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This is Georgie Bites with 
Oliver Strimpel. 

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The history of the Earth's 
climate is archived within the 

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sedimentary record. 
That is because there are 

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certain physical, chemical and 
biological properties of 

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sedimentary rocks that can serve
as indicators or proxies of the 

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climate that prevailed when they
were deposited. 

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Over the past few decades, we've
discovered more and more 

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proxies, enabling us to probe 
more aspects of past 

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environments such as the 
temperature and composition of 

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the atmosphere and of the 
oceans, sea level, the presence 

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and extent of ice caps, and even
patterns of wind and rainfall. 

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But now there is a heightened 
interest in such work, since we 

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want to understand what the 
rapid human generated rise in 

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carbon dioxide means for the 
planet. 

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Isabel Montagnez has been 
reconstructing past global and 

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regional climates throughout her
30 year research career. 

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She is a Distinguished Professor
of Earth and Planetary Sciences 

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and Director of the Institute of
the Environment at the 

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University of California, Davis.
One climate period in particular

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has attracted her attention, the
late Paleozoic Ice Age. 

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That is because in certain key 
respects, it can serve as an 

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analogue of the present day. 
It was the only time in Earth 

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history when carbon dioxide 
levels increased abruptly during

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a period of recurrent 
glaciation. 

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That Ice Age eventually gave way
to a much warmer greenhouse, 

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Earth devoid of ice. 
Isabel Montanez, welcome to 

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Geology Bytes. 
Thank you, Oliver. 

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It's a pleasure to join you 
today. 

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It's impressive that we can 
reconstruct such apparently 

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evanescent things as atmospheric
temperature and global sea level

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through geological time. 
I said that we use evermore 

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proxies for this purpose. 
Can you tell us what these 

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proxies are? 
And let's start with the 

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traditional ones. 
So some of these proxies that 

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we've been using for decades now
are oxygen isotopes of fossils 

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of marine shells and corals that
formed in the ocean, and equally

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as many for minerals that form 
in ancient soils on land. 

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And these can give us 
information like local surface 

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temperature and the composition 
of the seawater at the time or 

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of rainwater in which they 
formed and the carbon isotopic 

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composition, which we typically 
do with the oxygen, sometimes 

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elemental concentrations of 
these minerals. 

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Then when we combine all those 
together, it provides 

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information on the local 
temperatures, humidity, rainfall

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patterns. 
And I think one that is 

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particularly important is how we
reconstruct CO2 in the past. 

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And there are probably nearly a 
dozen approaches to 

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reconstructing CO2 in the past. 
All of them involve fossils of 

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living organisms or minerals 
that are forming in the oceans 

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or on land. 
And each of those has their 

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weaknesses and strengths. 
So we typically use multiple of 

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these proxies, like we might use
the minerals and soils and the 

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plants that form in the 
ecosystems associated with those

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soils and they will then 
together give us pretty good 

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constraints on what CO2 in the 
atmosphere was in the past. 

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Can you pick a few of the most 
important proxies and explain 

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the physical mechanisms or 
chemical mechanisms by which 

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they managed to record things 
like CO2 level or temperature? 

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Yeah. 
In the oceans, the proxies of 

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CO2 typically involve the 
isotopic composition of marine 

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shells. 
And why do they do that? 

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Because these isotopic 
compositions are very sensitive 

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to the pH of the sea water. 
And in turn, the pH is a good 

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recorder of how much CO2 the 
ocean is dissolving. 

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You know, the ocean is like a 
big sponge and it is always 

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absorbing CO2. 
It is limited by how much it can

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take by the other carbon of 
chemicals in the ocean. 

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So pH is a good indicator of 
what the balance of those other 

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carbon molecules are. 
If we can reconstruct pH and we 

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can reconstruct another 
component of the ocean, like how

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much one of these dissolved 
carbon molecules were in there, 

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then we can reconstruct CO2 in 
the atmosphere. 

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And what's really exciting is 
we've done this mostly on using 

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these micro fossils called 
foraminifera and it's worked 

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very, very well. 
Some of the best estimates of 

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CO2 in the past, unfortunately 
those former menifer have only 

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existed the last at best couple 
100 million years and that means

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we have this big void prior to 
that. 

