{"title":"Experimental investigation of impact close to the edge of boulders","authors":"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","doi":"10.1016/j.pss.2023.105763","DOIUrl":null,"url":null,"abstract":"<div><p><span><span>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 </span>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 </span>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.</p></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"236 ","pages":"Article 105763"},"PeriodicalIF":1.8000,"publicationDate":"2023-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0032063323001320","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
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.
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