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An early Proterozoic supercontinent whose assembly is commonly placed broadly around 1.9–1.6 billion years ago. The terms Columbia and Nuna are often used interchangeably, although some reconstructions distinguish their regional or temporal meanings. Geological connections and dated apparent polar wander paths test proposed configurations.^[ref]

Repeated assembly and dispersal are supported by mutually consistent paleogeography, paleomagnetism, dated collision belts and subsequent rifted margins. A useful reconstruction must explain both former connections and later separation, at the same geological ages.

For the youngest well-constrained example, Pangaea, matching continental outlines become more compelling when the fit uses the continental edges rather than mobile modern shorelines. More discriminating evidence includes the continuation of mountain belts, sedimentary successions and distinctive basement rocks across now-separated continents. Correlated terrestrial fossil assemblages and the distribution of glacial deposits become geographically coherent when the continents are restored. Each observation alone can have alternatives, but a single reconstruction that satisfies several independent tests is much harder to explain by coincidence.

For older examples, the most useful surviving record lies within the cratons and their margins. Dated suture zones, ophiolites, metamorphic belts and pressure-temperature-time paths document former ocean closure and continental collision. Restoring now-separated belts to continuity tests an assembly. Subsequent continental rifting, matching dike swarms, large igneous provinces and the transition to passive margins test its breakup. Uranium-lead dating of zircon, including detrital zircon populations and sedimentary provenance, helps establish whether the proposed connections existed at the same time.

Paleomagnetism supplies an independent quantitative test. A primary remanent magnetization constrains ancient latitude and orientation. After a proposed relative rotation brings two blocks together, compatible apparent polar wander paths over an interval support their travelling together; divergence of those paths can document separation. Radiometric dating, a paleomagnetic fold test and a paleomagnetic reversal test help identify primary records and distinguish them from remagnetization. There remain important ambiguities: conventional paleomagnetism does not fix absolute longitude, and sparse ages, later deformation and true polar wander complicate a reconstruction.

The broad succession is Columbia or Nuna, assembled mainly around 1.9–1.6 billion years ago; Rodinia, assembled mainly around 1.1–0.9 billion years ago and dispersed in stages during the later Proterozoic; and Pangaea, assembled by roughly 300 million years ago and breaking apart from roughly 200 million years ago. These are broad intervals rather than synchronous global events. A quantitative Nuna reconstruction combines paleomagnetism with the histories of continental margins rather than relying only on matching rock ages.^[ref]

Repeated global peaks in dated magmatism and metamorphism offer supporting evidence, but cannot prove a supercontinent cycle by themselves: erosion, burial and preferential preservation also change the observed age distribution. The persuasive case is the recurrence of dated assembly–breakup sequences in different continental configurations, with stronger geometric constraints for Pangaea than for the older supercontinents. A Wilson cycle describes an individual ocean's opening and closure; a supercontinent cycle concerns the much larger-scale continental assembly and dispersal.

The expected broad contrast is a less mature, commonly thinner early juvenile continental crust, with more mafic material and abundant sodic tonalite-trondhjemite-granodiorite, rather than the more differentiated, potassium-rich granitoid component characteristic of much Phanerozoic continental crust. This is a secular tendency, not a single stratified column applicable throughout the Archean.

Archean terrains commonly expose tonalite-trondhjemite-granodiorite gneiss associated with greenstone belts containing basalt, komatiite and metasedimentary rocks. Many later granitoids are richer in potassium, including granite and granodiorite. The proportions changed during the Archean: a reconstruction from trace element ratios in sedimentary rocks infers a markedly mafic upper continental crust before about 3.0 Ga and a more felsic upper continental crust by 2.5 Ga. Thus “all Archean continental crust was mafic” would be wrong. A preserved tonalite-trondhjemite-granodiorite-dominated nucleus can be strongly felsic, including at depth; its composition is not identical to that of its original juvenile precursor.^[ref]

Thickness needs a stated comparison. An influential seismic compilation found preserved Archean crust about 27–40 km thick, commonly without the thick high-velocity basal layer of its 40–55 km thick Proterozoic comparison provinces. That supports a relatively thin endmember, but is not a measurement of every original Archean continental crust, nor a demonstration that every Archean region was thinner than today's 35–40 km reference column. Tectonic thickening, magmatic underplating, erosion, delamination and preservation bias all alter what survives. The very thick lithospheric mantle beneath a craton must also not be mistaken for thick continental crust.^[ref]

The transferable answer is therefore more mafic early juvenile precursors, widespread sodic tonalite-trondhjemite-granodiorite production, and variable thickness evolving through time; late Archean felsic nuclei can already resemble substantial modern continental crust.

A Proterozoic supercontinent assembled principally around 1.1–0.9 billion years ago and dispersed in stages later in the Proterozoic. Its detailed continental configuration is less tightly constrained than that of Pangaea, because later deformation and recycling have removed much of the original evidence.