Decimetre-scaled spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from OSIRIS observations
C. Feller, S. Fornasier, P.H. Hasselmann, A. Barucci, F. Preusker, F., Scholten, L. Jorda, A. Pommerol, H. Sierks, J. Agarwal, M. A'Hearn, J.-L., Bertaux, I. Bertini, S. Boudreault, G. Cremonese, V. Da Deppo, B.J.R., Davidsson, S. Debei, M. De Cecco, J. Deller, M. Fulle

TL;DR
This study analyzes the decimetre-scale spectrophotometric properties of comet 67P/Churyumov-Gerasimenko's nucleus using OSIRIS data from a close fly-by, revealing local heterogeneities, spectral variations, and photometric characteristics.
Contribution
First detailed decimetre-scale spectrophotometric analysis of 67P's nucleus using OSIRIS data, including modeling with Hapke 2008 to understand surface properties.
Findings
Reflectance differences up to 40% between bright and dark regions
Spectral slope variations up to 50% across the surface
Region has a geometric albedo of 6.8% and high porosity (86%)
Abstract
We present the results of the photometric and spectrophotometric properties of the 67P/Churyumov-Gerasimenko nucleus derived with the OSIRIS instrument during the closest fly-by over the comet, which took place on 14 th February 2015 at a distance of {\~} 6 km from the surface. Several images covering the 0{\deg}-33{\deg} phase angle range were acquired, and the spatial resolution achieved was 11 cm/pxl. The flown-by region is located on the big lobe of the comet, near the borders of the Ash, Apis and Imhotep regions. Our analysis shows that this region features local heterogeneities at the decimetre scale. We observed difference of reflectance up to 40{\%} between bright spots and sombre regions, and spectral slope variations up to 50{\%}. The spectral reddening effect observed globally on the comet surface by Fornasier et al. (2015) is also observed locally on this region, but with a…
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