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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:最后的菲莱着陆点的特写镜头图象彗星的   67p / Churyumov-Gerasimenko被ROLIs相机收购

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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 thesurface below the lander, four of which were with the aid of LED illuminationof different colors. The images confirm that Philae was perched on a slopedsurface. A local horizon is visible in one corner of the image, beyond which wecan see the coma. Having spent a full day on the surface Philae was commandedto lift and rotate, after which a final, sixth, LED image was acquired. Thechange in perspective allowed us to construct a shape model of the surface. Thedistance 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 dominatethe image signal, complicating the analysis. The images show a lumpy surfacewith a roughness of apparently fractal nature. Its appearance is completelydifferent from that of the first landing site, which was characterized bycentimeter to meter-sized debris (Mottola et al., 2015). We recognize neitherparticles nor pores at the image resolution of 0.8 mm per pixel and large colorvariations are absent. The surface has a bi-modal brightness distribution thatcan be interpreted in terms of the degree of consolidation, a hypothesis thatwe support with experimental evidence. We propose the surface below the landerto consist of smooth, cracked plates with unconsolidated edges, similar toterrain 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,其中四幅借助于不同颜色的LED照明。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。在地面上待了整整一天后,命令Philae抬起并旋转,此后获得了最后的第六张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,使分析变得复杂。图像显示块状表面具有明显的分形性质。它的外观与第一个登陆点的外观完全不同,后者的特征是厘米到米大小的碎片(Mottola等人,2015)。我们认识到每像素0.8毫米的图像分辨率既没有微粒也没有气孔,并且没有大的颜色变化。表面具有双峰亮度分布,可以用固结度来解释,这一假设得到了实验证据的支持。我们建议在Landerto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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