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And just literally if a month 
ago someone has shown how well 

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this works on fossil 
brachiopods. 

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So that has really now expanded 
our ability to use that type of 

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CO2 proxy way back to 500 
million years on land. 

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There are several different 
approaches, but two of the best 

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are those carbonate minerals, we
call them pedogenic or soil 

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formed carbonates in soils and 
they are in any soils that 

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formed in relatively drier 
conditions. 

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So the southwest of the US would
be a good example, Africa, 

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Brazil. 
And these form around roots 

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because roots respires CO2 at 
night and that CO2 gets 

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dissolved in the poor waters of 
the soil and they get 

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oversaturated and that comes out
as a new mineral carbonate. 

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The very cool thing about soils 
is that there is a balance of 

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how much of the CO2 in the soil 
is from those roots respiring or

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microbes respiring in the soil, 
and how much is actually 

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infiltrated from the atmosphere.
And the balance of the 

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atmospheric CO2 versus the soil 
form CO2 is recorded in the 

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carbon isotopes of the carbonate
mineral as well as the organic 

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matter in the soil. 
And that can be then used to 

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reconstruct CO2 in the 
atmosphere. 

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And then the other one that I 
think it's just so elegant, but 

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very straightforward and that is
that all plants, vascular plants

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that have formed since you've 
440 million years ago or so, 

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have breathing pores on their 
leaves or on their stems, what 

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we call stomata. 
They are little holes where 

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water comes out because plants 
transpire water, but it's also 

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where they take in CO2 from the 
atmosphere to photosynthesize. 

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And so there is a very simple 
inverse relationship by how much

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CO2 is in the atmosphere and how
many of those pores they have on

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their leaves or stems. 
If there isn't a lot of CO2 in 

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the atmosphere, they need lots 
of those pores to be sure that 

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they get enough CO2. 
And vice versa, if there's a lot

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of CO2 in the atmosphere, they 
don't need as many of them. 

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And it's to their advantage to 
not have too many because as I 

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mentioned, they lose water 
through these pores and they 

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don't want to lose water, 
especially if it's getting drier

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in seasonally or with time. 
And it's a very tight connection

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between the amount of CO2 in the
atmosphere in those pores that 

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develop. 
And we simply use how many pores

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per square millimeter on a leaf.
We're not talking about proxies 

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based on isotopes. 
Why should they be sensitive to 

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these environmental parameters? 
Is it something to do with the 

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reaction kinetics of the 
different weight of the 

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different carbons in the carbon 
dioxide from the different 

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isotopes? 
Absolutely. 

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The proportion of the heavier 
versus the lighter isotope into 

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the mineral, for instance, will 
have a lot to do with 

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temperature. 
And if there are other 

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parameters in the soil or in the
water that are affecting the 

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rate at which those atoms are 
being brought in, yes, that will

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also affect it. 
It's a lot easier to move or 

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incorporate the lighter isotope 
than it is a heavier mass. 

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For plants, it's a bit more 
complicated in that it has to do

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with their physiological 
functioning. 

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How well are they taking in CO2 
or photosynthesizing and 

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processing it? 
Does any of the material you 

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analyze for these proxies 
include the actual original 

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organic matter from these 
skeletons, or from these leaves 

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that survives, or the soil? 
Or are you just talking about 

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the replaced material that 
generally forms a fossil? 

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Great question. 
Minerals in soils, very, very 

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small minerals will often form 
effectively cages around this 

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organic matter and we call it 
mineral associated organic 

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matter. 
Now millions of years ago, sure 

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it's not preserving it 
perfectly, but it is pretty 

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impressive how most of the 
molecular structure that it can 

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preserve. 
And another way is these 

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carbonates that form in the soil
actually entomb the organic 

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matter that was in the soil as 
they were precipitating for 

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plants. 
It isn't in fact, the actual 

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cellulose or lipids of the 
actual leaf. 

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It's that waxy layer, a 
cuticular layer that protects 

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the leaf. 
And there's a layer on the 

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bottom of the leaf and there's a
layer on the top of the leaf. 

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So effectively, those breathing 
pores that we measure their 

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sizes, their depths, and the 
number of them on the leaf. 

