Chapter 1 Introduction SE
Chapter 1 Introduction SE
Chapter 1 Introduction SE
DEFINITION OF MECHANICS
Mechanics may be defined as the physical science which describes and predicts
the conditions of rest or motion of bodies under the action of force systems. In
other words, where there is motion or force, there is mechanics.
Conditions involving speed of bodies close to the speed of light (about 300 x 106
m/s) and conditions requiring consideration of bodies with extremely small mass
and size (such as subatomic particles with sizes in the order of 10-12 m and
smaller) cannot be adequately described by Newton’s Laws. These extreme
conditions are treated in Relativistic Mechanics and Quantum Mechanics.
However, for a vast range of problems between these extremes, Newton’s Laws
give accurate results and are far simpler to apply. Although the fundamental
principles of Newtonian Mechanics are surprisingly few in numbers, they have
exceedingly wide range of applications. Modern research and development in the
fields of vibrations, stability and strength of machines and structures, rocket and
spacecraft design, robots, automatic control, engine performance, fluid flow,
electrical machines and apparatus are highly dependent upon the basic principles
of mechanics.
As seen, mechanics of rigid bodies is divided into two parts as “Statics” and
“Dynamics”.
Statics, is the branch of mechanics that deals with the bodies that are acted on
by balanced forces. A force system acting on a body is said to be balanced if it
has no tendency to change the state of rest or motion of the body in any way. If
a body is in equilibrium, the force system acting on it must be balanced.
Furthermore, a body in a state of equilibrium must be either at rest or moving
along a straight path with a constant velocity. Most problems in Statics concern
bodies at rest.
The third part of mechanics, mechanics of fluids is concerned with liquids and
gases at rest or in motion.
FUNDAMENTAL CONCEPTS
Certain concepts and definitions are basic to the study of mechanics and they
should be understood at the outset.
The basic concepts in mechanics are space, time, mass and force. These concepts
cannot be truly defined. They should be accepted on the basis of our intuition and
experience, and used as a mental frame of reference for our study of mechanics.
In Newtonian mechanics, space, time and mass are absolute quantities, which
mean that they are independent of each other (this is not true in Relativistic
Mechanics, where the time of an event depends upon its position and the mass of
a body varies with its velocity) and cannot be defined in terms of other quantities
or in simpler terms. Force is a derived quantity.
Space: is the geometric region occupied by bodies whose positions are described
by linear or angular measurements relative to a specific coordinate system. For
three dimensional problems, three independent coordinates are needed. For two
dimensional problems only two coordinates will be required.
Time: is a concept for measuring the succession and the duration of events. Time
is not directly involved in the analysis of problems in Statics.
Mass: is a measure of the translational inertia of the body, which is its resistance
to a change in velocity. Mass can also be thought of as the quantity of matter in a
body. The mass of a body affects the gravitational attraction force between it
and other bodies.
The concept of mass is used to characterize and compare two bodies on the basis
of certain fundamental mechanical experiments depending on the definitions given
above. For example: 1) Two bodies of the same mass will be attracted by the
Earth in the same manner. 2) They will also offer the same resistance to a change
in translational motion.
Force: A force represents the action of one body on another. Force can be
generated either by the direct contact of bodies or by their effect at a distance.
Forces always occur in pairs. Forces of a pair are always equal in magnitude and
opposite in direction. Force is a vector quantity. The action of a force is
characterized by its magnitude, by the direction of its action and by its point of
application. A force tends to move a body in the direction of its action (the push –
pull effect of the force). In addition, a force tends to rotate the body about any
axis which does not intersect the line of action of the force and which is not
parallel to it (the moment effect of the force).
LAWS OF MECHANICS
3) Newton’s First Law: If the resultant force acting on a particle is zero, then
v v
the particle is in equilibrium. Stated mathematically as ( F = 0 ), where F is the
vector sum (the resultant) of all the forces acting on the particle.
4) Newton’s Second Law: The acceleration of a particle is proportional to the
resultant force acting on it and is in the direction of this force.
v v
F = ma
5) Newton’s Third Law: The forces of action and reaction between interacting
bodies are equal in magnitude, opposite in direction and collinear.
m1m2
F =G
r2
where,
“r” is the centroidal distance between the two particles
11 m3
“G” is the universal constant of gravitation equal to 6.673 × 10
kg s 2
A particular case of great importance is that of the attraction of the Earth on a
particle located at its surface. The force F exerted by the Earth on the particle
is then defined as the weight W of the particle.
W = mg
Where,
“m” s the mass of the particle
“g” is the gravitational acceleration of the Earth