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首页> 外文期刊>Icarus: International Journal of Solar System Studies >Variability, absorption features, and parent body searches in 'spectrally featureless' meteorite reflectance spectra: Case study - Tagish Lake
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Variability, absorption features, and parent body searches in 'spectrally featureless' meteorite reflectance spectra: Case study - Tagish Lake

机译:在“无光谱特征”的陨石反射光谱中的可变性,吸收特征和母体搜索:案例研究-Tagish Lake

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摘要

Reflectance spectra of many asteroids and other Solar System bodies are commonly reported as "featureless". Here, we show that weak but consistently detectable absorption bands are observable in 200-2500 nm spectra of the Tagish Lake meteorite, a likely compositional and spectral analogue for low-albedo, "spectrally-featureless" asteroids. Tagish Lake presents a rare opportunity to study multiple lithologies within a single meteorite. Reflectance spectra of Tagish Lake display significant variation between different lithologies. The spectral variations are due in part to mineralogical variations between different Tagish Lake lithologies. Ultraviolet reflectance spectra (200-400 nm), few of which have been reported in the literature to date, reveal albedo and spectral ratio variations as a function of mineralogy. Similarly visible-near infrared reflectance spectra reveal variations in albedo, spectral slope, and the presence of weak absorption features that persist across different lithologies and can be attributed to various phases present in Tagish Lake. These observations demonstrate that significant spectral variability may exist between different lithologies of Tagish Lake, which may affect the interpretation of potential source body spectra. It is also important to consider the spectral variability within the meteorite before excluding compositional links between possible parent bodies in the main belt and Tagish Lake. Tagish Lake materials may also be spectral-compositional analogues for materials on the surfaces of other dark asteroids, including some that are targets of upcoming spacecraft missions. Tagish Lake has been proposed as a spectral match for 'ultra-primitive' D or P-type asteroids, and the variability reported here may be reflected in spatially or rotationally-resolved spectra of possible Tagish Lake parent bodies and source objects in the Near-Earth Asteroid population. A search for objects with spectra similar to Tagish Lake has been carried out among the Near-Earth Asteroids. We have identified three possible spectral matches, the best of which are Asteroids (326732) 2003 HB6, and (17274) 2000 LC16. (C) 2015 Elsevier Inc. All rights reserved.
机译:许多小行星和其他太阳系物体的反射光谱通常被报告为“无特征”。在这里,我们显示出在塔吉什湖陨石的200-2500 nm光谱中观察到了微弱但始终可检测到的吸收带,这是低反照率,“无光谱特征”的小行星的可能的成分和光谱类似物。塔吉什湖为在单个陨石中研究多种岩性提供了难得的机会。塔吉西湖的反射光谱显示出不同岩性之间的显着差异。光谱变化部分归因于不同塔吉什湖岩性之间的矿物学变化。紫外反射光谱(200-400 nm)迄今尚未在文献中报道过,它揭示了反照率和光谱比变化是矿物学的函数。类似的可见-近红外反射光谱揭示了反照率,光谱斜率的变化以及弱吸收特征的存在,这些特征在不同岩性中持续存在,并且可以归因于塔吉什湖中存在的不同相。这些观察结果表明,塔吉什湖的不同岩性之间可能存在明显的光谱变异性,这可能会影响潜在源体光谱的解释。在排除主带和塔吉什湖可能的母体之间的成分联系之前,考虑陨石内部的光谱变异性也很重要。塔吉什湖的物质也可能是其他暗小行星表面物质的光谱组成类似物,其中包括一些即将进行的航天器飞行任务的目标。塔吉什湖已被提议作为“超原始” D或P型小行星的光谱匹配,此处报道的变异性可能反映在塔吉什湖母体和近地中源物体的空间或旋转分辨谱中。地球小行星人口。在近地小行星中搜寻了具有类似于塔吉什湖光谱的物体。我们确定了三种可能的光谱匹配,其中最好的是小行星(326732)2003 HB6和(17274)2000 LC16。 (C)2015 Elsevier Inc.保留所有权利。

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