Dr. Neil S. Suits [email protected] WF: 9:20-1130; 896-5931.

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Dr. Neil S. Suits [email protected] du WF: 9:20-1130; 896-
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Transcript of Dr. Neil S. Suits [email protected] WF: 9:20-1130; 896-5931.

Page 1: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Dr. Neil S. Suits

[email protected]

WF: 9:20-1130; 896-5931

Page 2: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Our spheres of study:

Lithosphere lots

Hydrospheresome

Pedosphere little

Atmospheresome

Biosphere little

Noösphere no

Page 3: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Credit where credit is due:

I’ve gotten most of this material from web sources and textbooks resources, and from other Earth Science courses available on the Web. I will give the web addresses and proper credit as the course moves along.

Page 4: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Rocks

Igneous

Sedimentary

Metamorphic

Volcanoes

Intrusions

Weathering

SoilsErosion

WaterUnderground Surface

Oceans

Wind

Glaciers

Fossils

Earth History

Earth’s Interior

Earthquakes

Mountains

Plate Tectonics

Other Planets

Mineral Resources

What is Physical Geology?

Page 5: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

But first…

If these rocks could talk, what would they tell us?

Page 6: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

~14.9 GA (GigaAnnum, i.e,

Billion Years)

today

Page 7: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

~ 300,000 years after the Big Bang

The first map of the Universe. Not homogeneous.

Cosmic microwave background (CMB) anisotropy. First detected by the COBE DMR instrument.

Page 8: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Typical spiral galaxy. Similar to ‘our’ Milk Way Galaxy’

Page 9: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

http://faculty.rmwc.edu/tmichalik/NebandStar.htm

Star Birth and Formation

Page 10: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.
Page 11: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.
Page 12: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Magnetic fields around a sunspot

Page 13: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

SUN Rocky inner planets

The giant Gas planets of the outer solar system

Hydrogen, Helium, methane, water, ammonia

Silicates with Iron/Nickel cores

Hyd

rog

en (74%

), so

me h

elium

(24%)

Page 14: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Our moon: Luna

Page 15: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Current hypothesis: Luna was formed as a result of an impact by a Mars-sized object in the early stages of Solar System formation.

Page 16: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Lunar impact craters

Page 17: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Crater Tycho

Page 18: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Close up of Tycho

Page 19: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

The lunar interior: crust, mantle core

Mostly rock, very small iron core; cooled and tectonically inactive

Page 20: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Mars

Page 21: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Craters on Mars

Page 22: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

The Martian ice cap

Frozen water?

Page 23: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

View of the surface of Mars from the Martian lander

Page 24: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Wind-formed dunes on MarsAtmosphere: 0.7% of the Earth’s atmospheric pressure; 95%

Carbon Dioxide (CO2), 3% Nitrogen (N2); 1.7% Argon, 0.1% Oxygen (O2)

Page 25: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Olympus Mons

The largest mountain in the Solar System

Why is it so big?

~ 625 km (324 miles) diameter

Scarp Height ~ 6 km (4 miles)

Page 26: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.
Page 27: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Olympus Mons on an overcast day

Page 28: Dr. Neil S. Suits nsuits@msubillings.edu WF: 9:20-1130; 896-5931.

Evidence for water on mars