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Much of the floor of
Kandinsky is a region of permanent shadow, which has a bright radar signature. This is interpreted to represent a deposit of water ice.
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John K. Harmon, Martin A. Slade, Melissa S. Rice, 2011. Radar imagery of
Mercury’s putative polar ice: 1999–2005 Arecibo results.
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Radar-bright deposits near the north pole. Kandinsky is near the center.
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243:"First Photos of Water Ice on Mercury Captured by NASA Spacecraft"
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142:, located near the planet's north pole. It was named by the
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156:The possible water ice was directly imaged by
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273:This article about the planet Mercury is a
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231:doi.org/10.1016/j.icarus.2010.08.007
182:Gazetteer of Planetary Nomenclature
277:. You can help Knowledge (XXG) by
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214:PIA19411: Water Ice on Mercury
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116:The crater, showing possible
146:in 2012 for Russian painter
94:60.0 km (37.3 mi)
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329:Impact craters on Mercury
334:Mercury (planet) stubs
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324:Borealis quadrangle
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148:Wassily Kandinsky
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105:Wassily Kandinsky
19:Crater on Mercury
16:Crater on Mercury
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249:19 February
245:. Space.com
178:"Kandinsky"
64: /
39:Coordinates
318:Categories
199:23 January
164:References
134:is a deep
78:Quadrangle
158:MESSENGER
132:Kandinsky
118:water ice
23:Kandinsky
90:Diameter
83:Borealis
52:281°13′E
140:Mercury
49:87°53′N
33:Mercury
227:Icarus
136:crater
100:Eponym
29:Planet
275:stub
251:2022
201:2023
194:USGS
190:NASA
186:IAU
150:.
144:IAU
138:on
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192:/
188:/
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.