Abstract. The collision between Gondwana and Laurussia that formed the latest
supercontinent, Pangea, occurred during Devonian to early Permian times and
resulted in a large-scale orogeny that today transects Europe, northwest
Africa, and eastern North America. This orogen is characterized by an “S”
shaped corrugated geometry in Iberia. The northern curve of the corrugation
is the well-known and studied Cantabrian (or Ibero–Armorican) Orocline and
is convex to the east and towards the hinterland. Largely ignored for
decades, the geometry and kinematics of the southern curvature, known as the
Central Iberian curve, are still ambiguous and hotly debated. Despite the
paucity of data, the enigmatic Central Iberian curvature has inspired a
variety of kinematic models that attempt to explain its formation but with
little consensus. This paper presents the advances and milestones in our
understanding of the geometry and kinematics of the Central Iberian curve
from the last decade with particular attention to structural and
paleomagnetic studies. When combined, the currently available datasets suggest that the Central
Iberian curve did not undergo regional differential vertical-axis rotations
during or after the latest stages of the Variscan orogeny and did not form
as the consequence of a single process. Instead, its core is likely a
primary curve (i.e., inherited from previous physiographic features of the
Iberian crust), whereas the curvature in areas outside the core is dominated
by folding interference from the Variscan orogeny or more recent Cenozoic
(Alpine) tectonic events.