裂和批量浪费。

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