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We hope you have enjoyed this limited-length demo
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1. The deep history of life
- Prof. Andrew H. Knoll
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2. The neutral and nearly neutral theories of molecular evolution 2
- Prof. Joseph P. Bielawski
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3. The neutral and nearly neutral theories of molecular evolution 1
- Prof. Joseph P. Bielawski
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4. The coalescent
- Prof. Peter Beerli
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5. Evolution of drug resistance
- Dr. Pleuni Pennings
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6. Trends in macroevolution
- Prof. Luke Harmon
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7. Social evolution
- Prof. Dustin R. Rubenstein
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8. Principles of phylogeography and landscape genetics
- Dr. Ryan Garrick
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9. Evolutionary developmental biology
- Dr. Karen Sears
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10. Biogeography: explaining the geographical distribution of organisms
- Prof. Alexandre Antonelli
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11. Evolutionary case study: the genomics of speciation in Heliconius butterflies
- Prof. Adriana D. Briscoe
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12. Human evolution
- Prof. Vagheesh Narasimhan
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13. How do organisms evolve in response to global change?
- Prof. Erica Bree Rosenblum
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14. Conservation genomics: adaptation and gene flow
- Prof. Jacob Höglund
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15. Conservation genomics: genetic diversity and inbreeding
- Dr. Jacqueline Robinson
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16. Evolution of agriculture: the origin of our food crops
- Dr. Mona Schreiber
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17. Evolutionary medicine
- Prof. Stephen C. Stearns
Printable Handouts
Navigable Slide Index
- Introduction
- Life’s deep history: perspective from phylogeny
- A record of early microbial life
- Sedimentary rocks as history books
- Microfossils
- Stromatolites (1)
- Chemical clues
- Bil’yakh Group, Northern Siberia: ~1500 Ma
- The Warrawoona Group, Australia: life at 3460 Ma?
- Stromatolites (2)
- Chemical signatures of early life: C and S isotopes
- Rock chemistry records: Earth’s redox history
- Why were oxygen levels so low?
- Oxygen accumulation through time
- Biological consequences of GOE
- A new type of cell emerges: eukaryotes
- Recognizing Proterozoic microfossils as eukaryotic
- Roper Group, Australia: 1500–1400 Ma
- Functional interpretation: Tappania plana
- Valeria lophostriata, Satka favosa
- Mid-Proterozoic macrofossils
- Circa 1047 Ma Bangiomorpha
- 800 Ma: building diversity
- Predation and eukaryotic diversification
- Testate microfossils: in ca. 750 Ma rocks
- Scale microfossils
- Ediacaran Period (635–541 Ma)
- Green algae: important in marine phytoplankton
- The influence of nutrient levels
- Let’s look at phosphorus
- Consequences of increased phosphorus levels
- More food, more oxygen, and a world that supports large animals
- Conclusions
- Thank you!
Topics Covered
- Phylogeny
- Fossils and micro- and macrofossils
- Bacteria, archaea and eukaryotes
- Records of early microbial life
- Sedimentary rocks
- Stromatolites
- Molecular biomarkers for life
- Isotopic compositions of sedimentary carbonates
- Earth’s redox history
- Early Earth and oxygen levels
- Predation and early eukaryotic diversification
- Phosphorus levels
Talk Citation
Knoll, A.H. (2023, September 28). The deep history of life [Video file]. In The Biomedical & Life Sciences Collection, Henry Stewart Talks. Retrieved December 21, 2024, from https://doi.org/10.69645/YHGF9986.Export Citation (RIS)
Publication History
Financial Disclosures
- Prof. Andrew H. Knoll has not informed HSTalks of any commercial/financial relationship that it is appropriate to disclose.
A selection of talks on Plant & Animal Sciences
Transcript
Please wait while the transcript is being prepared...
0:00
Hello, my name is Andrew Knoll.
I am a Professor of
Earth Science and Biology
at Harvard University.
Today I'd like to talk about
"The Deep History of Life".
Now spoiler alert.
What most people call the
deep history of life.
You will see is actually most
of the history of
life on our planet.
Our familiar world of plants
and animals is actually
a fairly recent development
in our planet's history.
For most of its history,
the Earth has been an
alien place physically.
It has been a microbial
planet biologically.
0:39
Let's begin with a little
bit of perspective.
Most of you know something
about the fossil record.
If nothing else, you know that
dinosaurs once ruled
landscapes on this planet.
If you know a little bit more,
you may know that long
before there were dinosaurs,
animals like trilobites,
distant relatives of
shrimp and crabs,
swam in ancient oceans.
Now, it turns out that if we
could weigh all the
organisms alive today,
you'd find that only a
very small proportion
of that weight would
be made up of animals,
much less than 1%.
It's estimated that
there's something like
30 tons of bacteria for
every ton of animals.
If we look at the diagram,
that's something called
a universal phylogeny.
It's a hypothesis of
the evolutionary relationships
of all organisms,
from humans to bacteria
based on comparisons
of molecular sequences
for DNA and proteins.
The one thing I want to
call your attention to
in this diagram is on
the right with the star and
the arrow that
represents animals.
It turns out that all the
animals that have ever lived,
from trilobites to
dinosaurs to you reside
on one short distal
branch of the tree.
The same thing is
true of plants,
but there are many branches that
precede the branch that
gave rise to animals.
The inference from
this is that life
existed long before
animals first appeared,
and that that life
was mostly microbial.
Now if we look at the
time line on the right,
we can see that the oldest
fossil evidence for animals
is about 575 million years old.
Yet our planet is more than
4.5 billion years old.
Which raises the question
of what was going
on between the origin
of the planet and the
origin of animals.
From the phylogeny, we
should estimate that
there was life through
at least part of
this interval and that
life was microbial.
That then raises a real
empirical question
if the deep history
of life is microbial.
Can such tiny and
evanescent organisms like
bacteria leave a decipherable
record in the rock record?