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Close-up images of the final Philae landing site on comet 67P/Churyumov-Gerasimenko acquired by the ROLIS camera

机译:ROLIS相机获得的67P / Churyumov-Gerasimenko彗星最终菲莱登陆点的特写照片

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摘要

After coming to rest on the night side of comet 67P/Churyumov-Gerasimenko, the ROLIS camera on-board Rosetta’s Philae lander acquired five images of the surface below the lander, four of which were with the aid of LED illumination of different colors. The images confirm that Philae was perched on a sloped surface. A local horizon is visible in one corner of the image, beyond which we can see the coma. Having spent a full day on the surface Philae was commanded to lift and rotate, after which a final, sixth, LED image was acquired. The change in perspective allowed us to construct a shape model of the surface. The distance to the foreground was about 80 cm, much larger than the nominal 30 cm. This caused stray light, rather than directly reflected LED light, to dominate the image signal, complicating the analysis. The images show a lumpy surface with a roughness of apparently fractal nature. Its appearance is completely different from that of the first landing site, which was characterized by centimeter to meter-sized debris (Mottola et al., 2015). We recognize neither particles nor pores at the image resolution of 0.8 mm per pixel and large color variations are absent. The surface has a bi-modal brightness distribution that can be interpreted in terms of the degree of consolidation, a hypothesis that we support with experimental evidence. We propose the surface below the lander to consist of smooth, cracked plates with unconsolidated edges, similar to terrain seen in CIVA images.
机译:在67P / Churyumov-Gerasimenko彗星的夜间休息后,罗塞塔的Philae着陆器上的ROLIS摄像头获得了着陆器下方表面的五幅图像,其中四幅是借助不同颜色的LED照明获得的。图像确认Philae栖息在倾斜的表面上。在图像的一个角处可见局部水平线,超出该水平线我们可以看到昏迷。在地面上花了整整一天的时间后,Philae被命令抬起并旋转,此后获得了第六张LED图像。视角的变化使我们能够构建表面的形状模型。到前景的距离约为80厘米,比标称的30厘米大得多。这导致杂散光而不是直接反射的LED光在图像信号中占主导地位,从而使分析变得复杂。图像显示块状表面具有明显的分形性质。它的外观与第一个着陆点完全不同,后者的特征是厘米到米大小的碎片(Mottola等人,2015)。我们在每像素0.8毫米的图像分辨率下既没有颗粒也没有孔,而且没有大的颜色变化。该表面具有双峰亮度分布,可以用固结度来解释,这是我们得到实验证据支持的假设。我们建议着陆器下方的表面由光滑,破裂且边缘不固结的板块组成,类似于CIVA图像中看到的地形。

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