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Monte San Nicola (Sicily): Gelasian GSSP and base Quaternary/Pleistocene

  • L. Capraro*
  • , S. Bonomo
  • , A. Incarbona
  • , F. J. Hilgen
  • , E. Zanola
  • , A. Di Stefano
  • , F. Dela Pierre
  • , S. Ferraro
  • , P. Ferretti
  • , E. Fornaciari
  • , S. Galeotti
  • , P. Macrì
  • , A. Negri
  • , I. Raffi
  • , T. Rodrigues
  • , F. Speranza
  • , B. R. Spiering
  • , T. Tesei
  • , M. V. Triantaphyllou
  • , E. Turco
  • G. B. Vai, E. Di Stefano, R. Sprovieri, D. Rio
*Corresponding author for this work
  • University of Padova
  • National Research Council of Italy
  • University of Palermo
  • University of Catania
  • University of Turin
  • Ca’ Foscari University of Venice
  • University of Urbino
  • Istituto Nazionale Di Geofisica E Vulcanologia
  • Marche Polytechnic University
  • Gabriele d’Annunzio University
  • The Portuguese Institute for Sea and Atmosphere
  • University of Algarve
  • National and Kapodistrian University of Athens
  • University of Parma
  • University of Bologna

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

The Gelasian Stage, established in 1998 at Monte San Nicola (Southern Sicily) as the third Stage for the Pliocene Series above the Zanclean and the Piacenzian, was overlooked for years but regained global recognition in 2009, when the base of both the Pleistocene Series and the Quaternary System was lowered to match the Piacenzian/Gelasian boundary. In recent years, independent research groups have been collecting scientific data at Monte San Nicola from two sections, namely the “historical” GSSP profile and the nearby Mandorlo section. Evidence collected in the “historical” section prove that the current GSSP definition does no longer meet the standards for a modern formal chronostratigraphic boundary, and the relevant host section is affected by tectonic reductions that prevent achieving a continuous and reliable chronostratigraphic record. On the contrary, the Mandorlo section offers a pristine depiction of the geological and biotic events that are expected to occur from the Piacenzian/Gelasian boundary up to the base Calabrian, which possibly make it the best reference profile globally for investigating the Neogene – Quaternary transition. We provide a commented review of the current state of the scientific knowledge on the Monte San Nicola stratigraphy in the view of possible actions to be taken soon, such as the definition of the Astronomical Unit Stratotype and Astrochronozones for the Gelasian Stage.

Original languageEnglish
Article number109885
JournalQuaternary Science Reviews
Volume381
Early online date21 Feb 2026
DOIs
Publication statusE-pub ahead of print - 21 Feb 2026

Bibliographical note

Publisher Copyright:
© 2026 The Authors.

Funding

We are grateful to Dr. Biagio Giaccio, Editor of QSR, and to Dr. Martin Head and an anonymous reviewer for providing comments and suggestions that greatly improved the manuscript. This Research was funded by MUR (PRIN 20227ZCCFX to ADS and LC ).

FundersFunder number
Ministero dell'Università e della RicercaPRIN 20227ZCCFX

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