Properties of the Earth

I. Density
A. Density is the mass divided by the volume; d = m/v
B. Density of the Earth is about 5.5 g/cm3
1. This is not uniform
2. By comparison, the density of water is 1.0 g/cm3
II. Internal structure
A. determined from seismology: reflection of earthquake waves
1. P-waves (primary or "push"; compressional) : faster
2. S-waves (secondary or "shake"; shear) : slower, cannot go through liquid
B. discontinuities in the paths of seismic waves indicate layering



Density % volume % mass
1. crust: 2.0-3.5 g/cm3 2% <1%
2. mantle: 3.5-5.0 g/cm3 82% 68%
3. core: ~10.8 g/cm3 16% 32%


C. We know something about the internal composition because of meteorites (meteorites are rocks on Earth derived from outside Earth)
1. Iron meteorites (metallic Fe minerals); similar to core material
2. Stony meteorites
i. Achondrites (do not contain chondrules); similar to mantle & crust material)
ii. Chondrites (contain chondrules, silicate minerals in the shape of spherules); primitive planetary material
D. The eight most common elements in Earth's crust

Element Symbol % by weight % by volume
Oxygen O 46.6 93.8
Silicon Si 27.7 0.9
Aluminum Al 8.1 0.8
Iron Fe 5.0 0.5
Calcium Ca 3.6 1.0
Sodium Na 2.8 1.2
Potassium K 2.6 1.5
Magnesium Mg 2.1 0.3
All other elements
1.5 --


E. Sources of heat in the earth
1. Geothermal gradient
2. Radioactive heat from decay of radioactive uranium, thorium, and potassium

Last update 2/22/2005
Webpage designed by Hiram Jackson.
Contact Geology webmanager, Hiram Jackson, at jacksoh@crc.losrios.edu