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This is Geology Bytes with 
Oliver Strimple Compared to our 

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neighbours in the solar system, 
the Earth has experienced A 

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remarkably constant temperature 
over the four and a half billion

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years since its creation. 
Venus has experienced runaway 

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heating with surface 
temperatures of about 460°C, 

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while on Mars the temperature 
fluctuates between 20 and 

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-150°C. 
We owe this relative temperature

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stability to our atmosphere, 
which contains greenhouse gases 

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such as carbon dioxide that are 
transparent to visible and near 

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infrared light but opaque to 
thermal infrared. 

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Too little of such gases and the
Earth turns into a snowball. 

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Too much and the planet cooks. 
Since volcanoes continuously 

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inject greenhouse gases into the
atmosphere, the relative 

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temperature stability of the 
Earth implies that some feedback

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mechanism regulates the amount 
of greenhouse gas in the 

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atmosphere. 
It is widely accepted that over 

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geological time, this 
atmospheric thermostatic control

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is provided principally by the 
weathering of rocks containing 

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silicate minerals, a process 
that draws carbon dioxide out of

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the atmosphere. 
But how exactly does this 

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process function to regulate 
atmospheric temperature? 

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And how does it depend on the 
changes that have occurred 

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through geological time, such as
the growth of continental crust,

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the formation and destruction of
supercontinents, and the rise 

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and fall of mountain chains? 
Susan Brantley has conducted 

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extensive studies of the 
reactions between water and rock

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in the field and in the lab. 
Recently, she has scaled up our 

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findings to a regional and 
global scale so as to estimate 

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the overall temperature 
sensitivity of the Earth to 

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silicate rock weathering. 
She is a professor in the 

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Department of Geosciences at 
Pennsylvania State University. 

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Susan Brantley, Welcome to 
Geology Bytes. 

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Thanks, Oliver. 
Nice to talk to you this 

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morning. 
Can you remind us as to what 

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chemical processes are 
responsible for the weathering 

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of a silicate rock and how that 
removes carbon dioxide from the 

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atmosphere? 
Sure, When rock comes to the 

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surface of the Earth, when it's 
exposed, it first has to 

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fracture and break apart. 
That makes the surface exposed 

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to air and water, and then 
minerals dissolve in the air and

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water. 
And that dissolution for 

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silicate rocks pulls carbon 
dioxide out of the atmosphere 

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and then holds it dissolved in 
the water. 

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And then that water runs out of 
the soil and joins a stream and 

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flows in a stream to the ocean. 
And eventually, over geologic 

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time, that CO2 that was in the 
water recombines with calcium or

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magnesium in the ocean and then 
precipitates as carbonate rock. 

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So really it's a sequestration 
process that produces rock out 

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of the CO2 in the atmosphere. 
But this process operates over 

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geological time, so how do you 
go about studying this in the 

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lab? 
You take a flask and put some 

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rock powder, you know, rock that
you've ground up into the flask.

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And then you measure how the 
water chemistry changes with 

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time. 
And then sometimes we might take

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a column and put the rock powder
in the column and flow the water

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through. 
But either way, you're looking 

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at how the chemistry of the 
water changes with time and you 

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try to do that in a very 
controlled way in the 

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laboratory. 
And then if you look at that and

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change different minerals or you
change the conditions, the 

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chemistry of the water or the 
temperature, you can really 

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start to create a data set of 
rock weathering or mineral 

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weathering based on laboratory 
data. 

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Did you run these dissolution 
experiments by grinding up 

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different rock types, For 
example granite and basalt? 

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We wanted to make it even more 
simple by isolating not just the

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rock type, but whatever mineral 
was in the rock. 

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So granite, for example, is 
mostly feldspar and quartz, 

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let's say. 
So we might just grind up the 

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feldspar and look at how the 
feldspar dissolves. 

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And basalt can have feldspar, it
can have olivine, it can have 

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pyroxene. 
But if we separate the minerals 

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and we thought we could have a 
very precise measure of the 

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dissolution rates of individual 
minerals and then we should be 

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able to put those back together 
in some kind of model to make 

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predictions that predict how 
fast the weathering is happening

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out there in that soil that 
you're digging in your backyard.

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One of the things you were 
looking for was to see how 

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temperature dependent these 
various processes are. 

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What did you find on that score?
In almost every case, as you 

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increase the temperature, 
certainly for the silicates, 

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minerals dissolve faster and so 
there's a standard process by 

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which you measure some chemical 
process as a function of 

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temperature and then calculate 
the temperature dependence. 

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So the temperature sensitivity, 
and with that temperature 

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sensitivity you can suggest, but
any temperature you want to 

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extrapolate to down in 
temperature, up in temperature, 

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how fast the rate should 
proceed. 

