Upload
easter-holt
View
214
Download
0
Embed Size (px)
Citation preview
1
Terrestrial World Surfaces
Solid rocky surfaces shaped (to varying degrees) by: Impact cratering
Volcanism
Tectonics (gross movement of surface by interior forces)
Erosion (by impacts or by weather)
2
The Earth's Surface
Unlike Mercury and the Moon, impact craters are few and far between on the Earth.
From a crater counting perspective the surface is “young”
The Earth has been impacted as frequently, if not more frequently than the Moon, yet those scars have been erased
Note that the Earth's atmosphere offers little protection against the large impactors that produce the craters seen above.
3
The Earth's Surface
The Earth's larger size means that it is still geologically active.
New surface is being created and old surfaces are being resurfaced regularly.
The Earth also retains an atmosphere which makes for efficient erosion of craters.
4
Geological Activity vs. Planetary Size
It's no coincidence that the smallest worlds above are the ones that are heavily cratered.
The larger a world is the more readily it retains its internal heat. A pea cools off much more quickly than a potato
Earth and Venus are still hot in the interior and molten material can reach and re-surface the surface.
5
How Lightly Cratered?
6
How Lightly Cratered?
7
Two Distinct Terrains: Continents and Basins The Earth has two distinct surface levels
Continents: Thick portions of the crust that occupy high elevations
Basins: Thiner crust occupying the “lowlands”
8
Two Distinct Terrains: Continents and Basins Interestingly, there is just enough water on Earth to fill the basins.
9
Two Distinct Terrains: Continents and Basins Interestingly, there is just enough water on Earth to fill the basins. It didn't have to be this way, consider Jupiter's moon Europa
The world is submerged under a 60 mile deep ocean frozen at the top.
10
Two Distinct Terrains: Continents and Basins In contrast, Venus is completely different
11
Crustal Plates: Unique to Earth?
Mountain chains and tectonic activity delineate regions of the Earth's surface.
12
Crustal Plates: Unique to Earth?
Mountain chains and tectonic activity delineate regions of the Earth's surface.
13
A Thin Crust Enables Activity
14
Mantle Convection
Motions in the Earth's interior (think Lava Lamp) fracture and move the crust about.
15
Mantle Convection
Motions in the Earth's interior (think Lava Lamp) fracture and move the crust about.
Twenty crustal plates move under this influence (about 1 inch a year)
16
Mantle Convection
Motions in the Earth's interior (think Lava Lamp) fracture and move the crust about.
Twenty crustal plates move under this influence (about 1 inch a year)
17
Mantle Convection
Motions in the Earth's interior (think Lava Lamp) fracture and move the crust about.
Twenty crustal plates move under this influence (about 1 inch a year)
18
Plate Motion Drives Geology
19
Making an Ocean
The Atlantic Ocean has swung open in the last 300 million years. Given that amount of time one inch per year is plenty.
20
Earthquakes
Earthquakes are the result of “sticky” plate boundaries. Stress builds up followed by a sudden slip.
21
Continental Drift Continues
22
Continental Drift Continues
23
Erosion and Continental Craters
Some of the continental crust is quite old. However, erosion is a powerful force and fresh mountain range (e.g.
the Rockies) can be worn down in just a hundred million years. Craters don't stand much of a chance.
24
How Lightly Cratered?