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They're casts in that waxy 
cuticular layer and that is 

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preserved beautifully. 
I can show you images from a 

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microscope of something 300 
million years old and a ginkgo 

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from 100 million years and a 
modern one, and you'd be hard 

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pressed to know the difference. 
Wow, that's amazing. 

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The actual original wax 
material. 

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It is and we have even extracted
from them some of those lipids, 

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so you do get things stuck on 
there that are preserved. 

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Can you tell us about some of 
the more recently developed 

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nontraditional proxies? 
The turn of the Millennium has 

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been an explosion of development
of new proxies. 

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I think we can attribute a lot 
of that to the technology, the 

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machines that give us the 
possibility to do isotopes 

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across the periodic table. 
It's just amazing. 

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It's something that 40 years ago
we couldn't have even imagined. 

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I'll give you a couple of 
examples. 

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Uranium isotopes in carbonates 
that form in the ocean, and even

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some people are trying this in 
lakes. 

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These are now allowing us to 
look at the oxygenation levels 

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on the ocean floor where a lot 
of these shells and life might 

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be living. 
Today. 

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Our deep ocean is quite 
oxygenated, but it turns out 

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that when you have global 
warming, that changes 

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considerably. 
So these uranium isotopes that 

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are now measurable in these 
shells or even just disseminated

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carbonates in old sediments, 
allow us to see how the 

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oxygenation is changed, whether 
anoxic conditions are forming 

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anywhere on the sea floor, 
whether it's off a coast or deep

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in the ocean. 
And in turn, it tells us about 

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how changes in the ocean 
circulation were happening. 

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And the very cool thing about 
uranium isotopes is you can do 

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those in one location on Earth 
and it's representative of the 

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whole ocean because of the well 
mixed nature and the residence 

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time of uranium in the oceans. 
Another example, going back to 

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the periodic table, we now do 
the stable isotopic compositions

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of strontium, calcium, 
magnesium, lithium, potassium, 

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mercury, and these allow us to 
look at degrees of weathering on

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land, which is really important 
because weathering on land is 

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tightly coupled to CO2 in the 
atmosphere and to temperature. 

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So this gives us an opportunity 
to again, track what's happening

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in changes in greenhouse gases 
that we're getting from other 

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proxies and how is the landscape
responding. 

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And that's important because 
those responses in turn remove 

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CO2 from the atmosphere. 
In fact, it's one of the ways 

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that the Earth has maintained 
its temperatures through 

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maintaining its greenhouse gases
in these balances of these 

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processes, Mercury isotopes, 
fingerprints of passive volcanic

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episodes, so we can now tie them
directly to the other isotopes. 

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Was the increase in CO2 or 
methane in the atmosphere driven

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by volcanism? 
These same isotopes are telling 

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us something about aridity and 
seasonality on land in different

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places, and they can even tell 
us about other sources of 

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greenhouse gases that aren't 
volcanoes, like melting methane 

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out of the oceans. 
So it really opens up a whole 

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new world for us beyond just 
temperatures, effective moisture

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and maybe seawater and 
precipitation composition. 

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And then lastly, I'd be remiss 
if I didn't say they're all of 

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these biologic proxies, 
primarily what we call 

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biomarkers. 
Those are biomolecules. 

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So rather than looking at the 
organic matter that we extract 

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as a bulk form, we can actually 
extract specific biomolecules 

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like lipids, hope pains and 
others. 

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And each of them have their own 
function. 

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So we can look at things like 
the physiological functioning of

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the plants, how did they respond
to drought, Were they very 

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resilient to deep freezes. 
But we can also look at 

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microbial interactions with all 
of these other environmental 

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conditions and their role and 
temperatures. 

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They're another independent 
source of temperatures as well. 

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So all of this tool bag, no one 
group will do all of them, but 

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for any given time period there 
are just enormous amounts of 

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information that is being 
developed. 

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So how do you try and make sense
of all the paleoclimate data 

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you've been able to reconstruct 
from all these proxies? 

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So our approach is to 
contextualize that data by using

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an Earth system model. 
This model, which was produced 

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by the National Center for 
Atmospheric Research, or NCAR, 

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is our US model for the IPCC's 
work, but also for predicting 

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the climate over the next 10 
days. 

