Geology and colour of Kupalo crater on Ceres
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W. Goetz | H. Hiesinger | A. Nathues | N. Schmedemann | G. Thangjam | M. Hoffmann | K. Mengel | J. Hernandez | R. Sarkar
[1] V. Lapshin,et al. The effect of impact velocity on rebound height after impact interaction , 2020, IOP Conference Series: Materials Science and Engineering.
[2] Deutsche Forschungsanstalt für Luft und Raumfahrt,et al. The surface of (1) Ceres in visible light as seen by Dawn/VIR , 2020, 2010.03453.
[3] C. Russell,et al. Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process , 2020, Nature Communications.
[4] C. Russell,et al. The varied sources of faculae-forming brines in Ceres’ Occator crater emplaced via hydrothermal brine effusion , 2020, Nature Communications.
[5] B. Gądek,et al. Processes controlling the development of talus slopes in SW Spitsbergen: The role of deglaciation and periglacial conditions , 2020, Land Degradation & Development.
[6] E. Cloutis,et al. Recent cryovolcanic activity at Occator crater on Ceres , 2020, Nature Astronomy.
[7] M. Hesse,et al. Impact-driven mobilization of deep crustal brines on dwarf planet Ceres , 2019, Nature Astronomy.
[8] A. Nathues,et al. Landslides on Ceres: Diversity and Geologic Context , 2019, Journal of geophysical research. Planets.
[9] R. Kenner. Mass wasting processes affecting the surface of an alpine talus slope: Annual sediment budgets 2009–2018 at Flüelapass, eastern Swiss Alps. , 2019, Land Degradation & Development.
[10] C. Russell,et al. Fluidized Appearing Ejecta on Ceres: Implications for the Mechanical Properties, Frictional Properties, and Composition of its Shallow Subsurface , 2019, Journal of Geophysical Research: Planets.
[11] Brandon C. Johnson,et al. Post-impact thermal structure and cooling timescales of Occator crater on asteroid 1 Ceres , 2019, Icarus.
[12] J. E. Riedel,et al. High-resolution shape model of Ceres from stereophotoclinometry using Dawn Imaging Data , 2019, Icarus.
[13] G. Collins,et al. Formation of Complex Craters in Layered Targets With Material Anisotropy , 2019, Journal of Geophysical Research: Planets.
[14] F. G. Carrozzo,et al. Spectral analysis of the Cerean geological unit crater central peak material as an indicator of subsurface mineral composition , 2019, Icarus.
[15] T. McCord,et al. Ceres’s internal evolution: The view after Dawn , 2018, Meteoritics & Planetary Science.
[16] F. G. Carrozzo,et al. Nature, formation, and distribution of carbonates on Ceres , 2018, Science Advances.
[17] E. Cloutis,et al. Spectral properties and geology of bright and dark material on dwarf planet Ceres , 2017, 1712.05203.
[18] L. McFadden,et al. Stability of hydrated carbonates on Ceres , 2017, Icarus.
[19] Katherine E. Johnson,et al. Exposed H2O-rich areas detected on Ceres with the dawn visible and infrared mapping spectrometer , 2017, Icarus.
[20] F. G. Carrozzo,et al. Ceres’ impact craters – Relationships between surface composition and geology , 2017, Icarus.
[21] R. Jaumann,et al. The formation and evolution of bright spots on Ceres , 2017, Icarus.
[22] C. Russell,et al. The interior structure of Ceres as revealed by surface topography , 2017 .
[23] R. Jaumann,et al. The unique geomorphology and structural geology of the Haulani crater of dwarf planet Ceres as revealed by geological mapping of equatorial quadrangle Ac-6 Haulani , 2017, Icarus.
[24] E. Cloutis,et al. Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice , 2017 .
[25] F. G. Carrozzo,et al. Ac-H-11 Sintana and Ac-H-12 Toharu quadrangles: Assessing the large and small scale heterogeneities of Ceres’ surface , 2017, Icarus.
[26] C. Russell,et al. Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution , 2017, Geophysical research letters.
[27] C. Russell,et al. Geomorphological evidence for ground ice on dwarf planet Ceres , 2017 .
