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4 E. Borghi and V. Garilli
Downloaded by [vittorio garilli] at 22:43 08 June 2016 Figure 1. Distribution of genera of the regular echinoid family Temnopleuridae and of two genera of the closely related family Trigono-
cidaridae (data from Mortensen 1943; Smith & Kroh 2011). 1, Pentechinus Philip & Foster, 1971, Oligocene (Australia); 2, Paradoxe-
chinus, Upper EoceneÀLower Miocene (southern Australia); 3, Tremaster, Pliocene (France); 4, Temnechinus, PlioÀPleistocene
(England, The Netherlands, France); 5, Coptechinus, upper Miocene (France) to Pliocene (England, France); 6, Temnopleurus Agassiz,
1841, Pliocene to Recent (Indo-Paciï¬c), Recent (South Africa, Mozambico, Malay Archipelago, China Sea, Japan, Australia); 7, Temno-
trema, Miocene (Australia), Pleistocene (Japan), Recent (East Africa, Mauritius, Indian Ocean and Indo-West Paciï¬c, Japan, Australia,
Hawaii); 8, Erbechinus Jeannet in Lambert & Jeannet, 1935, Pliocene (Java), Recent (Kei Islands); 9, Opechinus, Eocene (Pakistan),
Miocene (Quatar and Saudi Arabia, India, Indonesia), Pliocene? (Indonesia), Recent (Indo-West Paciï¬c); 10, Microcyphus Agassiz, in
Agassiz & Desor, 1846, Miocene (Java), Pliocene (Indonesia), Recent (Red Sea, East Africa, Madagascar, Mauritius, Ceylon, Andaman
Sea, Philippines, Sumatra, Japan, Kei Islands, Australia); 11, Mespilia Desor, in Agassiz & Desor, 1846, Recent (Indo-West Paciï¬c);
12, Salmacis Agassiz, 1841, Recent (South Africa, Indian Ocean, Indo-West Paciï¬c); 13, Salmaciella Mortensen, 1942, Recent (Mozam-
bico, Seychelles, Indo-West Paciï¬c, Australia); 14, Amblypneustes Agassiz, 1841, Recent (Australia and New Zealand); 15, Holop-
neustes Agassiz, 1841, Recent (Australia and New Zealand); 16, Paratrema Koehler, 1927, Recent (Indo-Paciï¬c); 17, Placentinechinus
gen. nov., Early Pleistocene (Italy); 18, Hypsiechinus, Recent (Atlantic, around Iceland) (Trigonocidaridae); 19, Monilechinus, middle
Miocene (Portugal) (Trigonocidaridae). Possible routes of dispersal from the oldest descendants (as from Mortensen 1943 and Kroh &
Smith 2010) are outlined.
unconformities, as eccentricity-controlled clusters over been formed in a temperate shelf environment in deposi-
periods of 100À400 kyr, suggesting correlation with sap- tional settings not dissimilar to that of Puglia today
ropel clusters ‘0’, ‘A’ and ‘C’ (Roveri & Taviani 2003, (Tropeano & Sabato 2000, with references).
with references).
The site in Calabria (southern Italy, Fig. 2A, E) belongs
The sites in Puglia (south-eastern Italy, Fig. 2A, D) to the predominantly late Neogene succession deposited
belong to the late Cenozoic succession that overlies the in the Crotone Basin, a forearc basin (Zecchin et al. 2004)
Mesozoic rocks of the Apulian Platform, a relict of Meso- located in the Ionian side of the Calabrian Arc, an inde-
zoic rifting that became part of the foreland of the south- pendent arcuate terrane that connects the southern Apen-
ern Apennine chain during the Neogene (D’Argenio nine chain and the east-trending Sicilian Maghrebides and
1974; Channel et al. 1979; Ricchetti 1980). The youngest, separates the Ionian and Tyrrhenian basins (Zecchin et al.
PlioÀPleistocene, part of the Cenozoic succession was 2006, 2012 with references). This structural domain con-
deposited after the mid-Pliocene rapid increase of subsi- sists of pre-Mesozoic polymetamorphic nappes and local
dence in the Apulian foreland, forming a carbonate domi- remnants of a Mesozoic to Cenozoic succession (Zecchin
nated system in shallow, shelf environments (particularly et al. 2012). The succession of the Crotone Basin lies on
well represented by the Calcarenite di Gravina Forma- the crystalline basement of the Sila unit and its oldest
tion). The carbonate system was subsequently drowned by deposits are late Serravallian, though the most common
siliciclastic deposits derived from the Apennines thrust. outcrops are of PlioÀPleistocene age. These outcrops
The Calcarenite di Gravina has been interpreted as having mainly consist of two units deposited in outer shelf to