Oklay, N.; Vincent, J.-B.; Besse, S.; Fornasier, S.; Barucci, M. A.; Lara, L.; Scholten, F.; Preusker, F.; Forgia, F. L.; Monica Lazzarin and, H. S.et al.; Hall, I.; The OSIRIS Team: Colors of comet 67P/Churyumov-Gerasimenkos active pits and their surroundings as seen by OSIRIS on board Rosetta. European Geosciences Union General Assembly, Vienna, Austria (2015)
Oklay, N.; Vincent, J.-B.; Sierks, H.; Besse, S.; Fornasier, S.; Barucci, M. A.; Luisa, L.; Scholten, F.; Preusker, F.; Lazzarin, M.et al.; Pajola, M.; La Forgia, F.; Hall, I.; The OSIRIS Team: Colors of active regions on comet 67P. European Planetary Science Congress EPSC , Nantes, France (2015)
Oklay, N.; Vincent, J.-B.; Sierks, H.; Masoumzadeh, N.; Hall, I.; Fornasier, S.; Barucci, M.; Pajola, M.; Lazzarin, M.; Besse, S.et al.; Lara, L. M.; Mottola, S.; Scholten, F.; Preusker, F.; Pommerol, A.: Variegation of active regions on comet 67P/Churyumov-Gerasimenko. Division for Planetary Sciences 48, Washington DC, USA (2015)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
Data from NASA's Dawn mission, analyzed for the first time, suggest that brine rose from the depths and organic compounds were deposited in Urvara crater.