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So we've done that with a number
of minerals, and my lab only 

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produced a relatively small 
number of rates. 

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But if you compile those with 
all the data collected by people

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around the world, there's a 
pretty hefty data set now for 

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mineral dissolution rates. 
And can you give me a ballpark 

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of how that rate varies with 
temperature? 

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The rate double S with 10s of 
degrees of temperature rise. 

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It is a significant effect what 
the temperature does to the 

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process, and so that's very 
important when you start to 

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think about how the Earth Thermo
regulates how the Earth's global

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temperature has been regulated 
over time. 

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I said in the introduction that 
you've just been scaling up the 

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findings in the lab up to a 
regional and even global scale. 

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So how can you actually apply a 
lab result to the incredibly 

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messy and complicated and 
diverse situation that prevails 

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on a global scale? 
There's lots of papers in the 

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literature where people measured
the temperature dependence of 

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dissolution in the laboratory, 
and then there's some estimates 

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for the temperature dependence 
of dissolution. 

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You know, weathering in soils. 
And then there's temperature 

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dependences that have been 
measured for watersheds, and in 

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general they contradict one 
another. 

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I would like to be able to make 
those numbers make sense one to 

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the other. 
And so I moved from just 

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measuring in the laboratory to 
actually looking at how can we 

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measure weathering in the soils?
And then most recently, how can 

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we measure weathering in 
watersheds? 

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And so I've tried to answer the 
question that you just asked me 

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in both directions. 
I've done it from the direction 

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of can I predict it from the 
laboratory? 

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And then I've done it from the 
perspective of what can you 

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measure in the field and then 
pull out of that field 

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measurement, what is a number 
that is comparable to something 

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in the laboratory. 
And with those two approaches, 

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you can start to make some sense
out of this puzzle. 

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Let's look at different 
environments. 

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You have, say, a relatively flat
river, plain or floodplain, and 

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then you would have a 
mountainous region. 

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I mean, how did you subdivide 
the surface of the earth in 

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order to be able to do this 
scaling up? 

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Under some conditions be the 
overall rate of weathering is 

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limited by one process or 
another. 

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So you just said what about in 
floodplains sort of flatlands 

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versus mountainous areas. 
In the flatlands, sometimes what

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we see is very, very thick soils
that are depleted of the 

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minerals of interest. 
So they're depleted of 

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Feldspar's for example. 
And that's because the soil is 

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shielding the reactive minerals 
that are at depth from corrosive

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rainwater, basically. 
So the rain comes in and it may 

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or may not get all the way down 
to the bottom of the soil where 

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the reactive mineral is still 
there. 

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So it may not ever actually see 
any feldspar if all the feldspar

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has been removed from the soil. 
So in the flatlands, there 

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actually may be very little 
reactive mineral surface area 

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that's interacting with 
corrosive rain. 

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Whereas if you go to a 
mountaintop where there's very 

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little soil buildup, then the 
feldspar, let's say, or whatever

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reactive mineral you're 
interested in is exposed to the 

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rain. 
And so in the former case, the 

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flatland, that's erosive 
transport limited because if the

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erosion rate were just faster 
and the soil was removed, then a

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lot of that reactive mineral 
would be exposed. 

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And then in the mountain, we say
that it's kinetic limited 

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because the erosion is so fast 
in essence that the reactive 

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mineral surface area is right at
the surface interacting with the

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rain. 
So that's one way to simplify 

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these complex natural systems is
to think of these sort of end 

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member situations where you're 
either limited by very, very 

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slow erosion or actually limited
by kinetic weathering. 

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And then did you estimate the 
proportion of the Earth's 

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surface in which each of the 
erosive limited and kinetic 

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limited regimes prevail? 
And I presume you also have to 

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do something about gazettes or 
frozen areas. 

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How do you scale that up? 
When we started applying this 

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paradigm of this kinetic limit 
and erosive transport limit, it 

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allowed us to start to see why 
some of the data in the 

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literature made sense or didn't 
make sense or was comparable 

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across these different scales. 
And then we tried to make the 

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watersheds bigger and bigger and
started to think about the globe

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and at the global scale. 
Then we had to come up with how 

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much is erosive transport 
limited, how much is kinetic 

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limited. 
But as you also mentioned, 

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something like 1/2, the globe 
also has such a small amount of 

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runoff going through the system.
So it's such a small amount of 

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basically rainfall that the 
fluxes are very, very small. 

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So we ended up having to 
estimate how much of the globe 

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was runoff limited. 
It's just not getting enough. 

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Runoff versus kinetic limited 
versus erosive transport 

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limited. 
And then we had to think about 

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how much of the Earth's surface 
is characterized by different 

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rock types. 
So how much is granite, how much

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is basalt, how much is sediment,
and how much is carbonates? 

