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Spatially resolved Spectroscopy of Europa's Large-scale Compositional Units at 3–4 μm with Keck NIRSPEC

机译:欧凯巴(Keck NIRSPEC)在3-4μm处的欧罗巴大型组成单位的空间分辨光谱

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摘要

We present spatially resolved spectroscopic observations of Europa's surface at 3–4 μm obtained with the near-infrared spectrograph and adaptive optics system on the Keck II telescope. These are the highest quality spatially resolved reflectance spectra of Europa's surface at 3–4 μm. The observations spatially resolve Europa's large-scale compositional units at a resolution of several hundred kilometers. The spectra show distinct features and geographic variations associated with known compositional units; in particular, large-scale leading hemisphere chaos shows a characteristic longward shift in peak reflectance near 3.7 μm compared to icy regions. These observations complement previous spectra of large-scale chaos, and can aid efforts to identify the endogenous non-ice species.
机译:我们介绍了通过近红外光谱仪和Keck II望远镜上的自适应光学系统获得的欧罗巴表面在3-4μm处的空间分辨光谱观察结果。这些是欧罗巴表面在3-4μm处质量最高的空间分辨反射光谱。这些观测结果以数百公里的分辨率在空间上解析了欧罗巴的大型组成单位。光谱显示与已知组成单位相关的明显特征和地理变化;尤其是,与冰冷地区相比,大规模的前半球混乱显示出峰值反射率在3.7μm附近出现了特征性的长距离偏移。这些观察结果补充了以前的大规模混沌光谱,可以帮助确定内生非冰种。

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