Stephanian (stage)

Source: Wikipedia, the free encyclopedia.
System Series
(NW Europe)
Stage
(NW Europe)
Series
(ICS)
Stage
(ICS)
Age
(
Ma
)
Permian younger
Carboniferous Silesian Stephanian Pennsylvanian Gzhelian 298.9–303.7
Kasimovian 303.7–307.0
Westphalian Moscovian 307.0–315.2
Bashkirian 315.2–323.2
Namurian
Mississippian
Serpukhovian 323.2–330.9
Dinantian
Visean
Visean
330.9–346.7
Tournaisian Tournaisian 346.7–358.9
Devonian older
Subdivisions of the Carboniferous system in Europe compared with the official ICS-stages (as of 2018)

The Stephanian is a

Coal Measures of England and Wales are probably of Stephanian age, though the larger part of this formation is referred to the earlier Westphalian. The stage derives its name from the city of Saint-Étienne for its coal mining basin in eastern central France (which itself derives from associations with Saint Stephen) where strata of this age occur.[2]

In the official

geologic timescale of the ICS, the Stephanian is placed within the Pennsylvanian epoch (323-299 Ma).[3]

The (regionally defined) Stephanian stage corresponds to the (internationally used) Kasimovian and Gzhelian stages.[1] References appear in scientific literature to a Stephanian epoch or Stephanian series reflecting the stage's earlier status. Sediments younger than the Stephanian are sometimes termed the Autunian, a regional stage which includes the Carboniferous-Permian boundary.[4][5]

Stratigraphy

From youngest to oldest, the proposed substages of the Stephanian are:[4][5]

  • Stephanian C
  • Stephanian B
  • "Saberian" [correlation uncertain]
  • Barruelian (Stephanian A)
  • Cantabrian

Base of the Stephanian

The Westphalian-Stephanian boundary is controversial and has not been formally defined. The early part of the Stephanian is difficult to recognize in much of Europe, due to sediment hiatuses or a transition from coal to unfossiliferous red beds. This issue is most apparent in the Lorraine-Saar-Nahe Basin of France and Germany, where a long hiatus occupies several million years between the Westphalian D and Stephanian A substages.[1]

Several workarounds have been proposed, but many bring forward their own problems. Many sources air on the side of caution and position the start of the Stephanian at the end of the hiatus. By that time, Kasimovian-type plant species are well-established, suggesting that part of the Westphalian D is Kasimovian in age. Other studies disagree with this approach, instead defining the Westphalian-Stephanian boundary at a major transition of plant faunas prior to the hiatus.[1]

Northwest Spain seems to offer a potential solution to the debate, since the regions of Asturias and Cantabria offer undisrupted and fossil-rich sediments which appear to fill in the gap between Westphalian D and Stephanian A. Most Carboniferous stratigraphers accept the utility of this interval, which has been named as the "Cantabrian" substage, the earliest substage of the Stephanian. Kasimovian-type plants first appear just above the base of the Cantabrian, arguing that the base of the Stephanian is slightly older than the start of the Kasimovian (around 307 Ma).[1]

References

  1. ^
    ISSN 0305-8719
    .
  2. ^ "Archived copy" (PDF). Archived from the original (PDF) on 2011-03-04. Retrieved 2016-04-08.{{cite web}}: CS1 maint: archived copy as title (link)
  3. , retrieved 2023-10-09
  4. ^
  5. ^