Experimental investigation of impact close to the edge of boulders

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Toshihiko Kadono , Akiko M. Nakamura , Ryo Suetsugu , Daehyo Chang , Seiya Shiramizu , Issei Takatsu , Koki Ogawa , Keita Nomura , Yuuya Nagaashi , Yuichi Murakami , Yutaro Yamasaki , Junpei Shiomoto , Takaya Okamoto , Shigeru Tanaka , Nobuaki Kawai
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Abstract

Asteroid exploration has allowed detailed observations of boulders on the surface and measurements of craters on the boulders. We focused on the craters near the edges of the boulders and investigated the distance from the impact point to the side surfaces of finite-sized brittle targets when spallation of the side surfaces occurred. First, impact cratering data was compiled, including previous and newly conducted experiments on porous gypsum and less-porous basalt targets. When the distance from the edge to the impact point was shorter than approximately twice the crater radius, spallation of the side surfaces occurred, irrespective of the target material. Then, explosion experiments were conducted using porous gypsum targets to elucidate the physical mechanisms of this process. We investigated the relationship between the distance from the explosion point to the free surface and the incident angle of the stress waves relative to the free surface when spallation occurs. Experimental results suggest that spallation at the side surfaces occurs when the amplitude of the reflected wave caused by a stress wave incident perpendicular to the side surfaces is greater than that at the rim of the crater formed on the top surface. The quantitative relationships obtained in this study using both porous gypsum and less-porous basalt will help to constrain the history of cratered boulders with a wide variety of porosities on asteroids.

冲击接近巨石边缘的实验研究
对小行星的探索可以对表面的巨石进行详细的观察,并对巨石上的陨石坑进行测量。我们将重点放在巨石边缘附近的陨石坑上,并研究了在侧面发生碎裂时,从撞击点到有限尺寸脆性目标侧面的距离。首先,收集了撞击坑的数据,包括以前和新进行的多孔石膏和低多孔玄武岩目标的实验。当从边缘到撞击点的距离小于大约两倍的陨石坑半径时,不管目标材料是什么,侧壁都会发生剥落。然后,利用多孔石膏靶进行了爆炸实验,阐明了这一过程的物理机制。我们研究了爆炸点到自由表面的距离与发生裂裂时应力波相对于自由表面的入射角之间的关系。实验结果表明,当垂直于侧面入射的应力波反射波的振幅大于顶面形成的弹坑边缘的波幅时,侧面发生裂裂。本研究使用多孔石膏和多孔玄武岩获得的定量关系将有助于限制小行星上具有各种孔隙度的陨石坑巨石的历史。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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