Bhatt, M.; Mall, U.; Wöhler, C.; Grumpe, A.; Bugiolacchi, R.: A comparative study of iron abundance estimation methods: Application to the western nearside of the Moon. Icarus 248, pp. 72 - 88 (2015)
Mall, U.; Wöhler, C.; Grumpe, A.; Bugiolacchi, R.; Bhatt, M.: Characterization of lunar soils through spectral features extraction in the NIR. Advances in Space Research 54 (10), pp. 2029 - 2040 (2014)
Wöhler, C.; Grumpe, A.; Berezhnoy, A.; Bhatt, M. U.; Mall, U.: Integrated topographic, photometric and spectral analysis of the lunar surface: Application to impact melt flows and ponds. Icarus 235, pp. 86 - 122 (2014)
Bugiolacchi, R.; Mall, U.; Bhatt, M.; McKenna-Lawlor, S.; Ullaland, K.: From the Imbrium Basin to crater Tycho: The first regional spectral distribution map derived from SIR-2 near-infrared data. Icarus 223, pp. 804 - 818 (2013)
Reddy, V.; Le Corre, L.; O'Brien, D. P.; Nathues, A.; Cloutis, E. A.; Durda, D. D.; Bottke, W. F.; Bhatt, M. U.; Nesvorny, D.; Buczkowski, D.et al.; Scully, J. E. C.; Palmer, E. M.; Sierks, H.; Mann, P. J.; Becker, K. J.; Beck, A. W.; Mittlefehldt, D.; Li, J.-Y.; Gaskell, R.; Russell, C. T.; Gaffey, M. J.; McSween, H. Y.; McCord, T. B.; Combe, J.-P.; Blewett, D.: Corrigendum to ``Delivery of dark material to Vesta via carbonaceous chondritic impacts'' [Icarus 221, pg 544, 2012]. Icarus 223 (1), p. 632 - 632 (2013)
Bhatt, M.; Mall, U.; Bugiolacchi, R.; McKenna-Lawlor, S.; Banaszkiewicz, M.; Nathues, A.; Ullaland, K.: Lunar iron abundance determination using the 2-μm absorption band parameters. Icarus 220 (1), pp. 51 - 64 (2012)
Bugiolacchi, R.; Mall, U.; Bhatt, M.: A near-infrared reflectance survey across lunar crater Aristoteles. In: Proceedings of the 42nd Lunar and Planetary Science Conference. (2011)
Bugiolacchi, R.; Mall, U.; Bhatt, M.: NIR spectral investigation of the Delisle/Diophantus crater region by the SIR-2 instrument. In: Proceedings of the 42nd Lunar and Planetary Science Conference. (2011)
Bhatt, M. U.: Mineralogical analysis and iron abundance estimation of the Moon using the SIR-2 and other VIS-NIR spectrometers on-board the lunar orbiter Chandrayaan-1. Dissertation, Technische Universität Clausthal (2012)
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.