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They are the most comprehensive,
all inclusive of every process 

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that is in the ocean, the 
atmosphere on land that we know 

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of that influences climate. 
Climate is effectively the 

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interaction of the ocean and the
atmosphere. 

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So these models not only allow 
the ocean and the atmosphere to 

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interact and be fully in 
equilibrium, it allows for cloud

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differences and development. 
It allows for aerosols. 

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It models all of the changes in 
the circulation of the ocean, 

243
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the effects of sea ice on that 
circulation, continental ice 

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00:16:08,960 --> 00:16:12,600
sheets, how do they influence 
the temperatures, the air 

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humidity, sea ice response, and 
turn back to the ocean? 

246
00:16:17,960 --> 00:16:22,200
It has vegetation. 
Vegetation interacts with the 

247
00:16:22,200 --> 00:16:26,760
atmosphere and the soils in 
terms of moving carbon and 

248
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water. 
So it influences once again the 

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atmosphere and the ocean and it 
just iterates so that these 

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00:16:34,240 --> 00:16:39,840
processes are fully interacting 
and feeding back on one another.

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And the proof that these models 
are really comprehensive and 

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correct is that they are 
calibrated to the modern where 

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00:16:48,560 --> 00:16:52,600
we have 100 plus years of 
excellent data from around the 

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00:16:52,600 --> 00:16:57,720
world and they can reproduce 
those very, very accurately. 

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00:16:58,680 --> 00:17:00,880
OK, so you've managed to build 
this model. 

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How do you make use of it? 
What kind of questions can you 

257
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interrogate it with? 
So you start out with the 

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boundary conditions, those 
baseline boundary conditions, 

259
00:17:10,920 --> 00:17:15,520
and then they are run to 
evaluate the climate processes 

260
00:17:15,520 --> 00:17:19,920
and the ecosystem functioning. 
What is their sensitivity to 

261
00:17:19,920 --> 00:17:23,800
this changing CO2 and ice sheet 
distribution? 

262
00:17:24,280 --> 00:17:26,480
You don't usually change much 
else because you're not 

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interested in whether mountains 
are building or weathering down 

264
00:17:29,320 --> 00:17:32,600
or whether the ocean basins are 
changing in configuration. 

265
00:17:32,800 --> 00:17:34,840
Those are millions a year time 
scale things. 

266
00:17:35,160 --> 00:17:38,040
But you are interested in what 
happens if you lose tropical 

267
00:17:38,040 --> 00:17:41,800
forests or whether temperatures 
are changing and rainfall 

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00:17:41,800 --> 00:17:43,840
patterns are changing. 
So that's what we're after. 

269
00:17:43,840 --> 00:17:47,640
We're interested in seeing what 
is the sensitivity of these. 

270
00:17:48,120 --> 00:17:52,120
We're also interested in are 
there thresholds, are there CO2 

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00:17:52,120 --> 00:17:55,280
thresholds where things just 
plummet or where the changes 

272
00:17:55,280 --> 00:17:58,520
start accelerating? 
And are there tipping points 

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where those forests disappear, 
or where their ice collapses, or

274
00:18:02,920 --> 00:18:05,840
where the monsoon system 
effectively collapses or 

275
00:18:05,840 --> 00:18:08,760
intensifies? 
I said in my introduction that 

276
00:18:08,760 --> 00:18:12,240
you've been especially 
interested in the late Paleozoic

277
00:18:12,240 --> 00:18:17,120
Ice Age because it can serve as 
an analogue to the present day. 

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How far does the similarity go? 
I want to stress that it is the 

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00:18:21,840 --> 00:18:25,600
process scale we're after here. 
Continental configuration was 

280
00:18:25,600 --> 00:18:27,960
quite different. 
In fact, it was the opposite of 

281
00:18:27,960 --> 00:18:29,720
today. 
It was a supercontinent. 

282
00:18:30,000 --> 00:18:33,640
Today we have our continents at 
their maximum distribution away 

283
00:18:33,640 --> 00:18:36,760
from one another on the globe. 
Many things are different. 

284
00:18:37,400 --> 00:18:41,600
That said, the processes in the 
Earth system, whether it's in 

285
00:18:41,600 --> 00:18:45,880
the climate system, the 
ecosystems on land and how they 

286
00:18:45,880 --> 00:18:48,360
interact with the environmental 
parameters. 