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Because in general, we're 
interested in the silicate 

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weathering as opposed to the 
carbonate weathering. 

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Wow, it sounds like extremely 
ambitious undertaking to try and

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quantify all those different 
things, but perhaps the data is 

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already out there. 
But broadly speaking, then, what

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does introducing these different
considerations due to the 

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temperature sensitivities you 
measure in the lab? 

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Does it make it more temperature
sensitive, less temperature 

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sensitive, or some of one and 
some of the other? 

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When we went from laboratory 
scale up to watershed scale, and

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I'm talking relatively small 
watersheds now, I'm not talking 

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sort of global watersheds, What 
we saw was that the temperature 

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sensitivity actually increased 
from the laboratory up to 

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watersheds. 
It's not a huge increase, but it

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actually makes some sense 
because just as I've expressed 

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in the lab, we can constrain it 
so that the only thing that's 

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happening is dissolution. 
But when we go up in scale, 

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other processes come in that 
just aren't even present in the 

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lab. 
And so as those other processes 

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come in, they can be also 
temperature sensitive. 

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It actually makes it look like 
the activation energy, which is 

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what we call this temperature 
sensitivity, is higher in a 

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watershed than it is in the 
laboratory. 

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But then when we tried to go up 
to global scale, because so much

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of the earth is dry, when you 
try to get temperature 

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sensitivity for the whole globe,
temperature sensitivity 

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decreases again, mostly because 
of this dry land. 

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The fluxes are just so small and
dry lands that the temperature 

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sensitivity is pretty small. 
In your recent paper, you write 

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that the other processes that 
come into play as you scale up 

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from the lab to the watershed 
include solute transport, clay 

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precipitation, biotic activity, 
disaggregation, fracturing, and 

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erosion. 
And that these processes in turn

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can be influenced by climate 
factors such as temperature run 

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off and precipitation, and by 
weatherability factors such as 

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lithology, porosity, 
permeability, type of 

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vegetation, and position within 
a landscape. 

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That's a lot of processes to 
consider. 

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You characterize these processes
using a standard formula for the

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temperature dependence of 
reaction rates called the 

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Arrhenius equation, in which the
temperature sensitivity is 

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represented by an activation 
energy for each process or set 

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of processes. 
But in any particular setting, 

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isn't just one of the processes 
likely to be the overall rate 

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determining step? 
Is that what determines the 

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activation energy? 
The activation energy does 

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characterize something about the
rate limiting step. 

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But if you have a complex 
process that doesn't really even

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have a rate limiting step, it 
can have so many processes that 

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are all confounded to it, it can
be very hard to interpret what 

231
00:13:21,320 --> 00:13:23,320
that activation energy actually 
means. 

232
00:13:23,920 --> 00:13:28,360
Broadly speaking, then, you try 
and parameterize all those many,

233
00:13:28,360 --> 00:13:32,760
many different effects in terms 
of a single activation energy 

234
00:13:32,760 --> 00:13:35,360
that you then plug into the 
equation that is meant to 

235
00:13:35,360 --> 00:13:38,280
indicate the blended temperature
sensitivity. 

236
00:13:38,800 --> 00:13:41,520
That's right. 
And in a way it's like treating 

237
00:13:41,520 --> 00:13:44,640
each of these larger spatial 
scale systems the way a chemist 

238
00:13:44,640 --> 00:13:47,680
would treat it, without being 
able to isolate every single 

239
00:13:47,680 --> 00:13:49,560
process and measuring them all 
separately. 

240
00:13:50,080 --> 00:13:54,120
In the early days, people 
measured very complex processes 

241
00:13:54,440 --> 00:13:57,640
and then over time we simplified
them more and more and try to be

242
00:13:57,640 --> 00:14:00,440
very reductionist. 
And now what we're trying to do 

243
00:14:00,440 --> 00:14:03,160
is put it all back together 
again and try to understand 

244
00:14:03,160 --> 00:14:05,600
these really big, complex 
systems again as I. 

245
00:14:05,600 --> 00:14:09,320
Mentioned in the introduction, 
there have been enormous changes

246
00:14:09,320 --> 00:14:12,720
in the Earth's surface over 
geological time, such as the 

247
00:14:12,720 --> 00:14:16,000
growth of continental crusts and
the formation and destruction of

248
00:14:16,000 --> 00:14:19,520
supercontinents and the rise and
fall of mountain chains. 

249
00:14:20,080 --> 00:14:23,120
Would these changes be expected 
to affect the temperature 

250
00:14:23,120 --> 00:14:26,600
sensitivity of the thermostat, 
and if so, in what way? 

