Astr 1050    Fri., Dec. 6, 2002

The Material Available

Reason for Jovian Planets

Growth of the Planetisimals

Growth and Differentiation of Planets

Heterogeneous Growth of Planets

Evidence of Assembly Process?    Craters

Craters evident on almost all small “planets”

Even larger planets typically have some

Clearing of the Nebula

Patterns and Predictions

Chapter 17: Terrestrial Planets

“Comparative Planetology”

Four Stages of Planetary Development

Timeline

Earth’s Interior

The Active Earth

Earth’s Atmosphere: Greenhouse Effect

The Moon and Mercury

Patterns in Geologic Activity

What is a crater?

Formation of an impact crater

Examples of craters on the moon

Superposition
(way to get relative ages)

Why do lava flows come out in mare basins?

Problems with the Condensation Model:
Why is the moon so different than the earth?

Effects of late impacts

Moon: Giant Impact Hypothesis

Relative size of core in Mercury

Venus

Expect Venus to be similar to Earth
(but it isn’t)

Why does Venus have much more CO2 in atmosphere than Earth?

Surface Relief of Venus from Radar

Volcanoes

Lava Channels

Pancake Domes

“Ticks”

Corona and a possible model

Slide 39

Lots of Martian Science Fiction

Mars and the Pattern of Geologic Activity
and Atmospheric Loss

Why some atmospheres are lost

Which planets can retain which gasses?

Mars atmosphere today

Mars dust storm

Sand Dunes on Mars

Water ice clouds

Ancient River Channels?
(note channels older than some craters – by superposition)

Recent liquid water?
(water seeping out of underground “aquifer” ?)

Layered Deposits

Where is the water today?