摘要
本文选取3种类型的陨石分别进行脉冲激光辐照实验,模拟距离太阳1个天文单位(1 AU)处,10亿年(1 Ga)期间微陨石轰击的太空风化作用对E型、S型、C群等近地小行星光谱特征的改造。结果显示,激光辐照后,顽辉石无球粒陨石光谱的可见光波段反射率降低且近红外斜率增加,与E型小行星光谱改造特征一致;普通球粒陨石的可见光-近红外波段反射率均降低、吸收深度变浅且近红外斜率增加,与S型小行星光谱改造特征一致;CV3型碳质球粒陨石和CO3型碳质球粒陨石在激光辐照后可见光波段反射率降低,但近红外波段反射率升高,吸收深度变浅且近红外斜率增加,与贫挥发分的C群小行星光谱改造特征一致;CM2碳质陨石在激光辐照后,可见光波段反射率增加,但近红外波段反射率及近红外斜率降低,与富挥发分的C群小行星光谱改造特征一致。研究结果可为近地小行星探测任务备选目标的确定、光谱遥感数据以及表面物质演化过程的反演提供一定的参考。
In this paper,three types of meteorites were selected to have been undertaken pulse laser irradiation experiments for simulating the alteration effects on spectra of E-,M-,and C-group Near-Earth Asteroids by the space weathering resulted from the micrometeorite impact on their surfaces at an assumed place of 1 astronomical unit(1 AU)away from the Sun for 1 billion years(1 Ga).The results show that the laser irradiated aubrite has relatively low reflectivity of visible band but relatively high slope of near-infrared band in its spectrum,which is consistent with that of the weathered E-type asteroid. The ordinary chondrite has relatively low reflectivity of visible and near-infrared bands,relatively shallowadsorption but relatively high slope of near-infrared band in its spectrum,which is consistent with that of the weatheredS-type asteroid. The laser irradiated CV3 and CO3 carbonaceous chondrites have relatively low reflectivity of visibleband but high reflectivity of near-infrared band,relatively shallow adsorption but high slope of near-infrared band intheir spectra,which are consistent with that of the weathered volatile-poor C-group asteroid. The laser irradiated CM2carbonaceous chondrite has relatively high reflectivity of visible band but relative low reflectivity and slope of near-infraredband in its spectrum,which is consistent with that of the weathered volatile-rich C-group asteroid. The research mayprovide a certain reference and support for choosing suitable asteroid as target for the future Near-Earth Asteroid explorationmission,interpreting spectral remote sensing data,and understanding the evolution process of asteroid surface materials.
作者
张鹏飞
张江
李世杰
刘长卿
文愿运
孙浩
李阳
ZHANG Peng-fei;ZHANG Jiang;LI Shi-jie;LIU Chang-qing;WEN Yuan-yun;SUN Hao;LI Yang(Center for Lunar and Planetary Sciences,Institute of Geochemistry,Chinese Academy of Sciences,Guiyang 550081,China;Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,Institute of Space Science,Shandong University,Weihai Shandong 264209,China;State Key Laboratory of Lunar and Planetary Sciences,Macao University of Science and Technology,Macao 519020,China;College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,Beijing 100049,China;Key Laboratory of Earth and Planetary Physics,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China;Department of Geology,Northwest University,Xi'an 710069,China)
出处
《矿物岩石地球化学通报》
CAS
CSCD
北大核心
2020年第4期853-862,共10页
Bulletin of Mineralogy, Petrology and Geochemistry
基金
澳门科技大学开放基金资助项目(039/2013/A2)
中国科学院地球与行星物理重点实验室开放课题
国家自然科学基金资助项目(41673071,41931077)。
关键词
小行星
太空风化
反射光谱
陨石
纳米铁
挥发分
asteroids
space weathering
reflectance spectrum
meteorites
nanophase iron
volatiles