251
00:14:27,160 --> 00:14:29,560
In the points of Earth's 
history, when there were really 

252
00:14:29,560 --> 00:14:34,400
large supercontinents, very 
large fractions of the continent

253
00:14:34,720 --> 00:14:37,360
may have been very dry. 
Because as the rain comes in 

254
00:14:37,360 --> 00:14:40,720
from the oceans and gets rained 
out, you end up having big 

255
00:14:40,720 --> 00:14:42,400
deserts in the middle of big 
continents. 

256
00:14:42,400 --> 00:14:44,520
And you can see that even on 
today's Earth. 

257
00:14:45,200 --> 00:14:48,360
To do an analysis like the one I
did, one would have to think 

258
00:14:48,400 --> 00:14:52,480
about what would we expect the 
dry land fraction would be when 

259
00:14:52,480 --> 00:14:55,840
there are big supercontinents. 
And then you mentioned big 

260
00:14:55,840 --> 00:14:58,440
mountain building events. 
There have been times like 

261
00:14:58,640 --> 00:15:02,160
uplift of the Hamayas where you 
know mountains were going up 

262
00:15:02,160 --> 00:15:06,040
very, very fast, exposing a lot 
of mineral to weathering. 

263
00:15:06,480 --> 00:15:10,200
And there's been an ongoing 
argument for quite a while about

264
00:15:10,600 --> 00:15:13,080
how the mountain building 
effects weathering. 

265
00:15:13,320 --> 00:15:17,040
From one point of view, one 
might argue that more reactive 

266
00:15:17,040 --> 00:15:21,560
minerals should cause higher 
rates of weathering, and so it 

267
00:15:21,560 --> 00:15:24,600
could affect the temperature 
sensitivity of the planet if 

268
00:15:24,600 --> 00:15:26,920
more of the planet was kinetic 
limited. 

269
00:15:27,800 --> 00:15:33,680
So would it be fair to say that 
during the prevalence of 

270
00:15:33,680 --> 00:15:36,840
supercontinent, say every 500 
million years in the Wilson 

271
00:15:36,840 --> 00:15:41,960
cycle, that you get a period 
when the drawdown is less 

272
00:15:41,960 --> 00:15:44,840
effective because you have all 
these dry interiors and so that 

273
00:15:45,600 --> 00:15:49,600
the carbon dioxide might build 
up in the atmosphere and you get

274
00:15:49,600 --> 00:15:52,880
a little bit warmer. 
And conversely when you have a 

275
00:15:52,880 --> 00:15:57,200
lot of mountain chains forming 
that the weathering is more 

276
00:15:57,200 --> 00:16:00,280
efficient and so you get a draw 
down of the carbon dioxide and 

277
00:16:00,280 --> 00:16:02,240
it cools off. 
Is that something people have 

278
00:16:02,240 --> 00:16:05,360
looked to see? 
I think what you said is our 

279
00:16:05,360 --> 00:16:08,680
baseline set of hypothesis. 
And of course when they dig into

280
00:16:08,680 --> 00:16:11,160
that, there's a lot of other 
variables. 

281
00:16:11,160 --> 00:16:14,640
So where is this supercontinent?
Is it high latitude, low 

282
00:16:14,640 --> 00:16:17,200
latitude, Northern hemisphere? 
It depends. 

283
00:16:17,640 --> 00:16:21,640
And in terms of mountain 
building events and higher rates

284
00:16:21,640 --> 00:16:26,760
of drawdown, higher temperature 
sensitivities, again, it depends

285
00:16:26,880 --> 00:16:29,640
what's the rock type. 
It depends where the mountain 

286
00:16:29,640 --> 00:16:32,000
building's occurring. 
And then there's this other 

287
00:16:32,000 --> 00:16:35,800
wrinkle that we haven't really 
talked about and that is that 

288
00:16:35,920 --> 00:16:39,840
there's not that much CO2 in the
atmosphere and yet the CO2 in 

289
00:16:39,840 --> 00:16:43,800
the atmosphere has been 
maintained at relative constancy

290
00:16:43,800 --> 00:16:46,800
over periods of time. 
So all these processes have to 

291
00:16:46,800 --> 00:16:49,960
be balanced. 
So even if a mountain chain goes

292
00:16:49,960 --> 00:16:53,200
up and let's say there's a 
increased temperature 

293
00:16:53,200 --> 00:16:56,800
sensitivity because there's more
kinetic limited landscape, if 

294
00:16:56,800 --> 00:17:00,840
that were to pull too much CO2 
out of the atmosphere, the globe

295
00:17:00,840 --> 00:17:02,680
could quickly become ice 
covered. 

