, on Earth's
Moon Multi-ring basins are some of the largest, oldest, rarest and least understood of impact craters. There are various hypotheses to explain the formation of multi-ringed basins, including harmonic oscillations as is observed when a pebble is dropped on calm water, and brittle terrace faulting; however, there is currently no consensus. In 2016, research brought forward new hypotheses about the formation of the
lunar mare called
Mare Orientale on Earth's
Moon. Prior to this research, the most accepted explanation was the 'slumping/megaterrace' model, which suggested that a deep bowl-shaped basin forms during the impact and that subsidence along faults later produces the ring formations, though this hypothesis was always considered problematic because of evidence that the rings were produced simultaneously with the impact that formed the basin. The new research produced a model confirming instantaneous formation of all rings, a mechanism in which ductile subsurface rocks flowed towards the center of the basin as the crust rebounded, causing concentric cracking and slippage that formed the outer rings, and that the unstable central peak collapsing formed the inner ring. ==Examples==