The geology of the Ellsworth Mountains, Antarctica, is a rock record of continuous deposition that occurred from the Cambrian to the Permian periods, with basic igneous volcanism and uplift occurring during the Middle to Late Cambrian epochs, deformation occurring in the Late Permian period or early Mesozoic era, and glacier formation occurring in the Cretaceous period and Cenozoic era. The Ellsworth Mountains are located within West Antarctica at 79°S, 85°W. In general, it is made up of mostly rugged and angular peaks such as the Vinson Massif (), the highest mountain in Antarctica.
The early Cambrian, when carbonate deposits were deposited in shallow marine conditions, is when the geologic history record across the Ellsworth Mountains began. Up to the Permian period, subsidence and deposition process persisted. Volcanism was scarce in the early history of the Ellsworth Mountains. The majority of the strata are thought to have formed in marine environments at shallow to moderate depths. After sedimentary deposition occurred during the Permian time, all strata underwent orogeny, which lead to strong folding and localised metamorphism. It is hypothesised that there are two stages of the uplift separated by a steady period of erosional gradation as the deformed rocks have raised by at least . In the Ellsworth Mountains, alpine glaciation may have first appeared during the Mesozoic era. The local glacial processes in the Ellsworth Mountains are largely responsible for the contemporary landscapes that we observe today. The mountains were covered by the continental ice sheet throughout the middle to late Cenozoic period.
Stratigraphic geological history
The Ellsworth Mountains display a thick geologic sequence of Paleozoic sedimentary and volcanic rocks. The Lower to Upper Cambrian Heritage Group is part of the lower Paleozoic series old rock strata. The uppermost Cambrian to Devonian Crashsite Group makes up the middle portion of the geologic sequence, while the Permian-Carboniferous Whiteout Conglomerate and Permian Polarstar Formation make up the remaining upper portion.
The whole stratigraphic succession has been impacted by the two post-Permian episodes of deformation, Late Permian Deformation and Permian-Triassic Deformation (which will be covered in the Structural Geology portion). During the Permian-Triassic Gondwanian deformation event, the major dextral transpressive Permian-Triassic Deformation structure locally develops and superimposes the Late Permian Deformation structures. As a result, the rocks of the Ellsworth Mountains range from the Permian Polarstar Formation to lower strata of the Cambrian Heritage Group, with a positive correlation between depth and metamorphic grade.
Heritage Group
Union Glacier Formation, Hyde Glacier Formation, Drake Ice Fall Formation at southern Soholt Peaks, Conglomerate Ridge Formation, Library Hills Formation, Springer Peak Formation, Frazier Ridge Formation, and Minaret Formation are the eight clastic sedimentary and volcanic rock formations that make up the Heritage Group. The Heritage Group as a whole is around thick. The pumpellyite-actinolite grade and the lower greenschist facies make up the majority of the bottom units of the Cambrian Heritage Group. It is discovered to be a sequence of syn-rifts. The Heritage Group's conglomerate units' clast compositions indicate that an Early Cambrian carbonate platform and widespread quartzite exposures were present in the rift succession's source region.
Union Glacier Formation
The Union Glacier Formation is made up of volcaniclastic rocks that extend for around 3000 metres. Terrestrial lahar and ash-flow tuff deposits served as the raw ingredients for the formation of these rocks. In the late Early Cambrian to early Middle Cambrian era, it was developed. A continental rift, where the lithosphere was thinned, served as the tectonic backdrop for this formation during this time.
Hyde Glacier Formation
The heterolithic sequence bedding of the Hyde Glacier Formation, which ranges from sand to mud, demonstrates the depositional environment from fluvial to shallow-marine delta. This formation may be the result of tectonic movement or lateral discontinuity.