296
00:17:02,720 --> 00:17:05,680
And we don't always see that. 
So, well, what happens when a 

297
00:17:05,680 --> 00:17:08,680
mountain chain goes up and it 
causes this higher temperature 

298
00:17:08,680 --> 00:17:12,359
sensitivity? 
Is it perhaps modulated by other

299
00:17:12,359 --> 00:17:14,160
processes? 
And one of the big arguments out

300
00:17:14,160 --> 00:17:16,960
there right now is, you know, 
you can't just think of the 

301
00:17:16,960 --> 00:17:20,920
world as being silicate rock. 
There's also a lot of pyrite out

302
00:17:20,920 --> 00:17:23,560
there. 
Pyrite is iron sulfide, and when

303
00:17:23,560 --> 00:17:26,560
pyrite weathers, it produces 
sulfuric acid. 

304
00:17:26,920 --> 00:17:31,200
And weathering driven by pyrite 
also happens as mountains go up.

305
00:17:31,520 --> 00:17:34,920
And so there's other 
complexities that may actually 

306
00:17:34,920 --> 00:17:39,080
cause not only CO2 drawdown, but
actually caused some CO2 release

307
00:17:39,080 --> 00:17:42,080
during mountain building events.
What's about the effect on 

308
00:17:42,080 --> 00:17:45,680
weathering of life forms, both 
microscopic and macroscopic? 

309
00:17:46,480 --> 00:17:49,960
We've done some experiments 
where we've put in bacteria and 

310
00:17:50,400 --> 00:17:52,720
into our flask experiments with 
minerals. 

311
00:17:52,720 --> 00:17:55,240
We've done some column 
experiments with plants. 

312
00:17:55,640 --> 00:17:59,960
And in general, what you see at 
the lab scale sort of at that 

313
00:17:59,960 --> 00:18:03,560
small scale is there's usually 
an acceleration of weathering. 

314
00:18:03,920 --> 00:18:07,440
But when you go up in scale, if 
you think about your backyard, 

315
00:18:07,440 --> 00:18:10,880
if you have any kind of a slope 
in your backyard, you're often 

316
00:18:10,880 --> 00:18:13,760
advised to put plants on that 
slope because it'll hold the 

317
00:18:13,760 --> 00:18:17,680
soil in place and can move your 
system from something that could

318
00:18:17,680 --> 00:18:22,760
be kinetic limited to a system 
that is covered with soil that 

319
00:18:22,760 --> 00:18:24,440
has very little reactive mineral
in it. 

320
00:18:24,440 --> 00:18:26,200
So it could be more erosive 
transport limited. 

321
00:18:26,680 --> 00:18:30,760
So really, with the lab scale, 
biology tends to accelerate 

322
00:18:30,760 --> 00:18:33,680
weathering, but as you go up in 
scale, it can have both effects.

323
00:18:33,680 --> 00:18:35,880
It can accelerate weathering, 
but it can also slow down 

324
00:18:35,880 --> 00:18:40,560
weathering, and the jury's out 
as to how that has played out at

325
00:18:40,560 --> 00:18:43,280
higher and higher spatial scales
of analysis. 

326
00:18:43,760 --> 00:18:49,000
Why is it so important to know 
the overall temperature 

327
00:18:49,000 --> 00:18:52,680
sensitivity of the Earth's 
geological thermostat? 

328
00:18:53,320 --> 00:18:57,560
Broadly speaking, I suppose the 
higher the sensitivity, the 

329
00:18:57,560 --> 00:19:02,040
quicker any temperature 
excursion can be damped over 

330
00:19:02,040 --> 00:19:05,000
geological time and brought back
to its steady state value. 

331
00:19:05,520 --> 00:19:09,720
Is that something that we need 
to know both to understand 

332
00:19:09,920 --> 00:19:13,400
geological history, but also to 
understand what's happening 

333
00:19:13,400 --> 00:19:14,840
today? 
Sure. 

334
00:19:14,840 --> 00:19:20,320
Well, what we're doing today is 
totally changing this cycle that

335
00:19:20,320 --> 00:19:23,360
we're talking about. 
South geologists think about the

336
00:19:23,360 --> 00:19:27,960
CO2 in the atmosphere and the 
global temperature as being 

337
00:19:27,960 --> 00:19:32,800
modulated by how fast volcanoes 
release CO2 and how fast 

338
00:19:32,800 --> 00:19:35,320
weathering pulls the CO2 back 
out of the atmosphere. 

339
00:19:35,760 --> 00:19:37,560
But that's over a million year 
time scales. 

340
00:19:37,560 --> 00:19:39,360
That's a very long, slow 
process. 

341
00:19:39,600 --> 00:19:44,280
If the Earth is just left on its
own to respond, CO2 will be 

342
00:19:44,280 --> 00:19:47,000
drawn down out of the atmosphere
by weathering. 

