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Mechanics is the branch of physics concerned with the state of rest or motion of bodies subjected to the action of forces. It explains how and why bodies move or remain at rest when acted upon by forces.
Many scientists contributed to the development of mechanics: Archimedes (287-212 BC), Galileo (1564-1642), Sir Isaac Newton (1642-1727), Einstein (1878-1955), and others including Varignon, Euler and D'Alembert.
Mechanics may be grouped broadly as:
Sir Isaac Newton consolidated laws and experimental findings on motion and rest and stated the three laws of motion and the law of universal gravitation; mechanics based on these is called Classical (Newtonian) mechanics.
Albert Einstein showed that Newtonian mechanics does not correctly describe bodies moving at speeds near the speed of light and proposed Relativistic mechanics.
Schrödinger and de Broglie showed that Newtonian mechanics fails at atomic scales and proposed Quantum mechanics.
Definition: A rigid body is an idealised body in which the relative positions of any two particles remain unchanged under the action of forces. Equivalently, the distance between any two points in a rigid body remains the same before and after applying external forces.
In practice, physical bodies deform slightly when loaded. If that deformation is negligible compared to the body's size for the problem under consideration, the body is treated as rigid.
| Note : Physical bodies deform slightly under loads. If deformation is negligible compared to size, the body is termed rigid. Rigid body mechanics assumes bodies are rigid. |
Force is any action that tends to change the state of rest or motion of a body. A force is a vector quantity; its SI unit is the Newton (N).
Three quantities required to fully specify a force are:
The line of action of a force is the straight line passing through the point of application in the direction of the force; it determines the direction along which the force tends to move the body.
A force may be represented graphically by a directed line segment whose length is proportional to the magnitude and whose orientation gives the direction. The point where the segment meets the body is the point of application.
The fundamental laws used in rigid body mechanics include:
First law (Law of Inertia): A particle remains at rest or continues to move with uniform velocity unless acted upon by an unbalanced external force.
Second law: The rate of change of momentum of a body is directly proportional to the applied force and takes place in the direction of the applied force.
For a constant-mass body this gives the familiar form: F = ma, where F is the vector sum of forces, m is mass and a is acceleration.
Third law: To every action there is an equal and opposite reaction; the mutual forces of action and reaction between two bodies are equal in magnitude, opposite in direction and collinear.
Any two point masses attract each other with a force directed along the line joining them. The magnitude of the force is directly proportional to the product of the masses and inversely proportional to the square of the distance between them:
F = G m1 m2 / r², where G is the gravitational constant, m1 and m2 are the masses, and r is the separation.
Triangular law of forces: If two forces acting on a body are represented in magnitude and direction by two sides of a triangle taken in order, then the third side (closing side) of the triangle taken in the opposite order represents the resultant in magnitude and direction.
Polygon law of forces: If several concurrent forces acting on a body are represented in magnitude and direction by the sides of a polygon taken in order, then their resultant is represented by the closing side of the polygon taken in the reverse order.
The principle of transmissibility states that the external effect of a force on a rigid body is the same if the force is applied at any other point on the same line of action. In other words, a force can be moved along its line of action without changing the external effect on a rigid body.
Note: This principle does not hold if deformation of the body is significant for the problem.
| Examples Fig : Rigid Bodies (valid) Fig : Deformable Bodies (not valid) Note : In engineering mechanics we deal with rigid bodies. If deformation is considered in a problem, the law of transmissibility will not be valid. |
If two forces acting at a point are represented in magnitude and direction by the two adjacent sides of a parallelogram, then their resultant is represented in magnitude and direction by the diagonal of the parallelogram passing through the point.
Given OA = P and OB = Q represented as vector segments. Construct parallelogram OBCA. Drop perpendicular CD on extension of OA.
From the geometry,
AD = Q cos θ
CD = Q sin θ
Using right triangle relationships, the magnitude of resultant R is found by combining components of P and Q and gives the same result as the diagonal of the parallelogram.
Note : The parallelogram law is valid for all vectors and thus for forces.
A force system is when several forces of different magnitudes and directions act on a body or particle. The resultant and the net effect of the system depend on their magnitudes, directions and points of application.
Collinear forces act along the same straight line.
Coplanar force system: All forces lie in the same plane.
Non-coplanar force system: Forces do not lie in a single common plane.
Concurrent forces are forces whose lines of action meet at a common point. They may be coplanar or non-coplanar.
Non-concurrent forces have lines of action that do not all meet at a single point.
Forces with lines of action parallel to one another form a parallel force system. They are classified as:
To analyse a rigid body under several forces, we find the resultant force and the resultant moment. For a rigid body to be in equilibrium, the following conditions must be satisfied:
For three-dimensional problems the vector form of equilibrium is used: ΣF = 0 and ΣM = 0 (vector equations).
Moment (or torque) of a force about a point is the tendency of the force to cause rotation about that point. For a force F with position vector r, the moment is the vector cross-product M = r × F.
A couple consists of two equal, parallel and opposite forces whose lines of action do not coincide; a couple produces pure rotation and its moment is free vector (independent of the reference point).
Centre of mass of a rigid body is the point at which the entire mass may be considered to be concentrated for the purpose of translational motion analysis. For discrete masses, the coordinates of the centre of mass are given by the weighted average of particle positions. For continuous bodies, integrals over the mass distribution are used.
Centroid is the geometric centre of an area or volume and is used when the area or volume has uniform density; for uniform thickness bodies centroid and centre of mass coincide.
Mass moment of inertia (for dynamics) is a scalar or tensor quantity that measures a body's resistance to angular acceleration about an axis. For a rigid body rotating about a fixed axis, the kinetic energy and dynamics depend on the mass moment of inertia.
Second moment of area (often called area moment of inertia) is used in strength of materials to relate bending stress and deflection of beams.
To apply equilibrium equations, first draw a free body diagram: isolate the body or part, show all external forces and moments, including reactions at supports, weights, and applied loads. Indicate coordinate axes and the points about which moments are taken.
Consider a beam supported at two ends with a central load. The procedure to find support reactions is:
Final summary: Rigid body mechanics provides the foundations to analyse forces, moments and equilibrium for bodies idealised as non-deformable. Statics determines load distributions and reactions under equilibrium; dynamics links forces to motion. Understanding force systems, resultants, moments, free body diagrams, and equilibrium equations is essential for engineering analysis and design.
24 videos|67 docs|53 tests |
| 1. What is a rigid body? | ![]() |
| 2. How is the motion of a rigid body described? | ![]() |
| 3. What are the conditions for a body to be considered a rigid body? | ![]() |
| 4. What are some real-life examples of rigid bodies? | ![]() |
| 5. Can a rigid body have internal forces? | ![]() |