287
00:18:48,600 --> 00:18:53,320
So the atmosphere, the oceans, 
land, life, these processes have

288
00:18:53,480 --> 00:18:57,160
existed and fundamentally 
functioned as they do today 

289
00:18:57,240 --> 00:19:01,600
since we've had ecosystems in 
terms of general structure and 

290
00:19:01,600 --> 00:19:04,200
configuration similar to what we
have today. 

291
00:19:04,280 --> 00:19:08,760
So 400 million years or so, 
certainly the last 300 million 

292
00:19:08,760 --> 00:19:12,400
years. 
So inferring how climate may 

293
00:19:12,400 --> 00:19:16,640
change in the future in one 
particular region from looking 

294
00:19:16,640 --> 00:19:19,600
at the deep time, we can't do 
that because of the continental 

295
00:19:19,600 --> 00:19:22,400
configuration differences and 
other things like that. 

296
00:19:23,120 --> 00:19:28,040
But evaluating how these 
processes in the climate system,

297
00:19:28,120 --> 00:19:34,720
in the ecosystems, ice response,
ocean response, evaluating how 

298
00:19:34,720 --> 00:19:40,320
they respond to increases in CO2
or vice versa, decreases and the

299
00:19:40,320 --> 00:19:44,480
consequent warming or cooling 
that goes with that on a global 

300
00:19:44,480 --> 00:19:50,200
scale and how those responses 
interact with one another and 

301
00:19:50,200 --> 00:19:55,480
how they may even feedback on 
the initial warming or cooling, 

302
00:19:55,680 --> 00:19:59,960
that is fundamental information 
that we can glean from looking 

303
00:19:59,960 --> 00:20:04,080
at past periods. 
The main thing that makes a time

304
00:20:04,080 --> 00:20:07,760
period relevant or not is 
whether the atmospheric CO2 

305
00:20:07,760 --> 00:20:12,800
concentrations were within the 
range of what we are seeing 

306
00:20:13,040 --> 00:20:16,800
since we started burning fossil 
fuels and what we project into 

307
00:20:16,800 --> 00:20:21,480
our fairly near future. 
And that is the case for the 

308
00:20:21,480 --> 00:20:26,080
late paleozoric ice house. 
In fact it's the only time when 

309
00:20:26,080 --> 00:20:32,280
CO2 was in the range of what we 
see since the pre industrial and

310
00:20:32,280 --> 00:20:37,000
what we're going into except for
a transient period in the last 

311
00:20:37,000 --> 00:20:40,240
several million years. 
But isn't the fact that there 

312
00:20:40,240 --> 00:20:44,160
was ice or recurrent ice on the 
poles something that also 

313
00:20:44,160 --> 00:20:46,080
distinguished that period from 
others? 

314
00:20:46,160 --> 00:20:50,440
Of course this is the last time 
other than the last 34 million 

315
00:20:50,440 --> 00:20:54,480
years where there has been 
continental scale ice on Earth 

316
00:20:55,000 --> 00:20:57,040
all the time. 
In between there may have been 

317
00:20:57,240 --> 00:21:01,360
ephemeral, short lived, maybe 
small Alpine, maybe continental 

318
00:21:01,360 --> 00:21:05,080
glaciers, but nothing that we 
can find in the rock record nor 

319
00:21:05,080 --> 00:21:08,640
do we produce in climate models.
So this is it. 

320
00:21:08,640 --> 00:21:13,880
This is the last time that we 
see the ice house as it came on 

321
00:21:13,880 --> 00:21:19,680
the onset and its response to 
short lived warming, essentially

322
00:21:19,680 --> 00:21:23,120
the experiment we're doing now 
and ultimately it's terminal 

323
00:21:23,120 --> 00:21:25,760
demise as it turned into a 
greenhouse. 

