Week 2: - PowerPoint PPT Presentation

About This Presentation
Title:

Week 2:

Description:

Geologists seeking evidence of the oldest rocks on earth are up against large odds... ... our ... http://nssdc.gsfc.nasa.gov/planetary/image/near_mathilde3.jpg ... – PowerPoint PPT presentation

Number of Views:23
Avg rating:3.0/5.0
Slides: 16
Provided by: graemew
Category:
Tags: week

less

Transcript and Presenter's Notes

Title: Week 2:


1
Week 2 When the world was young...
EPSC233-001 Earth Life History (Fall 2002)
2
Recommended reading STANLEY Earth System
History Chapter 11.
Keywords Archean eon (4.6-2.5 billion years
ago), nebula, planets, meteorites, comets,
differentiation, oceanic crust, continental
crust, plate tectonics, mantle convection.
3
Geologists seeking evidence of the oldest rocks
on earth are up against large odds...
... our planet is a huge recycling engine.
4
Our solar system started with the explosion of a
supernova, the dying stage of a star. Clouds of
gas and dust were compressed by the shock wave,
giving rise to a solar nebula.
5
  1. a slowly rotating cloud of gases called a
    nebula starts to collapse (gravitational
    attraction)
  2. the cloud continues to condense and flattens, a
    gaseous protostar and solid planetesimals grow
  3. the sun lights up, solar wind vapourizes dust and
    blows it away
  4. the nebula clears up a solar system is born.

6
Dust accreted into larger bodies.
7
Planets which grew from planetesimals which
condensed close to the sun are rocky, those far
from the sun are gas- and ice-rich
8
http//nssdc.gsfc.nasa.gov/planetary/image/near_ma
thilde3.jpg
What did not grow into planets became asteroids
(rocky)...
Or comets (dirty snowballs)
http//www.jpl.nasa.gov/comet/hyakutake/gif/burger
2.jpg
9
Dates from about 70 meteorites
Allende meteorite (Mexico) 4.56 B.y. old, sample
of the stuff from the sun (- H, He).
10
Impacts and radioactive decay led to melting
differentiation
11
Around 4.5-4.4 Ga, an impact with a Mars-sized
body had a great effect on Earths history. All
volatiles were lost from Earth, and the
Moon formed from the impactor and
terrestrial debris.
12
Lunar basalts on the moon
Apollo 17, oldest lunar basalt samples 4.55 ?
0.1 b.y. and 4.60 ? 0.1 b.y.
13
Initially the Moon was hot-- covered by a magma
ocean.
But, the Moon is small and cooled rapidly. It
now has no volcanic activity and is
both biologically and geologically lifeless.
14
The Earth, bigger, is cooling more slowly and
remains geologically active. Crust showing scars
of early meteoritic impacts has been recycled.
Manicouagan crater 100 km diam (200 m.y. ago).
15
Why is there a difference? Earth is a
geologically active planet, the Moon is not.
Top few hundred km of Earth are broken into
tectonic plates which are constantly being
created and destroyed.
Write a Comment
User Comments (0)
About PowerShow.com