Description, Units, and Interpretation
Deformation belts are complex tectonic units including ridges, extensional fractures, and strike-slip fractures.
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Ridges or Ridge belts (see Ridged Plains) composed of parallel ridges, each a few hundred meters in elevation. Typical fold spacings are 5–10 km (Squyres et al. 1992). “Ridges are one of the main components of the deformation belts. Ridges are interpreted as contractional structures (large folds, thrusted antiforms). Individual ridges are convex-upwards, elongate features, of several km in width and tens of km in length. Commonly, ridges do not appear isolated, but organized in trains or bundles called ridge belts” (Fernández et al. 2010).
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Graben or Fracture belts dominated by intense...
References
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Fernández, C. (2014). Deformation Belt (Venus). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_151-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_151-1
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