343
00:19:47,360 --> 00:19:49,560
But it could take hundreds of 
thousands of years. 

344
00:19:49,960 --> 00:19:54,840
And right now we're in this big 
dialogue around the world about 

345
00:19:54,840 --> 00:19:58,240
how are we going to stop using 
fossil fuels. 

346
00:19:58,440 --> 00:20:01,840
But what's important is that 
there's still so much CO2 out 

347
00:20:01,840 --> 00:20:04,560
there in the atmosphere, and 
that's going to be still acting 

348
00:20:04,560 --> 00:20:06,720
like a thermostat. 
The greenhouse effect is going 

349
00:20:06,720 --> 00:20:10,280
to maintain the warming that 
we're observing, and it's going 

350
00:20:10,280 --> 00:20:12,200
to be a very long time to pull 
that out. 

351
00:20:12,200 --> 00:20:15,440
And so this basic understanding 
of the Earth system has spurred 

352
00:20:15,440 --> 00:20:19,760
a conversation about. 
Well, what can we do to pull the

353
00:20:19,760 --> 00:20:21,920
CO2 out of the atmosphere? 
Because the Earth is not going 

354
00:20:21,920 --> 00:20:26,360
to do it fast enough for us. 
There are silicate rocks on the 

355
00:20:26,360 --> 00:20:29,800
surface of Venus. 
Why have they not been able to 

356
00:20:29,800 --> 00:20:32,960
provide thermostatic temperature
control there? 

357
00:20:33,320 --> 00:20:38,440
Venus is closer to the Sun. 
It's rotation is slower, so part

358
00:20:38,440 --> 00:20:42,720
of it is facing the sun for 
longer periods of time, and the 

359
00:20:42,720 --> 00:20:46,040
temperature at the surface of 
the planet has been such that it

360
00:20:46,040 --> 00:20:49,200
has lost most of its water, if 
not all of its water. 

361
00:20:49,520 --> 00:20:52,160
And so the atmosphere is 
basically a CO2 atmosphere. 

362
00:20:52,160 --> 00:20:55,520
So there may be rock and there 
may be CO2, but there isn't the 

363
00:20:55,520 --> 00:20:58,280
water there to allow the 
weathering to proceed and pull 

364
00:20:58,280 --> 00:21:01,640
that CO2 out. 
And I guess on Mars the 

365
00:21:01,640 --> 00:21:04,720
situation is there's just not 
much of an atmosphere at all. 

366
00:21:04,800 --> 00:21:06,800
Right. 
There has been weathering on 

367
00:21:06,800 --> 00:21:09,880
Mars, our Rovers that we've put 
up on the planet and looked at 

368
00:21:09,880 --> 00:21:12,840
the geology. 
There's been beautiful evidence 

369
00:21:12,840 --> 00:21:17,040
that there have been times on 
Mars earlier in Mars's history 

370
00:21:17,040 --> 00:21:20,080
when there actually was very 
deep weathering that occurred, 

371
00:21:20,080 --> 00:21:25,080
and now it's not occurring. 
Coming back to the question of 

372
00:21:25,120 --> 00:21:29,600
global warming that we're facing
here on Earth, and your point 

373
00:21:29,600 --> 00:21:32,920
that the time scale for this 
geological drawdown is extremely

374
00:21:32,920 --> 00:21:40,000
long, does your work help inform
the attempts to sequester carbon

375
00:21:40,000 --> 00:21:45,840
dioxide by the use of enhanced 
weathering, which is one of the 

376
00:21:46,200 --> 00:21:48,400
many techniques that are being 
proposed now? 

377
00:21:48,760 --> 00:21:52,800
One way to do this is to dig up 
a bunch of rock, grind it up, 

378
00:21:53,000 --> 00:21:55,320
and then put it out on fields 
and let it weather. 

379
00:21:55,680 --> 00:21:58,560
And that's such a simple thing 
to imagine. 

380
00:21:58,560 --> 00:22:01,960
We know how to dig up rock, We 
know how to transport it, we 

381
00:22:01,960 --> 00:22:05,080
know how to grind it. 
We know how to disseminated on 

382
00:22:05,080 --> 00:22:06,720
fields. 
We do that all the time with 

383
00:22:06,720 --> 00:22:09,840
lime. 
So many farmers fields are lime,

384
00:22:09,880 --> 00:22:13,080
so they take limestone and grind
it up and put it just really 

385
00:22:13,080 --> 00:22:16,040
common. 
And so people have said why 

386
00:22:16,040 --> 00:22:19,920
don't we dig up, especially 
basalt, which is a rock type 

387
00:22:19,920 --> 00:22:21,960
that has a lot of calcium and 
magnesium. 

