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Conversations with the Earth Tom Burbine [email protected]

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Conversations with the Earth Tom Burbine [email protected]. Quiz on Thursday. Moon Mars. Need to account for these things when you form the Moon. The Moon's low density (3.3 g/cm 3 ) shows that it does not have a substantial iron core like the Earth does. - PowerPoint PPT Presentation
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Conversations with the Earth Tom Burbine [email protected]
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Page 1: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Conversations with the Earth

Tom [email protected]

Page 2: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Quiz on Thursday

• Moon• Mars

Page 3: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Need to account for these things when you form the Moon

• The Moon's low density (3.3 g/cm3) shows that it does not have a substantial iron core like the Earth does.

• Moon rocks contain few volatile substances (e.g. water), which implies extra baking of the lunar surface relative to that of Earth.

• The relative abundance of oxygen isotopes on Earth and on the Moon are identical, which suggests that the Earth and Moon formed at the same distance from the Sun.

Page 4: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Oxygen Isotopes• There are three stable isotopes of oxygen• They have masses of 16, 17, and 18 atomic mass

units %

• 16O ~99.762• 17O ~0.038 • 18O ~0.200• The oxygen isotopic ratios (17O /16O and 18O/16O of

silicate rocks from the Earth and Moon are the same and are different from most meteorites and Mars

Page 5: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 6: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 7: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 8: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Geologic Time Scale

• A scheme to relate stratigraphy to time

Page 9: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Ma – million years

http://geomaps.wr.usgs.gov/socal/geology/geologic_history/images/geologic_time_scale.jpg

Why is there such a large age difference between the beginning and end of theCambrian?

Page 10: Conversations with the Earth Tom Burbine tburbine@framingham.edu

• Cambrian is the earliest period where rocks are found with numerous large multicellular organisms that could be found as fossils

Page 11: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://pubs.usgs.gov/gip/geotime/fossils.html

Page 12: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://creationwiki.org/pool/images/thumb/c/c5/Evolution_timeline.jpg/400px-Evolution_timeline.jpg

Page 13: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://www.cityastronomy.com/geologic-earth-moon-graphic.bmp

Page 14: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://www.psrd.hawaii.edu/WebImg/LunarTimeScale.gif

http://www.etsu.edu/physics/etsuobs/starprty/21200mwc/moonmap.jpg

Page 15: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Mars

http://www.daviddarling.info/images/Mars_large.jpg

Page 16: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Mars• Names after Mars, Roman God of War• Mars has two tiny natural moons, Phobos and

Deimos, which orbit very close to the planet and are thought to be captured asteroids.

• Both satellites were discovered in 1877 by Asaph Hall, and are named after the characters Phobos (panic/fear) and Deimos (terror/dread) who, in Greek mythology, accompanied their father Ares, God of War

Page 17: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Percival Lowell (1855-1916)

• Lowell produced intricate drawings of the Red Planet

• Finding hundreds of straight lines (termed "canals")

Page 18: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 19: Conversations with the Earth Tom Burbine tburbine@framingham.edu

He thought

• Lowell concluded that the bright areas were deserts and the dark were patches of vegetation

• Lowell thought the canals were constructed by intelligent beings who once flourished on Mars.

Page 20: Conversations with the Earth Tom Burbine tburbine@framingham.edu

For years

• People thought life could exist on Mars and Venus, the closest planets to Earth

Page 21: Conversations with the Earth Tom Burbine tburbine@framingham.edu

However,

• Venus is extremely hot (~700-800 K)• Atmospheric pressure is 90 times that of Earth

Page 22: Conversations with the Earth Tom Burbine tburbine@framingham.edu

What happened on October 30, 1938?

Page 23: Conversations with the Earth Tom Burbine tburbine@framingham.edu

What happened on October 30, 1938?

• http://sounds.mercurytheatre.info/mercury/381030.mp3

Page 24: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Mars

• The average recorded temperature on Mars is -63 °C with a maximum temperature of 20 °C and a minimum of -140 °C

• Atmospheric pressure is 1/100 of Earth’s• Mars is often enveloped by planet-wide dust

storms

Page 25: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Dust Devils

• http://en.wikipedia.org/wiki/Image:Marsdustdevil2.gif

Page 26: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Dust Devils

• Dust devils are smaller and weaker than tornadoes• They are caused by convection on hot, calm

summer days. • Air near the surface becomes much warmer than

the air above, creating an updraft.

Page 27: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 28: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Key to Life

• All life on Earth depends on water• So if you find water, you may find life

Page 29: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Habitable Zone

• The region around a star in which planets could potentially have surface temperatures which liquid water could exist

Page 30: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 31: Conversations with the Earth Tom Burbine tburbine@framingham.edu

In the past

• Mars appeared to be warmer and wetter

Page 32: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Atmospheres

• Layer of gases that surround a body with sufficient mass

• Gravity keeps the gases around the body

Page 33: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Atmospheric Pressure• Pressure due to the weight of air above the

measurement point• Pressure is force per unit area• Standard atmosphere is defined as being

precisely equal to 101,325 Pascals where a Pascal is 1 N/m2

• 1 bar = 100,000 pascals• Pressure in the solar nebula was ~10-4-10-8 bars

Page 34: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Phase Diagram

http://img.search.com/thumb/d/dc/Phase-diag.png/300px-Phase-diag.png

Page 35: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://science.nasa.gov/headlines/y2000/ast29jun_1m.htm

Mars

Page 36: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://images.encarta.msn.com/xrefmedia/aencmed/targets/illus/cha/T073590A.gif

Page 37: Conversations with the Earth Tom Burbine tburbine@framingham.edu

http://www.splung.com/heat/images/phases/phasediagram.png Temperature

Pre

ssur

e

Page 38: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 39: Conversations with the Earth Tom Burbine tburbine@framingham.edu
Page 40: Conversations with the Earth Tom Burbine tburbine@framingham.edu

Any Questions?


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