geology first lecture

1. 1
Lecture # 1
Engineering Geology and Seismology
Origin and Interiors
of the Earth
SAFIULLAH 13CE07 Department of Civil Engineering
Swedish College of Engineering and Technology,Wah Cantt.

2. 2
Geology literally means
"study of the Earth.“
Physical geology examines the materials and
processes of the Earth.
Historical geology examines the origin and evolution of
our planet through time.
Engineering geology is the application of geological
data, techniques and principles to the study of rock
and soil surfacing materials, and ground water.
Seismology is study of the generation, propagation
and recording of the elastic waves and the source that
produce them.

3. Importance of engg geology in Civil Engineering
practice
What is Engineering Geology?
• Engineering geology is the application of geological
3
data, techniques and principles to the study of rock
and soil surficial materials and ground water.
• This is essential for the proper location, planning,
design, construction, operation and maintenance of
engineering structure.

4. 4
Importance of engg geology in Civil Engineering
practice
What does Engineering Geology study?
• Rock, soil, water and the interaction among these
constituents, as well as with engineering materials and
structures.

5. Why Engineering geology?
• Serve civil engineering to provide information in 3
most important areas:
• Resources for construction; aggregates, fills and
borrows.
• Finding stable foundations;
• Mitigation of geological hazards; Identify proplems,
evaluate the costs, provide information to mitigate
the problem
5
Importance of engg geology in Civil Engineering
practice

6. 6
Origin of Earth
Various Theory
1. Nebular Hypothesis
2. Planetesimal Hypothesis
3. Gaseous Tidal Hypothesis
4. Binary Star Hypothesis
5. Gas Dust Clout Hypothesis

7. 7
Nebular Hypothesis
German philosopher, Kant and French mathematician, Laplace
• Earth, planets and sun originated from Nebula.
• Nebula was large cloud of gas and dust. It rotates slowly.
• Gradually it cooled and contracted and its speed increased.
• A gaseous ring was separated from nebula
• Later the ring cooled and took form of a planet
• On repetition of the process all other planets came into being
• The central region, nebula became sun.

8. 8
Objections to Nebular Hypothesis :
• Sun should have the greatest angular momentum because
of its mass and situated in the center, however, it has only
two percent of momentum of the solar system
• How the hot gaseous material condensed in to rings

9. 9
Planetesimal Hypothesis
Chamberlin and Moulton proposed the theory in 1904
• The sun existed before the formation of planets
• A star came close to the sun.
• Because of the gravitation pull of the star, small gaseous
bodies were separated from the sun
• These bodies on cooing became small planet's
• During rotation the small planets collided and form planets

10. 10
Objection to Planetesimal Hypothesis
• The angular momentum could not be produced by
the passing star.

11. 11
Gaseous Tidal Theory
Jeans and Jeffrey proposed the theory in 1925
• Large star came near the sun. Due to gravitational pull a
gaseous tide was raised on the surface of the sun.
• As the star came nearer, the tide increased in size.
• Gaseous tide detached when star moved away.
• The shape of the tide was like spindle.
• It broke into pieces-forming nine planets of the solar system.

12. Interior of earth
 Crust:
 Continental crust (25-40 km)
 Oceanic crust (~6 km)
 Mantle
 Upper mantle (650 km)
 Lower mantle (2235 km)
 Core
 Outer core: liquid (2270 km)
 Inner core: solid (1216 km)
 Values in brackets represent the approximate thickness of each layer

13. Layers of the Earth
The earth is divided into three main layers: Inner core, outer
core, mantle and crust.
The core is composed mostly of iron (Fe) and is so hot that the
outer core is molten, with about 10% sulphur (S). The inner core
is under such extreme pressure that it remains solid.
Most of the Earth's mass is in the mantle, which is composed
of iron (Fe), magnesium (Mg), aluminum (Al), silicon (Si), and
oxygen (O) silicate compounds. At over 1000 degrees C, the
mantle is solid but can deform slowly in a plastic manner.

14. THE CRUST
The crust is much thinner than any of the other layers, and is composed of
the least dense calcium (Ca) and sodium (Na) aluminum-silicate minerals.
Being relatively cold, the crust is rocky and brittle, so it can fracture in
earthquakes.
The shell of the earth, the crust, can be said to have two different
thicknesses.
Under the oceans, it is relatively thin. It varies in thickness from 5 to
8 km. Under the land masses, it is relatively thick. The thickness of the
continental crust varies from 10 to 65 km.

15. THE CRUST
The eggshell analogy for the crust is not an exaggeration. It is
paper thin compared with the radius of the earth which is
approximately 6400 km.
The total weight of the continental crust is less than 0.3% of the
weight of the earth.
Variations in the crust thickness are compensated by the weight
of the water and the differences in the specific gravities of the
crust under the oceans (3.0 to 3.1) and under the continents(2.7 to
2.8).

16. THE CRUST
 If one thinks of the crust as virtually floating on the mantle,
one is less likely to wonder why the earth does not wobble as it
rotates about its axis.
 The weight of the crust plus the mantle has a reasonably
uniform distribution over the globe.

17. THE MOHO
The Moho, or the Mohorovicic Discontinuity, refers to a zone or
a thin shell below the crust of the earth that varies in thickness
from 1 to 3 km.

18. THE MOHO
In seismology, the term "discontinuity" is used in its general
sense. It refers to a change over a short distance of a material
property. In this case, the "short distance" may be as long as 3
km, a trifle compared with the radius of the earth.
In that zone, the P-wave velocity has been observed to
increase from approximately 6 to approximately 8 km/sec.
The Moho is considered to be the boundary between the
crust and the mantle.
The increase in P-wave velocity is ascribed to change in
composition of the medium. Rocks of the mantle are poorer in
silicon but richer in iron and magnesium

19. THE MANTLE
The mantle can be thought of having three different layers. The
separation is made because of different deformational properties in
the mantle inferred from seismic wave measurements.
(1) The upper layer is stiff. It is presumed that if the entire mantle
had been as stiff, the outer shell of the earth would stay put. This
stiff layer of the mantle and the overlying crust are referred to as the
lithosphere. The lithosphere is approximately 80-km thick

20. THE MANTLE
(2) Beneath the lithosphere is a soft layer of mantle called the
asthenosphere.
Its thickness is inferred to be several times that of the lithosphere.
One may think of this as a film of lubricant although film is not exactly
the word for something so thick. It is assumed that the lithosphere,
protruding (meaning: extending beyond) parts and all, can glide over the
asthenosphere with little distortion of the lithosphere

21. THE MANTLE
(3) The mesosphere is the lowest layer of the mantle.
Considering the vagueness in defining the lower boundary of
the asthenosphere it would be expected that the thickness and
material properties of the mesosphere are not well known.
It is expected to have a stiffness somewhere between those of
the lithosphere and the asthenosphere.

22. THE CORE
At a depth of approximately 2900 km, there is a large reduction
(on the order of 40%) in the measured velocity of seismic waves.
The boundary between the mantle and the core is assumed to be
at this depth.
Because no S-wave has been observed to travel through the
material below this boundary for a thickness of approximately 2300
km, it has been inferred that the core comprises two layers.
The 2300-km thick outer layer which is in a molten state and an
1100-km thick inner layer which is solid.

23. THE CORE
It is known that the pressure increases toward the center of the
earth. So does the temperature. The liquid outer layer versus the
solid inner layer is rationalized by recognizing that the melting
point of the material increases (with pressure) at a faster rate than
the temperature as the center of the earth is approached.