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Planetary Complexity

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Analysing Complexity

Macquarie University

4.7 (49 ratings) | 5.4K Students Enrolled

Course 1 of 4 in the Solving Complex Problems Specialization

The first course of the specialization ANALYZING COMPLEXITY will teach you what unifying patterns lie at the core of all complex problems. It advances your knowledge of your own field by teaching you to look at it in new ways. ANALYZING COMPLEXITY is constructed in the following way: Week I. "What is Complexity?" - What is at the core of all complex problems Week II. "Complex Physical Systems" - What complex problems all have in common in the inanimate world Week III. "Complex Adaptive Systems" - What complex problems all have in common in nature Week IV. "Complex Cultural Systems" - What complex problems all have in common in human society Week V. "Complexity, Fragility, and Breakdown" - Why complex problems arise Week VI. "Complexity in the Anthropocene" - What complex problems face us today

Reviews

4.7 (49 ratings)

5 stars
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TA

Oct 24, 2017

You should study Complexity from this course if you are interesting in complex system.

TW

Apr 23, 2017

Super interesting course, I have never seen in my lifetime.\n\nWatch me ;))

From the lesson

Complex Physical Systems

In this module, we'll look at how complexity operates in the inanimate universe, the corresponding links between physics, chemistry, and geology and how they reflect the ground rules of all forms of complexity.

Planetary Complexity6:49

Taught By

David Baker
Associate Lecturer
David Christian
Professor
Shawn Ross
Associate Professor

Transcript

The big question for

this segment is, do planetary systems represent a new level of complexity?

And how complex are planetary systems?

[MUSIC]

Planetary systems are interesting in that they may harbor life.

To do so, though, they need a long-lived stable orbit in the habitable zone

around a star where liquid water is stable.

And they need that liquid water to be stable for a long time.

Earth has achieved this remarkable stability through a number of feedback

mechanisms.

The emergence of a stable solar system from the protoplanetary

disc involved a gravitational ballet between these embryonic planets.

Some were ejected from the solar system, some collided, and

some of those that collided actually stuck.

Eventually, a system emerged where the remaining planets exerted gravitational

tugs on each other that balanced out, a gravitational feedback system.

And that has been stable for about 4.5 billion years.

Earth is remarkable in that it has maintained liquid water on its surface for

over 4.4 billion years.

And this is the result of a number of feedbacks between the surface and

the planetary interior.

Earth has several times frozen over.

Over 600 million years ago, lower levels of volcanic gas input resulted in

a weak greenhouse effect causing the ice sheets to grow.

Ice is reflective, resulting in the Earth reflecting more light back into space,

which lowered the temperatures further.

This caused the ice sheets to grow more.

And a runaway ice house was the result.

This global ice age was thwarted by another feedback.

With the world covered by ice, there was limited photosynthesis and

no weathering of continents.

Both these processes normally suck CO2 out of the atmosphere, and

without them, carbon dioxide had nowhere to go.

Since volcanoes were still pumping out these gases,

though, like CO2, the greenhouse gas levels in the atmosphere started to rise,

eventually leading to melting of the ice sheets.

Melting ice made the Earth less reflective and so

the planet absorbed more heat which melted more ice.

Until eventually the ice sheets disappeared, and

animals appeared in the Cambrian explosion shortly afterwards.

The most common type of planetary system observed in the galaxy

are hot Jupiter systems.

Gas giants in extremely close orbits to their stars.

These systems are largely hostile to complex life and

formed due to the migration of planets inwards early in their history.

The solar system possesses evidence of this process in the asteroid belt,

which Jupiter crossed at one point in a march towards Earth.

This catastrophe was averted for

us by an initial condition, the formation of Saturn.

Saturn was big enough to influence Jupiter gravitationally and entered into

a residence orbit, where the gravitational feedback between the two orbiting bodies

creates a stable configuration, putting the brakes on Jupiter's inward migration.

A further feedback between these bodies, and the gas in the disc,

resulted in them migrating back out to the outer solar system,

leaving behind the shattered remnants of the asteroid belt.

A failed world, but also in a stable inner solar system.

Plate tectonics is remarkably important for

long lived habitable planets,acting as a planetary thermostat.

It's responsible for most of the volcanoes and thus most of the CO2 and

water vapor delivered to the atmosphere from the planet's interior.

However, plate tectonics also creates mountains which erode,

absorbing CO2 into minerals as they do so.

This sediment is then recycled by plates back into the Earth's interior,

at places like subduction zones.

Why Earth has plate tectonics,

when no other planet in the solar system does, is still not clear.

The plates themselves are just the surface of a convection

system spanning the depth of the mantle.

This system is very sensitive to temperature.

If the mantle heats up too much, it becomes less viscous and

moves faster rapidly dumping heat from the interior.

If it cools too much, the mantle becomes sluggish and cools inefficiently.

This gives time for radioactive heating, the main power source for

the Earth, to warm the mantle.

These feedbacks operate to keep mantle temperature sensible and

the plates moving at regular speeds.

Simulations of plate tectonics show this nonlinear system is very dependent

on its initial conditions.

And a system may evolve in very different paths depending on how it started,

a characteristic of chaotic systems.

This history dependence is known as hysteresis, and

may be an important factor in why such similar planets as Earth and Venus,

have such very different tectonic states today.

Ultimately, Earth's long-lived habitability is due

to its ability to sequester CO2 out of the atmosphere and store it in the rocks.

Today, it is light that primarily accomplishes this task.

Both by photosynthesis, but also critically by marine organisms taking

carbonate, the dissolved form of CO2, and making shells.

From coral reefs to oceanic ooze and

chalk, the bodies of dead organisms constitute an enormous sink of CO2.

As a result, the biosphere can be considered a nested system,

an additional complex system working in coordination with the planet and

affecting its geology and moderating the system to sustain itself.

If all of those carbonates, now stored in rocks, were converted to CO2,

Earth's atmosphere would look a lot like Venus.

Venus is currently a searing hellhole.

Over 400 degrees Celsius on the surface, and over 90 times atmospheric pressure.

With clouds of sulfuric acid, its surface is hostile to all known life.

Yet, there is evidence on Venus that it once had liquid water.

The difference may have been that Venus did not have plate tectonics or,

as far as we know, did not have life.

As a result, it lacked the ability to suck CO2 out of its atmosphere and

put it in those surface rocks.

The CO2 levels rose, evaporating the oceans.

Water is an even more potent greenhouse gas than CO2, and

as a result temperatures on Venus skyrocketed further.

The end result is a runaway greenhouse effect,

the result of a positive feedback between the climate and volcanic degassing.

This is an example of a cascading failure, where a failure in one component for

life or tectonics resulted in a catastrophe for the entire system.

[MUSIC]

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