324
00:21:26,240 --> 00:21:29,200
I want to come back to the 
boundary conditions that you 

325
00:21:29,200 --> 00:21:31,680
mentioned. 
So when the configuration of the

326
00:21:31,680 --> 00:21:34,960
continents was completely 
different and presumably ocean 

327
00:21:34,960 --> 00:21:38,280
circulation as a result was 
completely different, how come 

328
00:21:38,520 --> 00:21:43,400
we believe that the 
sensitivities on a global scale 

329
00:21:43,480 --> 00:21:47,000
would still be relevant to the 
situation we find ourselves in 

330
00:21:47,000 --> 00:21:48,560
today? 
So I'm going to give you an 

331
00:21:48,560 --> 00:21:53,480
example of our modeling that 
gives us detailed seasonal 

332
00:21:53,520 --> 00:21:57,680
response to the CO2 changes 
within that range of the pre 

333
00:21:57,680 --> 00:22:00,360
industrial to what we anticipate
in the future. 

334
00:22:01,040 --> 00:22:05,560
And then how we can say that we 
have confidence in that modeling

335
00:22:05,560 --> 00:22:07,800
based on the proxies that we've 
developed. 

336
00:22:08,520 --> 00:22:11,760
We have the CO2 proxies, we have
the temperature proxies for the 

337
00:22:11,760 --> 00:22:14,760
late Pilozoic Ice Age. 
And now we had these uranium 

338
00:22:14,760 --> 00:22:17,840
isotopes and the uranium 
isotopes were telling us that up

339
00:22:17,840 --> 00:22:22,400
to 25% of the sea floor was 
going anoxic globe. 

340
00:22:23,000 --> 00:22:25,760
Yes, different continental 
configuration, so clearly 

341
00:22:25,760 --> 00:22:30,800
different ocean circulation and 
with ice sheets and we said this

342
00:22:30,800 --> 00:22:36,200
is during ice house where we 
have big ice where we are 

343
00:22:36,240 --> 00:22:38,520
generally cool. 
In fact, other studies we've 

344
00:22:38,520 --> 00:22:40,960
done have shown that this is the
only other time that global 

345
00:22:40,960 --> 00:22:43,800
temperatures on in line with 
what we're humans have been 

346
00:22:43,800 --> 00:22:45,920
seeing since they've evolved in 
today. 

347
00:22:46,720 --> 00:22:50,040
Why are we going 25% anoxic of 
the sea floor? 

348
00:22:50,040 --> 00:22:53,040
That's phenomenal. 
That has huge implications for 

349
00:22:53,040 --> 00:22:56,280
the future if correct. 
So the climate models, we use 

350
00:22:56,280 --> 00:23:01,080
them with the right boundary 
conditions to evaluate how the 

351
00:23:01,080 --> 00:23:05,480
presence of ice and sea ice 
included would change the ocean 

352
00:23:05,480 --> 00:23:08,440
circulation. 
Despite the fact that again we 

353
00:23:08,440 --> 00:23:11,400
are looking at very different 
continental configurations and 

354
00:23:11,400 --> 00:23:15,480
ice only in the Southern 
Hemisphere with the doubling of 

355
00:23:15,480 --> 00:23:20,240
CO2 or even 50% increase 
essentially where we are today 

356
00:23:20,600 --> 00:23:24,600
from pre industrial, we can see 
changes for instance in the 

357
00:23:24,600 --> 00:23:28,680
Northern hemisphere polar 
region, major changes in sea ice

358
00:23:28,720 --> 00:23:33,120
formation, but more importantly 
in circulation at the mid depth 

359
00:23:33,400 --> 00:23:38,080
of the ocean, we can see where 
deep water formation is forming.

360
00:23:38,760 --> 00:23:42,680
So during the times of low CO2, 
we have deep water formation at 

361
00:23:42,680 --> 00:23:45,880
both poles, very similar to 
today, even though the 

362
00:23:45,880 --> 00:23:49,920
continents in their very 
different configuration, we take

363
00:23:49,920 --> 00:23:53,480
the CO2, we double it and we 
lose the Northern hemisphere 

364
00:23:53,480 --> 00:23:55,920
deep water formation, very 
different world. 

365
00:23:55,920 --> 00:23:59,040
And we see that then in the 
climate on land and we see in 

366
00:23:59,040 --> 00:24:03,680
the sea surface temperatures, we
do a 50% increase in CO2 to make

367
00:24:03,680 --> 00:24:07,040
it more like today, 400 PPM. 
And what do we discover? 

