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Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Apr 01, 2015

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Page 1: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Lesson2d

Volcanoes

Page 2: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Olympus Mons (volcano on Mars) compared to Arizona

Page 3: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Olympus Mons on Mars

• Google Mars• Mars Reconnaissance orbiter – HiRISE• Basal Scarp on Olympus Mons

Page 4: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 5: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Hawaiian Islands

Page 6: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 7: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Mt. Saint Helens – May 18, 1980

Page 8: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 9: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

• The lava from the Hawaiian volcanoes is very low in silica and it flows easily across the surface, all the way to the ocean.

• What can you conclude about the Hawaiian volcanoes?

Page 10: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

.

1 2 3 4

0% 0%0%0%

1. Without silica their slopes will be steep

2. The magma must not be contaminated with crustal material

3. Both 1 & 24. None of the above

Page 11: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Lava Composition• Felsic lava (Strato-volcanoes) -- high viscosity and

strength, high in silica, aluminium, potassium, sodium, and calcium, forming a polymerized liquid rich in feldspar and quartz.

• Mafic or basaltic lavas (Shield volcanoes) are typified by their high ferromagnesian content, Basaltic magma is high in iron and magnesium, and has relatively lower aluminium and silica. This is mantle material.

• Note: Similar to the lava in the Mid-atlantic ridge.

Page 12: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Mt. Rainer overlooking Tacoma

Page 13: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 14: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Shield volcanoes

• Shield volcanoes get their appearance because the low viscosity lava flows out and spreads easily.

• Slopes for Shield volcanoes are around 1o – 5o

• Slopes for Stratovolcanoes are ~ 30o near summit and ~10o on outer slopes.

Page 15: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Shield volcanoes arise from mantle magma plumes.

Page 16: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Hot magma from near the core of the Earth rises in a plume.

Page 17: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Detailed model of plume rise.Slow process, last slide is 76.8 Million years.

Page 18: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Oldest Island

Youngest Island

Page 19: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 20: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Oldest

Youngest

Page 21: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Increasing age

Page 22: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 23: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Evidence.• Magma plumes take many millions of years to

form and rise up through the mantle.• The Big Island is the only one to have active

volcanoes today.• The farther away in the chain of islands you

get the older the island is.

• Given all this information, how did the Hawaiian Island chain form?

Page 24: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

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1 2 3

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1. From magma coming from a Pacific ridge similar to the mid-Atlantic ridge

2. From the wandering of the magma plume under the sea floor

3. From the motion of the Pacific Oceanic Plate over the magma plume.

Page 25: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Ocean plate motion relative to the mantle plume (Plate Tectonics)

Page 26: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.
Page 27: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

How can we determine how fast the Pacific plate moving?

Page 28: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Age from radiometric datingDistance is just measured

• Age = 60,000,000 years• Distance = 5000 km.• Speed = Distance/time • Speed = (5 x 103 km)/(6 x 107 years) or• Speed = (5 x 106 m)/(6 x 107 years)• Speed = 0.083 meters/year or 8.3 cm/year.

Page 29: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Velocity Vectors in Jules Verne Voyager Velocity vectors in Google Earth

http://jules.unavco.org/VoyagerJr/EarthScope Google Earth w/http://pboweb.unavco.org/products/velocity/pbo_final_frame.kmzhttp://facility.unavco.org/data/maps/maps.html

Using GPS velocity vectors to study plate motion

Page 30: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

GSRM Model of Kreemer and Holt

Observed GPS Velocities

Plus Earthquake Slip directions

Plate TectonicModel with DeformableBoundaries Model Velocities and Plate

Boundary Strain5170 geodetic velocities from 86 different studies

Global Plate Motions and Boundary Zones

Page 31: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Age from radiometric datingDistance is just measured

• Age = 60,000,000 years• Distance = 5000 km.• Speed = Distance/time • Speed = (5 x 103 km)/(6 x 107 years) or• Speed = (5 x 106 m)/(6 x 107 years)• Speed = 0.083 meters/year or 8.3 cm/year.

• Geodetic measurement of plate motion is 10.3 to 11.8 cm/year

Page 32: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Results we can use

• A shield volcano arises from a deep mantle plume.

• Shield volcanoes have gentle slopes (less than 5o).

• A chain of shield volcanoes can indicate plate tectonics is occurring.

Page 33: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Mons Rumker

Lunar volcano

Mons Rumker

Lava flow

Page 34: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Mons Rumker – Exaggerated viewHeight ~ 1100 meters

Diameter ~ 70 km.

Page 35: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Slope Measurement

1,100 m

35,000 m

Angle ϴ

Angle ϴ1,100 m

35,000 m

Page 36: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Which trigonometric function should you use to find the angle?

1,100 m

35,000 m

Angle ϴ

Angle ϴ1,100 m

35,000 m

Page 37: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

• The correct answer is Tangent

• Tan(θ) = opposite/adjacent• Tan(θ) = 1100/35000• Tan(θ) = 0.314• Θ = Tan-1(0.314)• Θ = 1.8o

Page 38: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

• The correct answer is Tangent

• Tan(θ) = opposite/adjacent• Tan(θ) = 1100/35000• Tan(θ) = 0.314• Θ = Tan-1(0.314)• Θ = 1.8o

Mons Rumker is a shield volcano

Page 39: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Olympus Mons – Largest volcano on Mars (and entire solar system)

Page 40: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Olympus Mons compared to Arizona

Page 41: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Topographical map of Mars

Olympus Mons

Page 42: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Estimate the ratio

of the opposite

to adjacent

sides

Page 43: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

• Using the ratio of 20km/320km = 0.0625

That gives θ = 3.6o

Olympus Mons is a shield volcano.

Page 44: Lesson2d Volcanoes. Olympus Mons (volcano on Mars) compared to Arizona.

Comparison