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How are mountain belts on Venus similar to the Himalayas?

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Venus
Venus Venus photographed in ultraviolet light by the Pioneer Venus Orbiter (Pioneer 12) spacecraft, February 26, 1979. Although Venus's cloud cover is nearly featureless in visible light, ultraviolet imaging reveals distinctive structure and pattern, including global-scale V-shaped bands that open toward the west (left). Added color in the image emulates Venus's yellow-white appearance to the eye.

Mountain belts on Venus are similar to those on Earth, such as the Himalayas, in their structural formation. Like Earth's mountain ranges, Venusian belts typically consist of parallel ridges and troughs that likely developed when broad bands of the lithosphere were compressed, thickened, and folded or thrust upward. Furthermore, specific features on Venus mirror terrestrial geography; for instance, the high plateau of Lakshmi Planum is configured similarly to the Plateau of Tibet, and the massive Maxwell Montes range is comparable in size to the Himalayas.12

However, their appearance differs significantly due to the absence of liquid water or ice on Venus. Without rivers or glaciers to facilitate erosion, Venusian mountains lack the typical erosional forms found on Earth. Instead, they exhibit extremely steep slopes caused by folding and faulting, with some slopes having collapsed under their own weight.1