[28] F. G. Carrozzo,et al. An investigation of the bluish material on Ceres , 2017 .
[29] F. G. Carrozzo,et al. Artifacts reduction in VIR/Dawn data. , 2016, The Review of scientific instruments.
[30] K. Matz,et al. Timing of optical maturation of recently exposed material on Ceres , 2016 .
[31] R. Jaumann,et al. Cryogenic flow features on Ceres: Implications for crater‐related cryovolcanism , 2016 .
[32] C. Russell,et al. FC colour images of dwarf planet Ceres reveal a complicated geological history , 2016 .
[33] A. Longobardo,et al. Compositional differences among Bright Spots on the Ceres surface , 2016, Icarus.
[34] Christopher T. Russell,et al. High-resolution Ceres High Altitude Mapping Orbit atlas derived from Dawn Framing Camera images , 2016 .
[35] C. Russell,et al. The geomorphology of Ceres , 2016, Science.
[36] C. Russell,et al. Cratering on Ceres: Implications for its crust and evolution , 2016, Science.
[37] C. Russell,et al. A partially differentiated interior for (1) Ceres deduced from its gravity field and shape , 2016, Nature.
[38] R. Mugnuolo,et al. Bright carbonate deposits as evidence of aqueous alteration on (1) Ceres , 2016, Nature.
[39] C. Russell,et al. Geological Mapping of the Ac-H-12 Toharu Quadrangle of Ceres from NASA Dawn Mission , 2016 .
[40] C. Russell,et al. Surface Processes and Space Weathering on Ceres , 2016 .
[41] R. Jaumann,et al. Dawn arrives at Ceres: Exploration of a small, volatile-rich world , 2016, Science.
[42] R. Jaumann,et al. Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres , 2015, Nature.
[43] C. Russell,et al. Sublimation in bright spots on (1) Ceres , 2015, Nature.
[44] C. Russell,et al. Exogenic olivine on Vesta from Dawn Framing Camera color data , 2015 .
[45] J. Head,et al. Lunar floor-fractured craters as magmatic intrusions: Geometry, modes of emplacement, associated tectonic and volcanic features, and implications for gravity anomalies , 2015 .
[46] S. Leroueil,et al. The Varnes classification of landslide types, an update , 2014, Landslides.
[47] Debra L. Buczkowski,et al. Introduction: The geologic mapping of Ceres , 2014, Icarus.
[48] F. Scholten,et al. Mass‐wasting features and processes in Vesta's south polar basin Rheasilvia , 2013 .
[49] C. Pieters,et al. Space weathering on airless bodies , 2016, Journal of geophysical research. Planets.
[50] P. Mouginis-Mark,et al. Origin of small pits in martian impact craters , 2012 .
[51] A. McEwen,et al. Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process , 2012 .
[52] Andreas Nathues,et al. Color and Albedo Heterogeneity of Vesta from Dawn , 2012, Science.
[53] Robert O. Green,et al. Thermal removal from near‐infrared imaging spectroscopy data of the Moon , 2011 .
[54] T. Maue,et al. The Dawn Framing Camera , 2011 .
[55] David P. O'Brien,et al. The global effects of impact-induced seismic activity on fractured asteroid surface morphology , 2005 .
[56] E. Shock,et al. Composition and stability of salts on the surface of Europa and their oceanic origin , 2001 .
[57] A. Jahn. Periglacial talus slopes. Geomorphological studies on spitsbergen and in Northern Scandinavia , 1984 .
[58] E. Heggy,et al. Exploring Ceres’s Unusual Regolith Porosity and Its Implications for Volatile Retention , 2021, The Planetary Science Journal.
[59] M. Zolotov. The composition and structure of Ceres' interior , 2020 .
[60] R. Jaumann,et al. Bright carbonate surfaces on Ceres as remnants of salt-rich water fountains , 2019, Icarus.
[61] J. Plescia. Transitional Crater (Simple/Complex) , 2014 .
[62] F. D. Blasio,et al. Introduction to the Physics of Landslides , 2011 .
[63] D. Varnes. SLOPE MOVEMENT TYPES AND PROCESSES , 1978 .