EGU26-8483, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-8483
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 04 May, 16:20–16:40 (CEST)
 
Room G2
Assembling Pangaea – The Complex Morphology of the Laurussia – Gondwana Collision
Yvette Kuiper1, Brendan Murphy2, Damian Nance3,4, Karel Schulmann5,6, and José Martínez Catalán7
Yvette Kuiper et al.
  • 1Colorado School of Mines, Geology and Geological Engineering, Golden CO, 80401, United States of America (ykuiper@mines.edu)
  • 2Department of Earth and Environmental Sciences, St. Francis Xavier University, Antigonish, NS B2G 2W5, Canada
  • 3Department of Earth and Environmental Geosciences, Ohio University, Athens, Ohio 45701, United States of America
  • 4Department of Earth and Planetary Sciences, Yale University, New Haven, Connecticut 06511, United States of America
  • 5Institut Terre et Environnement de Strasbourg, Université de Strasbourg, UMR 7063, 1 Rue Blessig, Strasbourg, 67084, France
  • 6Center for Lithospheric Research, Czech Geological Survey, Klárov 3, Prague 1, 11821, Czech Republic
  • 7Departamento de Geología, Facultad de Ciencias, Universidad de Salamanca, Salamanca, 37008, Spain

The Late Paleozoic convergence and collision between Gondwana and Laurentia resulted in along-strike variations in the Alleghanian–Mauritanide–Variscan orogeny during the assembly of the greater part of Pangaea. A series of ca. 380–290 Ma events segmented the orogen into two principal geodynamic domains with contrasting tectonic evolutions. In the northeast, the European Variscan belt records multiple subduction–collisional tectonic events, including indentation by Laurussian and later Gondwanan promontories and by Gondwana-derived terranes. Late-stage events (330–290 Ma) produced strongly curved deformation belts (oroclines), and late- to postorogenic extension. In contrast, the southern Appalachians formed southwest of the promontory collisions where subduction of Rheic Ocean remnants produced a continuous Andean-style orogenic arc that preceded ca. 290 Ma terminal collision. We explain Pangaea amalgamation using a global model of mantle convection like that of modern Earth.

How to cite: Kuiper, Y., Murphy, B., Nance, D., Schulmann, K., and Martínez Catalán, J.: Assembling Pangaea – The Complex Morphology of the Laurussia – Gondwana Collision, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8483, https://doi.org/10.5194/egusphere-egu26-8483, 2026.