利用陨石类似物的反射光谱评价小行星的物质组成

Savelova A. A., Busarev V. V., Shcherbina M. P.
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引用次数: 0

摘要

开发了估算小行星物质组成的MATLAB程序。该程序利用陨石类似物的反射光谱来模拟小行星的反射光谱。讨论了10颗小行星(1颗谷神星,4颗灶神星,51颗Nemausa, 65颗Cybele, 102颗Miriam, 250颗Bettina, 266颗Aline, 379颗Huenna, 704颗Interamnia, 1474颗Beira)的建模结果和物质组成估算。许多小行星(1颗谷神星,4颗灶神星,51颗Nemausa, 250颗Bettina, 704颗Interamnia)的模型光谱与反射率光谱吻合较好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evaluation of the asteroid material composition by reflectance spectra using meteorite analogues
The MATLAB program was developed to estimate composition of the asteroid material. The program models reflectance spectra of asteroids using reflectance spectra of meteorite analogues. Modeling results and estimation of the material composition for 10 asteroids (1 Ceres, 4 Vesta, 51 Nemausa, 65 Cybele, 102 Miriam, 250 Bettina, 266 Aline, 379 Huenna, 704 Interamnia, 1474 Beira) are discussed. A good agreement between the model spectra and the asteroids reflectance spectra is achieved for a number of asteroids (1 Ceres, 4 Vesta, 51 Nemausa, 250 Bettina, 704 Interamnia)
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