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The SMART-1 Mission: Photometric Studies of the Moon with the AMIE Camera

机译：SMART-1任务：使用AMIE相机进行月球光度研究

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摘要

We describe the future SMART-1 European Space Mission whose objective is to study the lunar surface from a polar lunar orbit. In particular, it is anticipated that selected regions of the Moon will be photographed using the AMIE camera with a mean spatial resolution of about 100 m in three spectral channels (0.75, 0.92, and 0.96 μm) over a wide range of phase angles. Since these spectral channels and the AMIE resolution are close to those of the UVVIS camera onboard the Clementine spacecraft, the simultaneous processing of SMART-1 and Clementine data can be planned, for example, to obtain phase-ratio images. These images carry information on the structural features of the lunar surface. In particular, UVVIS/Clementine data revealed a photometric anomaly at the Apollo-15 landing site associated with the blowing of the lunar regolith by the lander engine. Anomalies were found in the ejection zones of several fresh craters.
机译：我们描述了未来的SMART-1欧洲太空任务，其目的是从极地月球轨道研究月球表面。特别是，预计将使用AMIE相机在较宽的相角范围内的三个光谱通道（0.75、0.92和0.96μm）中以平均空间分辨率约为100 m拍摄月球的选定区域。由于这些光谱通道和AMIE分辨率接近于Clementine航天器上的UVVIS相机，因此可以计划同时处理SMART-1和Clementine数据，例如以获得相位比图像。这些图像带有有关月球表面结构特征的信息。特别是，UVVIS / Clementine数据显示，阿波罗15号着陆点的光度学异常与着陆器吹月球重石有关。在几个新的陨石坑的弹射区发现异常。

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