388
00:22:22,240 --> 00:22:26,320
It's actually a very good set of
minerals to pull CO2 out of the 

389
00:22:26,320 --> 00:22:28,480
atmosphere. 
Why don't we dig up a lot of 

390
00:22:28,480 --> 00:22:32,720
basalt, grind it up, transport 
it to farmers fields, put it out

391
00:22:33,120 --> 00:22:35,520
and let it pull the CO2 out of 
the atmosphere? 

392
00:22:35,880 --> 00:22:39,040
And people are doing this. 
People are trying this in the 

393
00:22:39,040 --> 00:22:42,880
Midwest, people are trying it in
small plots around the world. 

394
00:22:43,240 --> 00:22:48,160
And people are trying to measure
then whether CO2 that's pulled 

395
00:22:48,160 --> 00:22:50,520
out is what they might have 
predicted. 

396
00:22:50,840 --> 00:22:54,640
And then they have to compare 
the CO2 that's pulled out to the

397
00:22:54,640 --> 00:22:59,680
total calculated CO2 of digging 
up the rock, grinding the rock, 

398
00:22:59,680 --> 00:23:02,120
transporting the rock, and then 
spreading the rocks. 

399
00:23:02,120 --> 00:23:04,880
So there's like all those 
processes in there that you have

400
00:23:04,880 --> 00:23:09,000
to figure out how much CO2 was 
released by the hydrocarbons 

401
00:23:09,000 --> 00:23:11,440
that you used to do all those 
kinds of processes as well. 

402
00:23:12,040 --> 00:23:15,800
This could be successful. 
You could run this system in the

403
00:23:15,800 --> 00:23:19,040
way that you'd pull more CO2 out
than you'd put in, in terms of 

404
00:23:19,040 --> 00:23:22,160
the digging, grinding, 
transporting and spreading. 

405
00:23:22,520 --> 00:23:25,760
I discussed enhanced weathering 
in an earlier episode with Phil 

406
00:23:25,760 --> 00:23:29,800
Renforth and learn that to 
remove gigatons of carbon 

407
00:23:29,800 --> 00:23:33,240
dioxide from the atmosphere per 
year, which is what we need to 

408
00:23:33,240 --> 00:23:36,040
do in order to have a 
significant impact, we would 

409
00:23:36,040 --> 00:23:38,840
have to do this on a truly 
gigantic scale. 

410
00:23:39,160 --> 00:23:41,640
Right. 
Really large percentages of the 

411
00:23:41,640 --> 00:23:46,400
farmland in the top agricultural
countries in the world would 

412
00:23:46,400 --> 00:23:51,200
have to be used to make a dent 
in the amount of CO2 that we put

413
00:23:51,200 --> 00:23:54,960
in the atmosphere. 
We may say, well this is too 

414
00:23:54,960 --> 00:23:58,320
much rock to be dug up and 
transported and powdered and 

415
00:23:58,320 --> 00:24:00,560
spread to solve the whole 
problem. 

416
00:24:00,800 --> 00:24:05,440
But in certain areas, possibly 
near big basalt deposits, it 

417
00:24:05,440 --> 00:24:09,200
might be a really good process, 
especially because the ground up

418
00:24:09,200 --> 00:24:13,840
powder has nutrients in it. 
As you mentioned, you clearly 

419
00:24:13,840 --> 00:24:17,560
had to make a lot of simplifying
assumptions in order to build a 

420
00:24:17,560 --> 00:24:20,680
model for how weathering depends
on temperature on a global 

421
00:24:20,680 --> 00:24:23,120
scale. 
Are there any aspects in 

422
00:24:23,120 --> 00:24:26,400
particular that you'd like to 
add to your model to make it 

423
00:24:26,400 --> 00:24:29,120
more realistic? 
One of the puzzles is the effect

424
00:24:29,120 --> 00:24:33,000
of biota. 
So plants and organisms and how 

425
00:24:33,000 --> 00:24:35,840
that affects weathering. 
I mentioned that the laboratory 

426
00:24:35,840 --> 00:24:39,320
scale, it seems to accelerate, 
but then as you get up to field 

427
00:24:39,320 --> 00:24:42,720
scales, you often see that biota
can decelerate weathering. 

428
00:24:42,720 --> 00:24:47,080
So I did work on that to some 
extent in order to do this first

429
00:24:47,240 --> 00:24:50,400
estimate that we did as a global
scale temperature sensitivity. 

