{"title":"月球伊纳不规则赤铁矿斑块(IMP)的撞击陨石坑:关于撞击多孔玄武岩基质性质的实验证据和悬而未决的问题","authors":"James W. Head , Boris Ivanov","doi":"10.1016/j.pss.2024.105954","DOIUrl":null,"url":null,"abstract":"<div><p>The enigma of the apparently young crater retention age for the large lunar volcanic Irregular Mare Patch Ina (∼33.2 Myr) is critically analyzed through the review of: 1) experimental data on high velocity impacts into porous targets, 2) observed small impact crater morphology, and 3) the possible variation in small impact crater morphology with age. While we find that these different data sets and approaches could not unequivocally resolve the enigma, our analysis provides directions for new studies in several disciplines that are designed to help resolve the age conundrum and improve upcoming exploration mission goals and objectives.</p></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"250 ","pages":"Article 105954"},"PeriodicalIF":1.8000,"publicationDate":"2024-08-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Impact cratering at the lunar Ina irregular mare patch (IMP): Experimental evidence for the nature of impacts into porous basaltic substrate and outstanding questions\",\"authors\":\"James W. Head , Boris Ivanov\",\"doi\":\"10.1016/j.pss.2024.105954\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The enigma of the apparently young crater retention age for the large lunar volcanic Irregular Mare Patch Ina (∼33.2 Myr) is critically analyzed through the review of: 1) experimental data on high velocity impacts into porous targets, 2) observed small impact crater morphology, and 3) the possible variation in small impact crater morphology with age. While we find that these different data sets and approaches could not unequivocally resolve the enigma, our analysis provides directions for new studies in several disciplines that are designed to help resolve the age conundrum and improve upcoming exploration mission goals and objectives.</p></div>\",\"PeriodicalId\":20054,\"journal\":{\"name\":\"Planetary and Space Science\",\"volume\":\"250 \",\"pages\":\"Article 105954\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2024-08-12\",\"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/S0032063324001181\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0032063324001181","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}
Impact cratering at the lunar Ina irregular mare patch (IMP): Experimental evidence for the nature of impacts into porous basaltic substrate and outstanding questions
The enigma of the apparently young crater retention age for the large lunar volcanic Irregular Mare Patch Ina (∼33.2 Myr) is critically analyzed through the review of: 1) experimental data on high velocity impacts into porous targets, 2) observed small impact crater morphology, and 3) the possible variation in small impact crater morphology with age. While we find that these different data sets and approaches could not unequivocally resolve the enigma, our analysis provides directions for new studies in several disciplines that are designed to help resolve the age conundrum and improve upcoming exploration mission goals and objectives.
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