ORIGIN OF THE WHITE SHARK CARCHARODON (LAMNIFORMES: LAMNIDAE) BASED ON RECALIBRATION OF THE UPPER NEOGENE PISCO FORMATION OF PERU

被引:132
作者
Ehret, Dana J. [1 ]
Macfadden, Bruce J. [2 ]
Jones, Douglas S. [2 ]
Devries, Thomas J. [3 ]
Foster, David A. [4 ]
Salas-Gismondi, Rodolfo [5 ]
机构
[1] Monmouth Univ, W Long Branch, NJ 07764 USA
[2] Univ Florida, Florida Museum Nat Hist, Gainesville, FL 32611 USA
[3] Univ Washington, Burke Museum Nat Hist & Culture, Seattle, WA 98195 USA
[4] Univ Florida, Dept Geol Sci, Gainesville, FL 32611 USA
[5] Univ Nacl Mayor San Marcos, Museo Hist Nat Javier Prado, Dept Paleontol Vertebrados, Lima 11, Peru
基金
美国国家科学基金会;
关键词
Carcharocles; Cosmopolitodus; geochronology; Miocene; Isurus; strontium; NIOBRARA CHALK; EARLY-PLIOCENE; MIOCENE; ISOTOPE; CHONDRICHTHYES; OLIGOCENE; AGE; ELASMOBRANCHII; VERTEBRATES; SKELETAL;
D O I
10.1111/j.1475-4983.2012.01201.x
中图分类号
Q91 [古生物学];
学科分类号
0709 ; 070903 ;
摘要
The taxonomic origin of the white shark, Carcharodon, is a highly debated subject. New fossil evidence presented in this study suggests that the genus is derived from the broad-toothed 'mako', Carcharodon (Cosmopolitodus) hastalis, and includes the new species C. hubbelli sp. nov. - a taxon that demonstrates a transition between C. hastalis and Carcharodon carcharias. Specimens from the Pisco Formation clearly demonstrate an evolutionary mosaic of characters of both recent C. carcharias and fossil C. hastalis. Characters diagnostic to C. carcharias include the presence tooth serrations and a symmetrical first upper anterior tooth that is the largest in the tooth row, while those indicative of C. hastalis include a mesially slanted third anterior (intermediate) tooth. We also provide a recalibration of critical fossil horizons within the Pisco Formation, Peru using zircon U-Pb dating and strontium-ratio isotopic analysis. The recalibration of the absolute dates suggests that Carcharodon hubbelli sp. nov. is Late Miocene (6-8 Ma) in age. This research revises and elucidates lamnid shark evolution based on the calibration of the Neogene Pisco Formation.
引用
收藏
页码:1139 / 1153
页数:15
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