The Characteristics of Polygonal Impact Craters on Venus.
- Published in:
- Earth, Moon & Planets, 2007, v. 101, n. 1-2, p. 41, doi. 10.1007/s11038-007-9148-4
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- Article
Works matching Venusian craters
Results: 8
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2
Postimpact modification by volcanic or tectonic processes as the rule, not the exception, for Venusian craters.
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- Journal of Geophysical Research. Planets, 2011, v. 116, n. E2, p. n/a, doi. 10.1029/2010JE003722
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- Article
3
Implications from stereo-derived topography of Venusian impact craters.
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- Journal of Geophysical Research. Planets, 2000, v. 105, n. E8, p. 20245, doi. 10.1029/1999JE001225
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- Article
4
Impact crater degradation on venusian plains.
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- Geophysical Research Letters, 1994, v. 21, n. 4, p. 289, doi. 10.1029/94GL00080
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- Article
5
Estimation of the age of impact craters and other adjacent geological subdivisions within the Thetis Regio on Venus.
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- Solar System Research, 2013, v. 47, n. 3, p. 159, doi. 10.1134/S0038094613030027
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- Article
6
Venusian craters.
- Published in:
- Nature, 1976, v. 263, n. 5572, p. 12, doi. 10.1038/263012a0
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- Article
7
Studying the Global Spatial Randomness of Impact Craters on Mercury, Venus, and the Moon With Geodesic Neighborhood Relationships.
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- Journal of Geophysical Research. Planets, 2021, v. 126, n. 3, p. 1, doi. 10.1029/2020JE006693
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- Article
8
Comparison of central pit craters on Mars, Mercury, Ganymede, and the Saturnian satellites.
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- Meteoritics & Planetary Science, 2017, v. 52, n. 7, p. 1371, doi. 10.1111/maps.12857
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- Article