Transcript
Page 1: Graham Slater's 2013 SVP talk

Graham SlaterDepartment of Paleobiology, National Museum of

Natural History

Tempo or Mode in Evolution? The Case of Mammalian Body

Size Evolution

www.fourdimensionalbiology.com

Page 2: Graham Slater's 2013 SVP talk

- Gene Hunt- Pete Wagner- Jon Marcot- Dave Bapst- Tom Ezard- Gavin Thomas- Andy Purvis

- Peter Smits- Greg Wilson

authors

- Luke Harmon*- Rob Freckleton- Sam Ponton

- Arne Mooers- Dave Polly- Folmer Bokma- Graeme Lloyd

organization reviews

data

“Unifying Fossils and Phylogenies for Comparative Analyses of Diversification

and Trait Evolution”

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Page 4: Graham Slater's 2013 SVP talk

How fast do animals evolve? That is one of

the fundamental questions regarding evolution.

Photo: Florida Museum of Natural History

Simpson (1944, 1953)

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is our emphasis on rates appropriate?

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Illustration by Mark Hallet

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Eoce

ne

Olig

oce

ne

Mio

cene

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Alroy (1999) Systematic Biology

fossil data show a rapid increase in body size disparity after the K-Pg

Sd

(m

ass

)

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Venditti et al. (2011) Nature

K Pg NgJ

relative rate

phylogenetic data suggest increased rates with the origin of modern

orders

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Page 11: Graham Slater's 2013 SVP talk

Do we really think the Tempo of mammalian

body size evolution increased after the K-

PG extinction?

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the mammalian body size zone

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the mammalian body size zone

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the mammalian body size zone

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variation in tempo

evolution slow

evolution fast

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Page 18: Graham Slater's 2013 SVP talk

variation in mode

evolution constrained

evolution unconstrained

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3 paleo-motivated models for mammalian body size evolution

BM rate 1 BM rate 2

Mesozoic CenozoicK-Pg rate shift

Ornstein-Uhlenbeck BM

Mesozoic Cenozoicecological release

Mesozoic Cenozoicrelease and radiate

BM*Ornstein-Uhlenbeck

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time calibrated phylogeny of living and fossil mammals

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Estimating body masses for Mesozoic mammals

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standard models paleo-inspired models

Brownian motion

directional

evolution

Ornstein-Uhlenbeck

Accelerating /

Decelerating

white noise

K-Pg Shift

ecological

release

release & radiate

extant taxa only

extant + fossils

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release & radiate fits best for extant taxa...

standard models paleo-inspired models

Brownian motion

directional

evolution

Ornstein-Uhlenbeck

Accelerating /

Decelerating

white noise

K-Pg Shift

ecological

release

release & radiate

extant taxa only

extant + fossils

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...and more so for the fossil dataset

standard models paleo-inspired models

Brownian motion

directional

evolution

Ornstein-Uhlenbeck

Accelerating /

Decelerating

white noise

K-Pg Shift

ecological

release

release & radiate

extant taxa only

extant + fossils

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Parameter Mesozoic Cenozoic

rate (σ2) 0.97 0.1

faster rates of body size evolution in the Cenozoic?

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Brownian motion is a diversifying process

time

ph

en

oty

pe

rate σ2

starting state starting state

σ2 * time

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time

ph

en

oty

pe

σ2 / 2α

rubber band parameter α

OU is an equilibrium process

rate σ2

starting state starting state

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time

ph

en

oty

pe

Brownian motionOrnstein-Uhlenbeck

BM and OU simulated at the same rate give very different disparities

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the OU process has an equilibrium disparity

ln(b

ody m

ass

) dis

pari

ty

Mesozoic CenozoicT J PgK Ng

α= 0.01σ2 = 0.97

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Mesozoic CenozoicT J PgK Ng

a low BM rate increases disparityln

(body m

ass

) dis

pari

ty

σ2 = 0.1α= 0.01σ2 = 0.97

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Do we really think the Tempo of mammalian

body size evolution increased after the K-

PG extinction?

Variation in the Mode of evolution is a more intuitive and

more likely explanation that

variation in Tempo

Page 32: Graham Slater's 2013 SVP talk

Do we really think the Tempo of mammalian

body size evolution increased after the K-

PG extinction?

Page 33: Graham Slater's 2013 SVP talk

How fast do animals evolve? That is one of

the fundamental questions regarding evolution.

Photo: Florida Museum of Natural History

Simpson (1944, 1953)

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Page 35: Graham Slater's 2013 SVP talk

From Simpson (1953)

Simpson’s adaptive zones


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