Central mountain

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The central mountain is a typical topographical feature of larger impact craters . As the name suggests, the central mountain is located roughly in the middle of such a crater. It is created by the springback of the crater floor in the moments after the impact . Depending on the nature of the subsoil, the energy of the impact and the gravitation of the celestial body concerned, the central elevation is formed in craters with different diameters; on the moon of about 20 km in diameter. The 93 km diameter lunar crater Copernicus (see below) has several central mountains that rise up to a height of 1200 m above the crater floor.

Individual evidence

  1. Lunar Reconnaissance Orbiter: Sunrise View of Tycho Crater's Peak