A CAMBRIAN ORIGIN FOR CRINOIDS? PROBABILISTIC MODELING OF EVOLUTIONARY TREES SUPPORTS A LONG FUSE OF LATENT DIVERSIFICATION ACROSS THE CAMBRIAN-ORDOVICIAN BOUNDARY
The origin of the Class Crinoidea (Echinodermata) has been a subject of major debate for the last 20 years, when Ausich & Babcock (1998) first argued that the oldest tentative crinoid, Echmatocrinus brachiatus Sprinkle 1973, was probably an octocoral. More recently, another debate has emerged as to whether the Crinoidea are sister to edrioasteroids (such as edrioblastoids) or to the diploporitan Eumorphocystis.
Using an empirically constrained crinoid suptertree and occurrence data of Ordovician species (N=597), including the oldest representatives (e.g., Guensburg & Sprinkle 2003), I apply multiple probabilistic approaches to estimate the age of the MRCA of total-group Crinoidea. Importantly, I do not condition on outgroup selection. Results indicate crinoids likely originated during the latest Cambrian. This does not falsify either sister group hypothesis, but it does suggest a substantial “latent” diversification may have taken place during the Cambrian-Ordovician transition. Although the latest Cambrian is characterized by a highly incomplete echinoderm record, additional studies searching for the oldest crinoid fossils are warranted, especially in geographically undersampled paleocontinents.