Chelyabinsk Meteorite

O. Popova
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引用次数: 5

Abstract

The asteroid impact near the Russian city of Chelyabinsk on February 15, 2013, was the largest airburst on Earth since the 1908 Tunguska event, causing a natural disaster in an area with a population exceeding 1 million. On clear morning at 9:20 a.m. local time, an asteroid about 19 m in size entered the Earth atmosphere near southern Ural Mountains (Russia) and, with its bright illumination, attracted the attention of hundreds of thousands of people. Dust trail in the atmosphere after the bolide was tens of kilometers long and was visible for several hours. Thousands of different size meteorites were found in the areas south-southwest of Chelyabinsk. A powerful airburst, which was formed due to meteoroid energy deposition, shattered thousands of windows and doors in Chelyabinsk and wide surroundings, with flying glass injuring many residents. The entrance and destruction of the 500-kt Chelyabinsk asteroid produced a number of observable effects, including light and thermal radiation; acoustic, infrasound, blast, and seismic waves; and release of interplanetary substance. This unexpected and unusual event is the most well-documented bolide airburst, and it attracted worldwide attention. The airburst was observed globally by multiple instruments. Analyses of the observational data allowed determination of the size of the body that caused the superbolide, its velocity, its trajectory, its behavior in the atmosphere, the strength of the blast wave, and other characteristics. The entry of the 19-m-diameter Chelyabinsk asteroid provides a unique opportunity to calibrate the different approaches used to model meteoroid entry and to calculate the damaging effects. The recovered meteorite material was characterized as brecciated LL5 ordinary chondrite, in which three different lithologies can be distinguished (light-colored, dark-colored, and impact-melt). The structure and properties of meteorites demonstrate that before encountering Earth, the Chelyabinsk asteroid had experienced a very complex history involving at least a few impacts with other bodies and thermal metamorphism. The Chelyabinsk airburst of February 15, 2013, was exceptional because of the large kinetic energy of the impacting body and the damaging airburst that was generated. Before the event, decameter-sized objects were considered to be safe. With the Chelyabinsk event, it is possible, for the first time, to link the damage from an impact event to a well-determined impact energy in order to assess the future hazards of asteroids to lives and property.
2013年2月15日,俄罗斯车里雅宾斯克市附近的小行星撞击,是自1908年通古斯事件以来地球上最大的一次空中爆炸,在一个人口超过100万的地区造成了自然灾害。在一个晴朗的早晨,当地时间上午9点20分,一颗直径约19米的小行星在俄罗斯南部乌拉尔山脉附近进入地球大气层,明亮的灯光吸引了数十万人的注意。流星后大气中的尘埃轨迹长达数十公里,持续数小时可见。在车里雅宾斯克西南偏南地区发现了数千颗不同大小的陨石。由于流星体能量沉积而形成的强大空中爆炸,粉碎了车里雅宾斯克及周边地区数千扇门窗,飞溅的玻璃伤及许多居民。500吨的车里雅宾斯克小行星的进入和破坏产生了许多可观察到的影响,包括光辐射和热辐射;声波、次声波、冲击波和地震波;以及星际物质的释放。这一意外和不寻常的事件是记录最充分的火流星空爆事件,引起了全世界的关注。这次空爆在全球由多个仪器观测到。对观测数据的分析可以确定产生超级流星的物体的大小、速度、轨迹、在大气中的行为、冲击波的强度和其他特征。直径19米的车里雅宾斯克小行星的进入为校准用于模拟流星体进入和计算破坏性影响的不同方法提供了一个独特的机会。回收的陨石材料被表征为角砾LL5普通球粒陨石,其中可以区分出三种不同的岩性(浅色,深色和冲击熔融)。陨石的结构和性质表明,在与地球相遇之前,车里雅宾斯克小行星经历了一段非常复杂的历史,至少与其他天体发生了几次撞击,并发生了热变质作用。2013年2月15日的车里雅宾斯克空爆,由于撞击体的巨大动能和产生的破坏性空爆,是一个例外。在此之前,十米大小的物体被认为是安全的。通过车里雅宾斯克事件,首次有可能将撞击事件造成的损害与确定的撞击能量联系起来,以便评估小行星对生命和财产的未来危害。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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