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The Muridae from Kastellios Hill (late Miocene, Crete, Greece): updated taxonomy and age

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Abstract

In discussions on European Neogene continental chronology, the Kastellios Hill section has played an important role because of the presence of strata with planktonic foraminifers and strata with mammalian remains. With the primary papers written in the 1970s and 1980s, the time is ripe for an update on age and taxonomy of the murid rodents from Kastellios Hill by comparing the fauna with time-equivalent southern and central European faunas. This comparison results in a partly revised faunal list consisting of the dominant Progonomys mixtus n. sp., the less common Cricetulodon cf. C. hartenbergeri Freudenthal, 1967 and P. cathalai Schaub, 1938, and the rare P. hispanicus Michaux, 1971 and cf. Hansdebruijnia neutra (de Bruijn, 1976). Based on the updated species list and magnetic polarity data, the most probable age of the Kastellios Hill mammal localities is 9.3–9.1 Ma (Chron C4Ar.1r, late Vallesian, MN10). The genus Hansdebruijnia is narrowed down to two species in an ancestor–descendant relationship: the ancestral type species H. neutra, which is restricted to southeastern Europe and Anatolia, and the descendant species H. magna (Sen, 1977), representing a new combination and including ‘Occitanomys alcalai’ Adrover et al., 1988 and ‘O. debruijni’ (Hordijk and de Bruijn, 2009). H. magna colonized both southeastern and southwestern Europe.

Original languageEnglish
Pages (from-to)1218-1238
Number of pages21
JournalJournal of Paleontology
Volume99
Issue number5
DOIs
Publication statusPublished - Sept 2025

Bibliographical note

Publisher Copyright:
© The Author(s), 2025. Published by Cambridge University Press on behalf of Paleontological Society.

Funding

We are grateful to M. Palmero and L. Bik for drawing Fig. 4. A. Bosma is thanked for sharing her opinion on the Sciuridae from K1, J. van der Made for providing information on the large mammals from Kastellios Hill. D. van Hinsbergen, W. Krijgsman, C. Langereis, and S. Sen are thanked for discussing the magnetostratigraphy. We thank the reviewers for their constructive comments and J. Calede for editorial handling. This work was funded by MCIN/AEI/10.13039/501100011033 (R+D+I project PID2020-117289GB-I00) and the Generalitat de Catalunya/CERCA Program (to J.A.v.D.).

FundersFunder number
Ministerio de Ciencia, Innovacin y UniversidadesMCIN/AEI/10.13039/501100011033, PID2020-117289GB-I00
Generalitat de Catalunya/CERCA Program

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