An impact crater with relatively low depth/diameter ratio; central uplift; annular trough; and down-faulted, terraced rim structure. Central uplift can be expressed topographically as a peak and/or ring.
Solid, liquid, or vaporized rock ejected ballistically from an explosion or impact crater during formation. Such material may be distributed around a crater in distinctive patterns, forming "ejecta rays" or "ejecta loops", as well as partially building the rim.
The distance from rim to rim of the cavity once collapse has completed.
An impact crater of relatively small diameter, characterized by a uniformly concave-upward shape and a maximum depth in the center, and lacking a central uplift and rim terraces. Simple craters differ from transient craters by the presence of a breccia lens; e.g. Barringer Crater (Meteor Crater) in Coconino County, Ariz.
The cavity formed immediately after the end of crater excavation, before it undergoes collapse and modification. Its outer extent is defined by the boundary between excavated and non-excavated (but possibly displaced) target material, and its depth is the maximum achieved by material that will eventually form the floor of the true crater after cratering motions cease. Although it is by nature temporary, laboratory-derived scaling relations apply only to the diameter of the transient crater, not the final collapsed crater form. Collapse of a transient crater produces both simple and complex impact craters.