DOC PREVIEW
OU ASTR 1514 - Tectonism, Volcanism, and Erosion

This preview shows page 1 out of 4 pages.

Save
View full document
View full document
Premium Document
Do you want full access? Go Premium and unlock all 4 pages.
Access to all documents
Download any document
Ad free experience
Premium Document
Do you want full access? Go Premium and unlock all 4 pages.
Access to all documents
Download any document
Ad free experience

Unformatted text preview:

ASTR 1514 1st Edition Lecture 14Tectonism Chapter 6.3Tectonism – The deformation of Earth’s crust.- The Lithosphere is broken into plates around the Earth they are drifting- Continental Drift and plate tectonics describe the movement of those plates- Crustal plates move due to convection, the rising and falling of hot/cold material. - Continental plates are made of lower density rock so they float on top and are dragged around.- Earth has seven major plates and six smaller ones that are all continually moving. - Plates can separate, collide or move parallel to each-other. There are several types of motion/features that are due to tectonic plates1. Sea-Floor Spreading- Two plates separate and new lithosphere is created at the boundary of their separation. - Sea-floor spreading gives us direct evidence for change in Earth’s magnetic field direction. 2. Plate Collisions (Convergence)- Continental plates float on the mantle where they collide and form mountains. - Example: Indian plate colliding or converging with the Eurasian plate to form the Himalaya Mountains. 3. Subduction- Also a type of converging or colliding plate boundary. - Occurs when dense sear-floor crust sinks under less dense continental plates. - Subducting plate bends in a “plastic” manner due to water content. - Subducting plate sinks due to thickness and weight, weight pulls it down.- Ex: Coast of Oregon/Washington. 4. Continental Plates pull apart (Diverge)- When Continental plates pull apart a rift valley may be formed- Ex: Great African Rift Valley. And Iceland Rift Valleys. 5. Plates sliding past each other (Transform Boundary)- Plates may slide sideways with respect to one another- Ex: San Andreas Fault in California. 6. Hot Spots- Hot spots mark a plume of hot mantle - The pacific plate moves over hot spots creating a string of islands. - Ex: Hawaiian Islands. Earthquakes commonly occur along plate boundaries, most often occur along converging or colliding plate boundaries. Tectonics onOther Terrestrial Planets- Only Earth has its crust broken up into plates- All terrestrial planets have seen some form of disruption. Ex: Mercury’s surface shrank after it cooled, leaving cliffs.- Mars has experienced extensive tectonism, it is home to the Valles Marineris (Giant Rift Valley) that is four times deeper than Earth’s Grand Canyon. - Venus may have different forms of tectonism, with melting and overturning of the crust and some hot spots. Volcanoes Chapter 6.4- Volcanoes form (primarily) at hot spots and plate boundaries.- Friction raises the temperature of the rock along plate boundaries to its melting point. - Two different kinds of Volcanoes1. Shield Volcanoes Formed from very fluid like lava Low water content in the rock Formed from low – viscosity (Runny, liquidy) lava from basaltic rock. 2. Composite Volcanoes  Formed from pasty viscous (thick and slow like molasses) lava High water content in rocks Lithosphere created at mid-ocean ridges gains thickness and water due to sediment build up and dead animals When the heavy rock sinks below the continental plate it is heated due to friction producing composite volcanoes. Common along subduction zones Explosive Volcanic Activity.The Moon- Does NOT have volcanoes- Lava flows smoothed out parts of its surface, could’ve been impacts cracking surface.Mercury- Also has smooth surfaces from past volcanism’- A few inactive volcanoes have been identified on Mercury.Mars- Volcanoes on Mars are the largest mountains in the Solar System- Shield Volcanoes- Olympus Mons – Highest Volcano in the entire Solar System- No currently active volcanoes on Mars- Mars is a small planet that possibly cooled too much. Venus - Has most of the volcanoes of the terrestrial planets- All of Venus’s volcanoes are shield volcanoes, so no plate tectonics- Surface too hot and dry so plates dried out - Few craters: Surface of Venus is about half a billion years old, could have been a global crust break up and turnover. - Venus’s volcanoes are mostly inactive- Monitoring of sulfur dioxide in Venus’s atmosphere has shown changes over past 30 years indicating a little volcanic activity. - Baltis Vallis – Longest lava flow in solar system. Erosion Chapter 6.5- Erosion is the wearing a way of a planet’s surface by mechanical action. (Running water, Wind, etc.)- Wind modifies the surfaces of Venus and Mars- Landslides and radiation from the Sun also change the surface. - On Earth, the only planet with liquid water today, wind and water strongly erode the surface.- Water modified the surface of Mars in the past and it exists as ice today. - Water ice exists on Mars, the moon, and possibly Mercury. Geology of Oklahoma- Much of Oklahoma is Sedimentary rock- Used to be covered by a shallow sea that rose and fell over the eons- Metamorphic Rocks in Oklahoma: Ouachita Mountains/Arbuckle Mountains.- Igneous Rocks in Oklahoma: Wichita Mountains- Wichita Mountains formed from lava flowing into a rift valley. It was then buried under layers of shale. Uplifted due to the collision between North America and South America. - New Madrid Fault is a failed rift zone, an Earth-quake in 1811-1812 caused Mississippi River to run backwards.- Magnitude 6 Earth-quake expected to occur every 100


View Full Document

OU ASTR 1514 - Tectonism, Volcanism, and Erosion

Download Tectonism, Volcanism, and Erosion
Our administrator received your request to download this document. We will send you the file to your email shortly.
Loading Unlocking...
Login

Join to view Tectonism, Volcanism, and Erosion and access 3M+ class-specific study document.

or
We will never post anything without your permission.
Don't have an account?
Sign Up

Join to view Tectonism, Volcanism, and Erosion 2 2 and access 3M+ class-specific study document.

or

By creating an account you agree to our Privacy Policy and Terms Of Use

Already a member?