430
00:24:50,400 --> 00:24:53,000
But I'd like to work on that 
more and think more about again,

431
00:24:53,000 --> 00:24:56,000
scaling up biota. 
There's a lot of papers and all 

432
00:24:56,000 --> 00:24:58,720
these different spatial scales. 
I'd like to see if I could do 

433
00:24:58,720 --> 00:25:02,040
something similar and make sense
out of why the different 

434
00:25:02,320 --> 00:25:04,920
observations at different 
spatial scales don't always seem

435
00:25:04,920 --> 00:25:07,480
to make sense. 
What are you working on at the 

436
00:25:07,480 --> 00:25:09,520
moment? 
One thing that I'm very 

437
00:25:09,520 --> 00:25:13,840
intrigued by is this idea that 
soil can become depleted in 

438
00:25:13,840 --> 00:25:16,520
minerals because of weathering. 
If you think of weathering as 

439
00:25:16,520 --> 00:25:20,400
being top down, the rain comes 
from the atmosphere and moves 

440
00:25:20,400 --> 00:25:22,800
down. 
Like A1 dimensional worldview 

441
00:25:23,200 --> 00:25:26,400
that upper soil becomes depleted
in their reactive minerals. 

442
00:25:26,720 --> 00:25:30,440
Eventually, as you dig down, you
come to a zone where there are 

443
00:25:30,440 --> 00:25:34,800
reactive minerals and they are 
reacting sometimes at very, very

444
00:25:34,800 --> 00:25:38,040
slow rates if they're very deep.
But that zone where they're 

445
00:25:38,040 --> 00:25:41,040
reacting, I call that a reaction
front or the weathering front 

446
00:25:41,680 --> 00:25:45,480
and weathering front should be 
all around us in the landscape 

447
00:25:45,480 --> 00:25:47,880
beneath our feet. 
So we can see the landscape that

448
00:25:47,880 --> 00:25:51,240
we walk on and we can see the 
morphology of that landscape. 

449
00:25:51,240 --> 00:25:54,080
That's a geomorphologist study, 
is why the shape of the 

450
00:25:54,080 --> 00:25:57,640
landscape looks the way it does.
What we don't know is what does 

451
00:25:57,640 --> 00:26:00,800
the landscape of that reaction 
front look like in the 

452
00:26:00,800 --> 00:26:03,960
subsurface? 
So for each mineral in a rock, 

453
00:26:04,160 --> 00:26:06,920
there will be a landscape, there
will be a depth at which that 

454
00:26:06,920 --> 00:26:12,560
mineral is dissolving, and how 
does that landscape for each 

455
00:26:12,560 --> 00:26:17,280
mineral vary as you move across 
the landscape that we can walk 

456
00:26:17,280 --> 00:26:19,360
on. 
So for example, at a Ridge top, 

457
00:26:19,440 --> 00:26:23,520
you may only have to go very 
shallow before you start to see 

458
00:26:23,520 --> 00:26:27,880
a reaction front versus if you 
go down to a stream, you might 

459
00:26:27,880 --> 00:26:30,320
have a different depth down to 
the reaction front. 

460
00:26:30,880 --> 00:26:34,160
And realistically, geochemists 
have never been able to study 

461
00:26:34,160 --> 00:26:37,640
those landscapes because that 
three dimensionality of it is 

462
00:26:37,640 --> 00:26:40,320
very difficult. 
And so recently I've worked with

463
00:26:40,320 --> 00:26:44,000
geophysicists who have all these
tools that can look at 

464
00:26:44,000 --> 00:26:47,880
landscapes in the subsurface and
start to measure geophysical 

465
00:26:47,880 --> 00:26:50,960
properties in the subsurface. 
So if we could understand 

466
00:26:50,960 --> 00:26:53,840
distributions of these 
geochemical landscapes of 

467
00:26:53,840 --> 00:26:57,160
reaction in the subsurface and 
relate that to the geophysical 

468
00:26:57,160 --> 00:27:00,720
signals, we could map what the 
subsurface looks like and where 

469
00:27:00,720 --> 00:27:03,680
weathering is happening. 
And I think that in itself would

470
00:27:03,680 --> 00:27:07,320
help us understand this puzzle 
of global weathering as well, 

471
00:27:07,600 --> 00:27:10,920
namely how it's distributed 
across our landscapes. 

472
00:27:12,080 --> 00:27:13,960
Susan Bradley, thank you very 
much. 

473
00:27:14,280 --> 00:27:16,080
Thank you. 
It was a pleasure to talk to 

474
00:27:16,080 --> 00:27:18,160
you. 
To see pictures and 

475
00:27:18,160 --> 00:27:23,600
illustrations that support this 
podcast, go to geologybytes.com,

476
00:27:24,120 --> 00:27:27,440
where you'll also find 
transcripts and a subject matter

477
00:27:27,440 --> 00:27:31,400
index of all the episodes there.
You can also give me feedback, 

478
00:27:31,400 --> 00:27:35,160
which I welcome, as well as sign
up to get my emails about new 

479
00:27:35,160 --> 00:27:35,920
episodes.
