Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals

Adaptive radiations are hypothesised as a generating mechanism for much of the morphological diversity of extant species 1,2,3,4,5,6,7 . The Cenozoic radiation of placental mammals, the foundational example of this concept 8,9 , gave rise to much of the morphological disparity of extant mammals, and...

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Auteurs principaux: Brocklehurst, N, Panciroli, E, Benevento, G, Benson, RBJ
Format: Journal article
Langue:English
Publié: Cell Press 2021
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author Brocklehurst, N
Panciroli, E
Benevento, G
Benson, RBJ
author_facet Brocklehurst, N
Panciroli, E
Benevento, G
Benson, RBJ
author_sort Brocklehurst, N
collection OXFORD
description Adaptive radiations are hypothesised as a generating mechanism for much of the morphological diversity of extant species 1,2,3,4,5,6,7 . The Cenozoic radiation of placental mammals, the foundational example of this concept 8,9 , gave rise to much of the morphological disparity of extant mammals, and is generally attributed to relaxed evolutionary constraints following the extinction of non-avian dinosaurs 10,11,12,13 . However, study of this and other radiations has focussed on variation in evolutionary rates 4,5,7,14 , leaving the extent to which relaxation of constraints enabled the origin of novel phenotypes less well-characterised 15,16,17 . We evaluate constraints on morphological evolution among mammaliaforms (mammals and their closest relatives) using a new method that quantifies the capacity of evolutionary change to generate phenotypic novelty. We find that Mesozoic crown-group therians, which include the ancestors of placental mammals, were significantly more constrained than other mammaliaforms. Relaxation of these constraints occurred in the mid-Paleocene, postdating the extinction of non-avian dinosaurs at the K/Pg boundary, instead coinciding with important environmental shifts and with declining ecomorphological diversity in non-theriimorph mammaliaforms. This relaxation occurred even in small-bodied Cenozoic mammals weighing <100g, which are unlikely to have competed with dinosaurs. Instead, our findings support a more complex model whereby Mesozoic crown therian evolution was in-part constrained by co-occurrence with disparate mammaliaforms, as well as by presence of dinosaurs, within-lineage incumbency effects and environmental factors. Our results demonstrate that variation in evolutionary constraints can occur independently of variation in evolutionary rate; and that both make important contributions to the understanding of adaptive radiations.
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spelling oxford-uuid:bda82407-db76-4c15-b061-ceb9ae271dd52022-05-17T08:04:05ZMammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammalsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:bda82407-db76-4c15-b061-ceb9ae271dd5EnglishSymplectic ElementsCell Press2021Brocklehurst, NPanciroli, EBenevento, GBenson, RBJAdaptive radiations are hypothesised as a generating mechanism for much of the morphological diversity of extant species 1,2,3,4,5,6,7 . The Cenozoic radiation of placental mammals, the foundational example of this concept 8,9 , gave rise to much of the morphological disparity of extant mammals, and is generally attributed to relaxed evolutionary constraints following the extinction of non-avian dinosaurs 10,11,12,13 . However, study of this and other radiations has focussed on variation in evolutionary rates 4,5,7,14 , leaving the extent to which relaxation of constraints enabled the origin of novel phenotypes less well-characterised 15,16,17 . We evaluate constraints on morphological evolution among mammaliaforms (mammals and their closest relatives) using a new method that quantifies the capacity of evolutionary change to generate phenotypic novelty. We find that Mesozoic crown-group therians, which include the ancestors of placental mammals, were significantly more constrained than other mammaliaforms. Relaxation of these constraints occurred in the mid-Paleocene, postdating the extinction of non-avian dinosaurs at the K/Pg boundary, instead coinciding with important environmental shifts and with declining ecomorphological diversity in non-theriimorph mammaliaforms. This relaxation occurred even in small-bodied Cenozoic mammals weighing <100g, which are unlikely to have competed with dinosaurs. Instead, our findings support a more complex model whereby Mesozoic crown therian evolution was in-part constrained by co-occurrence with disparate mammaliaforms, as well as by presence of dinosaurs, within-lineage incumbency effects and environmental factors. Our results demonstrate that variation in evolutionary constraints can occur independently of variation in evolutionary rate; and that both make important contributions to the understanding of adaptive radiations.
spellingShingle Brocklehurst, N
Panciroli, E
Benevento, G
Benson, RBJ
Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title_full Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title_fullStr Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title_full_unstemmed Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title_short Mammaliaform extinctions as a driver of the morphological radiation of Cenozoic mammals
title_sort mammaliaform extinctions as a driver of the morphological radiation of cenozoic mammals
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