see page 11 of the text book (Understanding Earth by Press and Siever)
The composition of the Earth has been figured out through a variety of
methods. The deepest drill hole is about 12 km deep and cost
over $100 million. Volcanoes bring up foreign rocks (known as
xenoliths) from several hundred km depth. Since the Earth is some
12,000 km in radius, our knowledge of the upper 200 km may be completely
irrelevant.
Nonetheless, we are fairly
confident of we know what the Earth
is made of because we can determine the chemistry of meteorites
born of the same womb, hence can be reasonably expected to
have the same chemistry. From analysis of these meteorites (and also
the composition of the Sun reveals that
the Earth is made up of Iron (35%), Oxygen (30%), Silicon (15%)
Magnesium (13%) and traces of the other elements.
If you pick up your ordinary everyday average rock, however,
you will immediately notice that it can't be 35% iron. In fact there
is no where near that much iron in the crust in general. Looking at
Figure 1.8 in the text, you will see that in fact the crust (which we
can study directly) has only a little Iron (6%). This means that the
iron must be "hidden".
From the orbits of satellites, we know that the Earth has a very dense core.
We therefore surmise that the iron that the Earth was born with migrated
at some point down to the core. Iron and a little nickle (which is also
missing in the crust) together have the right density to explain the
density structure of Earth.
Thus, the Earth is far from a
homogeneous body but has differentiated into a metallic core (radius of
about 6000 km) and a more
rocky mantle. We walk about on the less dense froth ejected from the
mantle known as the crust which varies in thickness from about 5km to
about 60 km.
Earth Statistics
(from here )
Mass (kg) 5.976e+24
Mass (Earth = 1) 1.0000e+00
Equatorial radius (km) 6,378.14
Equatorial radius (Earth = 1) 1.0000e+00
Mean density (gm/cm^3) 5.515
Mean distance from the Sun (km) 149,600,000
Mean distance from the Sun (Earth = 1) 1.0000
Rotational period (days) 0.99727
Rotational period (hours) 23.9345
Orbital period (days) 365.256
Mean orbital velocity (km/sec) 29.79
Orbital eccentricity 0.0167
Tilt of axis (degrees) 23.45
Orbital inclination (degrees) 0.000
Equatorial escape velocity (km/sec) 11.18
Equatorial surface gravity (m/sec^2) 9.78
Visual geometric albedo 0.37
Mean surface temperature 15°C
Atmospheric pressure (bars) 1.013
Atmospheric composition
77%
21%
2%
Composition of the Earth
Earthquakes and the Earth's interior
Earth Structure
Most of what we know about the Earth comes from
seismology, or the study of earthquakes.
When the Earth breaks, it quakes and
sometimes generates sound waves strong enough to blow
houses down. There are special "listening" stations that record these
sound waves called "seismometers". Large earthquakes can be "heard" the
world over and these seismic messages have travelled through the Earth.
Lisa Tauxe