368
00:24:07,240 --> 00:24:11,200
It's a threshold because under 
that we're not seeing much 

369
00:24:11,200 --> 00:24:14,280
change. 
At 400, all of a sudden we see 

370
00:24:14,280 --> 00:24:16,880
these major changes and not much
more. 

371
00:24:17,000 --> 00:24:20,720
Even when we double go 50% more,
and it fits our proxies 

372
00:24:20,720 --> 00:24:25,040
beautifully, it tells us that 
about 18 to 25% of the sea floor

373
00:24:25,040 --> 00:24:27,640
would go anoxic because of this 
change. 

374
00:24:28,600 --> 00:24:31,840
So again, different boundary 
conditions in terms of 

375
00:24:31,840 --> 00:24:36,480
continental configuration has to
be different ocean circulation 

376
00:24:36,480 --> 00:24:40,120
because you have one huge ocean 
called Panthelasa and then a 

377
00:24:40,120 --> 00:24:43,720
more huge Mediterranean. 
That's the other part of the 

378
00:24:43,720 --> 00:24:47,640
ocean, open to the other one, 
but still very different. 

379
00:24:48,360 --> 00:24:52,680
But what have we learned? 
It doesn't matter the ocean, it 

380
00:24:52,680 --> 00:24:56,040
circulates and it still couples 
with the atmosphere, and it is 

381
00:24:56,040 --> 00:24:59,480
still equally sensitive to 
changes in CO2. 

382
00:24:59,760 --> 00:25:03,800
Where the water may go down deep
to circulate in our conveyor 

383
00:25:03,800 --> 00:25:07,840
belt may be different, but it's 
not about where those continents

384
00:25:07,840 --> 00:25:09,960
are. 
It's about the CO2 and the 

385
00:25:09,960 --> 00:25:14,560
warming effect on the ocean and 
the ice and sea ice behaviour 

386
00:25:15,160 --> 00:25:18,720
that seems to be robust 
regardless of that boundary 

387
00:25:18,720 --> 00:25:21,720
conditions of the continent. 
Wow, That's a pretty dramatic 

388
00:25:21,760 --> 00:25:27,040
conclusion then, that it just so
happens based on your model that

389
00:25:27,120 --> 00:25:28,840
we've gotten to the tipping 
point. 

390
00:25:29,440 --> 00:25:33,040
You can imagine we put that out 
there and the default response 

391
00:25:33,040 --> 00:25:35,880
by scientists is, oh, come on, 
it's so different back then. 

392
00:25:35,920 --> 00:25:41,400
And our response back is yes, 
but step back and ask yourself 

393
00:25:41,400 --> 00:25:44,520
why the responses are not that 
different. 

394
00:25:45,120 --> 00:25:49,840
It's because there are physics 
in the system that don't care 

395
00:25:49,840 --> 00:25:53,640
where the continents are. 
They care about the ocean as a 

396
00:25:53,640 --> 00:25:57,560
whole and how it's operating. 
It's always a conveyor belt. 

397
00:25:57,800 --> 00:26:01,640
It may slow down, it may 
accelerate, but it's still a 

398
00:26:01,680 --> 00:26:06,720
conveyor belt that is strongly 
governed by how much sea ice is 

399
00:26:06,800 --> 00:26:10,320
in the polar regions, how much 
continental ice is there, how 

400
00:26:10,320 --> 00:26:15,520
warm the ocean is in that 
region, how stratified it is. 

401
00:26:16,160 --> 00:26:19,640
So nuanced differences, yes, 
hugely. 

402
00:26:19,800 --> 00:26:23,160
But as a global system, it's 
still operating as the systems 

403
00:26:23,320 --> 00:26:27,840
as we know it. 
What can we learn then from your

404
00:26:27,840 --> 00:26:33,480
late Paleozoic Ice Age or ice 
house model with regard to our 

405
00:26:33,480 --> 00:26:38,160
climate future and I presume one
of the differences that even 

406
00:26:38,160 --> 00:26:43,400
though CO2 was rising rapidly 
than it was not rising on 

407
00:26:43,520 --> 00:26:47,360
anything like the rate that has 
happened since pre industrial 

408
00:26:47,360 --> 00:26:49,680
times? 
You hit the nail on the head. 

