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Lesson4b The Case for water on Mars

Lesson4b The Case for water on Mars. Viking – And the Face

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Page 1: Lesson4b The Case for water on Mars. Viking – And the Face

Lesson4b

The Case for water on Mars

Page 2: Lesson4b The Case for water on Mars. Viking – And the Face

Viking – And the Face

Page 3: Lesson4b The Case for water on Mars. Viking – And the Face

The Martians were BACK!

Page 4: Lesson4b The Case for water on Mars. Viking – And the Face

New Data – Higher resolution

Page 5: Lesson4b The Case for water on Mars. Viking – And the Face

3-D Projection

Page 6: Lesson4b The Case for water on Mars. Viking – And the Face
Page 7: Lesson4b The Case for water on Mars. Viking – And the Face

• Extraordinary claims requires extraordinary evidence. (Carl Sagan)

Page 8: Lesson4b The Case for water on Mars. Viking – And the Face

Today on Mars there is no liquid

Today on Mars there is no liquid water in the form of rivers, lakes or oceans.

Why is there no liquid water on Mars?

Page 9: Lesson4b The Case for water on Mars. Viking – And the Face

.1. It is too cold, all water is frozen

2. It is too hot, all water is a gas3. The pressure is too low for

liquid water4. Mars is a dry world like the

Moon

Page 10: Lesson4b The Case for water on Mars. Viking – And the Face

Temperature on Mars

• Although the temperature is very cold on Mars (-200o F at the poles during winter) the temperature can reach as high as 80o F near the equator during the day.

• So temperatures frequently go above freezing on Mars.

Page 11: Lesson4b The Case for water on Mars. Viking – And the Face

This is a water phase diagram– Pressure verses Temperature

Page 12: Lesson4b The Case for water on Mars. Viking – And the Face

• If you are high in the mountains and you decide to boil water in a pan, what will happen?

Page 13: Lesson4b The Case for water on Mars. Viking – And the Face

.1. Water would boil at a lower temperature

2. Water would boil at a higher temperature

3. What wouldn’t boil at all because the pressure is wrong.

Page 14: Lesson4b The Case for water on Mars. Viking – And the Face

Phase diagram for water

Page 15: Lesson4b The Case for water on Mars. Viking – And the Face

• At high altitudes water boils at a lower temperature than at sea-level.

• What about carbon dioxide?

Page 16: Lesson4b The Case for water on Mars. Viking – And the Face

Phase diagram for C02

Page 17: Lesson4b The Case for water on Mars. Viking – And the Face

• At one Earth atmosphere pressure there is no temperature where CO2 is a liquid.

• Martian atmospheric pressure is 0.006 that of the Earth’s atmosphere at sea-level.

• Let’s look at the water phase diagram again.

Page 18: Lesson4b The Case for water on Mars. Viking – And the Face

On Mars the atmospheric pressure is too low for liquid water.

Page 19: Lesson4b The Case for water on Mars. Viking – And the Face

• On Mars water either exists as ice or as what vapor.

• When the temperature gets high enough the ice sublimes directly to gas.

• This prevents liquid water from existing on the surface of Mars.

Page 20: Lesson4b The Case for water on Mars. Viking – And the Face

A history of Mars through fluid flow (water?)

Page 21: Lesson4b The Case for water on Mars. Viking – And the Face

Large ancient outflows that

begin in chaos regions

Page 22: Lesson4b The Case for water on Mars. Viking – And the Face

Large outflow regions

Page 23: Lesson4b The Case for water on Mars. Viking – And the Face

• http://www.google.com/mars/

Page 24: Lesson4b The Case for water on Mars. Viking – And the Face

Dendriticdrainage valleys

found in hilly regions

Page 25: Lesson4b The Case for water on Mars. Viking – And the Face

Dendritic Drainage Valleys

Page 26: Lesson4b The Case for water on Mars. Viking – And the Face

Characteristics of fluid flowRiver meander

Page 27: Lesson4b The Case for water on Mars. Viking – And the Face

What causes a river to meander?

• As water flows along the surface it always flows to the lowest level. This is because gravity is the force causing the water to flow.

• The path of water flow is initially dictated by the contour of the ground that the water is flowing over.

Page 28: Lesson4b The Case for water on Mars. Viking – And the Face

What will happen to the water’s speed as it approaches the curve?

Page 29: Lesson4b The Case for water on Mars. Viking – And the Face

What will happen to the water’s speed as it approaches the curve?

