The highly active Anhur–Bes regions in the 67P/Churyumov–Gerasimenko comet: results from OSIRIS/ROSETTA observations

Fornasier, S.; Feller, C.; Lee, J.-C.; Ferrari, S.; Massironi, M.; Hasselmann, P. H.; Deshapriya, J. D. P.; Barucci, M. A.; Elmaarry, Mohamed Ramy; Giacomini, L.; Mottola, S.; Keller, H. U.; Ip, W.-H.; Lin, Z.-Y.; Sierks, H.; Barbieri, C.; Lamy, P. L.; Rodrigo, Rafael; Koschny, D.; Rickman, H.; ... (2017). The highly active Anhur–Bes regions in the 67P/Churyumov–Gerasimenko comet: results from OSIRIS/ROSETTA observations. Monthly notices of the Royal Astronomical Society, 469(Suppl_2), S93-S107. Oxford University Press 10.1093/mnras/stx1275

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The Southern hemisphere of the 67P/Churyumov–Gerasimenko comet has become visible
from Rosetta only since 2015 March. It was illuminated during the perihelion passage and
therefore it contains the regions that experienced the strongest heating and erosion rates, thus exposing the sub-surface most pristine material. In this work we investigate, thanks to the OSIRIS images, the geomorphology, the spectrophotometry and some transient events of two Southern hemisphere regions: Anhur and part of Bes. Bes is dominated by outcropping consolidated terrain covered with fine particle deposits, while Anhur appears strongly eroded with elongated canyon-like structures, scarp retreats, different kinds of deposits and degraded sequences of strata indicating a pervasive layering. We discovered a new 140 m long and 10 m high scarp formed in the Anhur–Bes boundary during/after the perihelion passage, close to the area where exposed CO₂ and H₂O ices were previously detected. Several jets have been observed originating from these regions, including the strong perihelion outburst, an active pit and a faint optically thick dust plume. We identify several areas with a relatively bluer slope (i.e. a lower spectral slope value) than their surroundings, indicating a surface composition enriched with some water ice. These spectrally bluer areas are observed especially in talus and
gravitational accumulation deposits where freshly exposed material had fallen from nearby
scarps and cliffs. The investigated regions become spectrally redder beyond 2 au outbound when the dust mantle became thicker, masking the underlying ice-rich layers.

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