Chapter 9 Planetary Geology

 

The Terrestrial Objects

         Mercury  Venus  Earth  Moon  Mars

 

The Physics of the Interior

         Pressure, temperature, density

         Layers

Differentiation into:

core, mantle, crust

         asthenosphere, lithosphere

         the importance of the lithosphere

 

The Five Objects

 

How do we know what the interior looks like?

Average density

Shape

Gravity measures

Magnetic field

Surface features and chemistry

Seismic primary and secondary waves

 

The Heating and Cooling of Interiors

 

Energy sources

Accretion and contraction  (most important at first)

Differentiation

Radioactive heating (most important for terrestrials now)

Tidal heating (not important for us)

 

Heat transfer and loss

Convection

Conduction

Radiation

 

How fast does a planet cool?

         Any new energy sources?

Surface to volume ratio

The difference between cooling slowly and cooling fast.

 

Planetary Magnetic fields

         Two ways to create a magnetic field  easy   hard

 

So, why does Earth and Mercury have magnetic field and Mars, Venus and the moon do not?

Electrically conducting fluid, convection and rotation

 

How are terrestrial surfaces modified?

 

 

Impact cratering

Crater  depends on energy but is about 10x size of impactor

Ejecta

Largest are called impact basins  lunar maria  more on the earthside

Sometimes they get really small

Different types

Bowl

Flat

Filled

 

They show what they hit.   Rock  ice and rock   ice

 

Impacts ‘garden’ the soil  e.g. lunar regolith

 

 

Vulcanism

Shield volcanoes

stratovolcanoes

domes, rilles

Magma flows  Basalt

   depends on the lava

         outgassing (atmosphere production)

 

 

Tectonics

Mountains

Rifts

Plates  earth  heat transfer and plates

 

Erosion

Wind dunes

Water gullies, deltas

 

 

What matters?

         Size

         Distance from the Sun (temperature)

         Rotation

 

 

THE TOUR

 

Moon

 

The Surface

Highlands and maria

Volcanic flows

Craters

Breccia and regolith

 

What would it be like to live on the moon?

 

 

Mercury

 

Somewhat like the moon.

        Intercrater plains smoother plus scarps

         But scarps show global shrinkage

 

 

Mars movie

 

Topography

Shield volcanoes  Tharsis

Valles Marineris

Volcanic plains

 

The Surface

 

water  and more water but is it recent?

solid evidence layering  dried mud

Distribution

Did it produce life?

 

The Atmosphere

         Thin, cold and mostly CO2

 

Venus

         map

The Atmosphere

         Thick, hot and mostly CO2

 

Topography

Shield volcanoes   pancake domes  coronae

 

The Surface

 

 

Earth

 

Compare surfaces of Venus;  Earth; Mars

The four processes

         Plate Tectonics

Plate motion  or continental drift  global plates 

drift movie

Multiple shifts affect continents

New rifts and mountains forming  and sea floor spreading

Earthquakes are mostly along plate boundaries  movie 1   2  

 

Vulcanism

         Near plate boundaries stratovolcanoes

         Hot spots shield volcanoes

Mantle plumes

 

Erosion

Wind

Water 

Glaciers

 

Impacts

 

The Surface

 

Why does the Earth have plates and Venus does not?

 

 

Why are the surfaces so different?

Cooling

Atmosphere

Interrelationships