Page 30: Lesson4b The Case for water on Mars. Viking – And the Face

.1. The water on the outside of the curve will move more slowly than the inside of the curve

2. The water on the outside of the curve will move more rapidly

3. Water is a liquid so it will all move at the same speed

Page 31: Lesson4b The Case for water on Mars. Viking – And the Face

What will happen to the water’s speed as it approaches the curve?

Fast moving water

Slow moving water

Page 32: Lesson4b The Case for water on Mars. Viking – And the Face

Fast moving water erodes soil more effectively

As Time goes by

Page 33: Lesson4b The Case for water on Mars. Viking – And the Face

Characteristics of fluid flowRiver meander

Page 34: Lesson4b The Case for water on Mars. Viking – And the Face

Other characteristics

Cut Bank

Deposition Bar (Sand bar)

Page 35: Lesson4b The Case for water on Mars. Viking – And the Face

• A deposition bar is composed of rocks, sand and dirt that is carried along in the water flow.

• Where should you expect a deposition bar to form in a river?

Page 36: Lesson4b The Case for water on Mars. Viking – And the Face

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1. Where the water moves the slowest because debris will drop out of the water

2. Where the water moves the fastest because it can then carry debris

3. Usually on the outside of the curve

Page 37: Lesson4b The Case for water on Mars. Viking – And the Face

Other characteristics

Cut Bank

Deposition Bar (Sand bar)

Page 38: Lesson4b The Case for water on Mars. Viking – And the Face
Page 39: Lesson4b The Case for water on Mars. Viking – And the Face

Deposition bar is always on the inside curve of a river

• Fast moving water on the outside curve cuts into the river bank and creates a cut-bank.

• Slow moving water on the inside curve drops material carried by the water forming a deposition bar.

• Over time the cut-bank erosion moves the river farther out, and the deposition fills in as the curves become more pronounced.

Page 40: Lesson4b The Case for water on Mars. Viking – And the Face

Eventually curve can become pinched off and oxbow lake forms

Page 41: Lesson4b The Case for water on Mars. Viking – And the Face

Mars from the HiRISE Camera

Page 42: Lesson4b The Case for water on Mars. Viking – And the Face

Wind erosion

Harder river bed material

Page 43: Lesson4b The Case for water on Mars. Viking – And the Face

Which is older, the river bed or the surface around the river bed?

Page 44: Lesson4b The Case for water on Mars. Viking – And the Face

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1. The surface surrounding the river bed, because the bed is on top.

2. The river bed because it flowed over the surface around it.

3. The river bed. It has a greater crater density.

Page 45: Lesson4b The Case for water on Mars. Viking – And the Face

The river bed is older. Crater density is higher.

Page 46: Lesson4b The Case for water on Mars. Viking – And the Face

Ancient meander on Mars

Page 47: Lesson4b The Case for water on Mars. Viking – And the Face

Dendritic (tree-like) drainage valleys

Earth Mars

Page 48: Lesson4b The Case for water on Mars. Viking – And the Face

• When ground slope is steep water runs quickly in small streams, which eventually run together to form a tributary system for the main river.

Page 49: Lesson4b The Case for water on Mars. Viking – And the Face

Stream-lined islands

Page 50: Lesson4b The Case for water on Mars. Viking – And the Face

Stream-lined islands

Page 51: Lesson4b The Case for water on Mars. Viking – And the Face

Fluting – Longitudinal lines caused by fluid flow

Page 52: Lesson4b The Case for water on Mars. Viking – And the Face

Changes in water level

Page 53: Lesson4b The Case for water on Mars. Viking – And the Face

Large outflowsThey look like

enormous flooding events, but they are not tied to

tributary systems like we would see

on Earth where water comes from

precipitation

Page 54: Lesson4b The Case for water on Mars. Viking – And the Face

SourceChaos

Regions

Page 55: Lesson4b The Case for water on Mars. Viking – And the Face
Page 56: Lesson4b The Case for water on Mars. Viking – And the Face

Sapping Springs

Very hard Caprock

Softer rock like sandstone

Sapping Springs

Page 57: Lesson4b The Case for water on Mars. Viking – And the Face

Sapping Springs as time goes by

Very hard Caprock

Softer rock like sandstone

Sapping Springs

Page 58: Lesson4b The Case for water on Mars. Viking – And the Face

Sapping Springs as time goes by

Very hard Caprock

Softer rock like sandstone

Sapping Springs

Fracture

Page 59: Lesson4b The Case for water on Mars. Viking – And the Face

Sapping Springs as time goes by

Very hard Caprock

Softer rock like sandstone

Sapping Springs

Fracture

Chaos

Page 60: Lesson4b The Case for water on Mars. Viking – And the Face

Water appears to come from underground sources