409
00:26:49,720 --> 00:26:53,960
I would say two key findings. 
Just by changing the climate 

410
00:26:53,960 --> 00:26:59,720
initially, and if the ecosystem 
in a given location is changed, 

411
00:27:00,000 --> 00:27:04,120
we can actually change other 
parameters in the Earth system 

412
00:27:04,320 --> 00:27:08,160
substantially. 
For example, we've modeled that 

413
00:27:08,160 --> 00:27:13,520
if we changed the ecosystem in 
the tropics, the wet tropics at 

414
00:27:13,520 --> 00:27:18,520
that time, by moving one type of
ecosystem and replacing it with 

415
00:27:18,520 --> 00:27:22,400
another, based on the fossil 
record that these shifts really 

416
00:27:22,400 --> 00:27:28,080
happened, we could change the 
outflow from the Amazon basin by

417
00:27:28,080 --> 00:27:35,600
fourfold or decrease it by half.
So changing the ecosystem in a 

418
00:27:35,600 --> 00:27:38,840
given location can change our 
runoff. 

419
00:27:39,360 --> 00:27:43,960
So flooding it can change the 
coastal environment because it 

420
00:27:43,960 --> 00:27:46,880
can bring a lot of nutrients to 
coastal waters. 

421
00:27:46,880 --> 00:27:50,000
That is not a good thing. 
It causes eutrophication. 

422
00:27:50,280 --> 00:27:54,360
It can change the atmosphere's 
water because it can put less in

423
00:27:54,360 --> 00:27:57,480
the atmosphere and more in the 
ground to run off. 

424
00:27:58,080 --> 00:28:01,920
So that's a big finding. 
We're looking at a time period 

425
00:28:02,440 --> 00:28:06,800
similar to Dave in terms of ice 
sheets, where CO2 was at its low

426
00:28:06,800 --> 00:28:11,240
point, precisely in the range of
the lows of the last glacials 

427
00:28:11,240 --> 00:28:13,720
during the Pleistocene, the last
million years. 

428
00:28:14,160 --> 00:28:18,480
And it rose within these glacial
interglacial cycles, similarly 

429
00:28:18,480 --> 00:28:20,840
doubling. 
But there were also these 

430
00:28:20,840 --> 00:28:26,080
intervals of rapid rises in CO2 
that were driven by volcanism 

431
00:28:26,120 --> 00:28:29,280
and maybe even changes in ocean 
circulation. 

432
00:28:30,000 --> 00:28:34,480
The important thing here is that
we are seeing enormous changes 

433
00:28:34,640 --> 00:28:38,280
in the climate system, 
influences on the ecosystems and

434
00:28:38,280 --> 00:28:41,960
land in the ocean, changes in 
the oxygenation state of the 

435
00:28:42,040 --> 00:28:47,880
oceans, changes in ice sheet 
stability, all in response to 

436
00:28:47,880 --> 00:28:52,560
these changes in CO2 within the 
range of our pre industrial 

437
00:28:52,840 --> 00:28:56,600
Pleistocene to our future. 
And as you said, at rates 

438
00:28:56,600 --> 00:28:59,520
minimally an order of magnitude 
slower. 

439
00:28:59,880 --> 00:29:04,080
And that should be eye opening 
that our Earth system is capable

440
00:29:04,560 --> 00:29:09,840
of responding to changes in CO2 
analogous to our world and 

441
00:29:09,840 --> 00:29:13,600
future at all. 
Because we should be thinking, 

442
00:29:13,600 --> 00:29:17,800
why would it not be now? 
Isabel Montanez, thank you very 

443
00:29:17,800 --> 00:29:19,560
much. 
It's very much my pleasure. 

444
00:29:20,800 --> 00:29:23,480
To see pictures and 
illustrations that support this 

445
00:29:23,480 --> 00:29:28,720
podcast, go to geologybytescom 
where you'll also find a subject

446
00:29:28,720 --> 00:29:30,640
matter index of all the 
episodes. 

447
00:29:31,080 --> 00:29:34,600
There you can also give me 
feedback which I welcome as well

448
00:29:34,600 --> 00:29:37,440
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