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Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

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Part II: Building a Goldilocks World om the Big Bang to Habitable Plane
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Page 1: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Part II: Building a Goldilocks WorldPart II: Building a Goldilocks World

From the Big Bang to Habitable PlanetsFrom the Big Bang to Habitable Planets

Page 2: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Outline:

Formation of the planets

Distribution (and redistribution) of volatiles

Heat production and transport

Radiation budget

The traditional habitable zoneBased on the approach in Jim Kasting’s “How to Find a

Habitable Planet”

Page 3: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Planet Formation

Page 4: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.
Page 5: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Chambers, 2001

Modeling Accretion

Page 6: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Condensation of Volatiles in the Circumstellar Disk

Page 7: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Jupiter Uranus

Distance from Sun (AU)

Saturn

Tem

pera

ture

(K

)Earth

20

2000

1000

151050

Silicates

Metals

Water Ice

Ammonia Ice

Condensation of Volatiles in the Circumstellar Disk

Page 8: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

But not so much the presence of Earth’s oceans . . .

This model does a good job of explaining the distribution of rocky, gas giant, and ice

giant planets

Page 9: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Volatiles are redistributed from the outer to the inner solar system by asteroids and comets (which, recall,

carry more than just volatiles . . . )

Page 10: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Heat

Page 11: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Accretion and Impacts Deliver Energy(much of which becomes heat)

Page 12: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

So does radioactive decay . . .

238U → 234Th + α(this is nuclear fission (= energy – remember?))

Page 13: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Consequences of Interior HeatingI. Differentiation

Page 14: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

II. Liquid Core = Earth’s Dynamo (Magnetic Field)

Page 15: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

III. Volcanism and Plate Tectonics(important for many reasons – we’ll discuss one now, one later)

Page 16: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Volcanic activity connects the terminals

=

A chemically and thermally differentiated planet is like a

battery . . .

Page 17: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Chemical Energy for LifeChemical Energy for Life

Page 18: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Bigger bodies (= higher SA/Vol) cool more slowly, and may have more active or longer lasting volcanism as a result

Page 19: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Nope.

Only about 0.025% of

surface heating comes from

geothermal heat flux.

The rest comes from…

Is this geological heating what

keeps the surface of our planet

warm (and our water in liquid

form)?

Page 20: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Solar Solar RadiatioRadiation Budgetn Budget

Solar Solar RadiatioRadiation Budgetn Budget

Page 21: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

(mostly visible)

(mostly infrared)

(NASA Earth Observatory)

Radiation intercepted by planet goes as 1/d2

d

Radiation Budget

Absorbed (Visible) Energy =Radiated (Infrared) Energy

Page 22: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

TooHot

TooCold

JustRight

Got Liquid Surface Water?(simple view)

Page 23: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.
Page 24: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.
Page 25: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Negative Feedback on Greenhouse Warming

The Carbonate Silicate Cycle

(courtesy Jim Kasting)

Constant source while volcanism is active

Enhanced by higher temperature, more CO2

Puts CO2 back into circulation

Enhanced by biology.

Would still happen without, but with higher CO2 levels

Ocean-atmosphere exchange required to

make this happen

Page 26: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Cautionary Tales for Worlds Aspiring to Habitability

Page 27: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Venus and the Runaway Greenhouse

Page 28: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Mars: The Case of the Missing Greenhouse

Effect

Page 29: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

http://www.dlr.de/en/desktopdefault.aspx/tabid-5170/8702_read-15322/8702_page-2/

The Traditional (Liquid Water) Habitable Zone

Page 30: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Extras

Page 31: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.
Page 32: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

year

century

million yr.

billion yr.

ten thousand yr.

100 millionmillion10,00010010.01

Hiroshima

Tunguska

K/T

TNT equivalent yield (MT)

Global catastrophe

Tsunami danger

(Credit: D. Morrison)

Terrestrial ImpactFrequency

“Armageddon” Impact(Texas-sized!)

“Catastrophic” depends on who you are and where you live . . .

“Catastrophic” depends on who you are and where you live . . .

Page 33: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Temperature (°C)

Dep

th (

km)

2

0

200

1

1000

Geotherm

al Gradient

Surface-Sterilizing Impacts

(Sleep & Zahnle, 1998)

Habitable

Heat-Sterilized

Impact Heating

Page 34: Part II: Building a Goldilocks World From the Big Bang to Habitable Planets.

Effects of Impacts on

Established Life:

Interplanetary Transfer of Life?


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