Definition: Gravitation
"Every particle of matter in the universe attracts every other particle with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them. The direction of the force is along the line joining the particles."
or
The force by which the Earth attracts objects towards its centre is called gravitational force.
OR
The force of mutual attraction that any two objects in the universe exert on each other, which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres, is called the gravitational force.
Definition: Centripetal Force
Centripetal force is the force acting on a body moving in a circular path, in a direction towards the centre of the circular path.
OR
A force acts on any object moving along a circle and it is directed towards the centre of the circle. This is called the Centripetal force.
OR
The inward force required to keep an object moving in a circular path, directed towards the centre of the circle, expressed as FC = \[\frac {mv^2}{r}\] = mrω2, which always acts perpendicular to the direction of linear velocity, is called Centripetal Force.
Define Centripetal force.
At each of circular path, the particle, instead of moving straight continuously, turn towards the centre. Therefore, the motion in the circular path is under the action of a force called the centripetal force.
Definition: Universal Law of Gravitation
"Every particle of matter attracts every other particle of matter with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between them."
Definition: Angular Acceleration (α)
The rate of change of angular velocity of a body is called angular acceleration.
Definition: Radial (Centripetal) Acceleration
The component of acceleration directed towards the centre of the circular path is called centripetal acceleration (or radial acceleration).
Definition: Angular Displacement
The angle traced out by the radius vector at the centre of the circular path in a given time, expressed as Δθ = θ2 − θ1, is called angular displacement.
Definition: Angular Velocity (ω)
The rate of change of angular displacement of a body undergoing circular motion is called angular velocity.
Define Uniform circular motion.
When a particle moves with a constant speed in a circular path, its motion is said to be the uniform circular motion.
Angular velocity of a particle is the rate of change of angular displacement.
Definition: Uniform Circular Motion
When a particle moves with a constant speed in a circular path, its motion is said to be uniform circular motion.
OR
The motion of a body moving with constant speed along a circular path is called uniform circular motion.
OR
The motion of a body moving with constant speed along a circular path, where the velocity is always tangential to the circular path and remains constant in magnitude, is called uniform circular motion.
Definition: Centripetal Force
The force directed towards the centre along the radius, required to keep a body moving along a circular path at constant speed, is called centripetal force.
Definition: Acceleration Due to Gravity
The gravitational force due to the earth on a body results in its acceleration. This is called acceleration due to gravity and is denoted by ‘g’. Acceleration is a vector.
Definition: Weight
The weight of an object is defined as the force with which the earth attracts the object.
Definition: Mass
Mass is the amount of matter present in the object. The SI unit of mass is kg.
Define acceleration due to gravity.
The acceleration produced in a body due to the gravitational force of the earth is called the acceleration due to gravity.
Definition: Gravitational Potential
The gravitational potential energy per unit mass at a point is called gravitational potential.
OR
The negative of the work done by the gravitational force in displacing a unit mass from that point to infinity (or equivalently, the work done in bringing a unit mass from infinity to that point without acceleration) is called 'gravitational potential'.
Definition: Gravitational Potential Energy
The amount of work done in bringing a given body from infinity to that point against the gravitational force is called gravitational potential energy.
OR
The energy possessed by a system of two or more bodies by virtue of their positions and mutual gravitational attraction, which equals the work done against the gravitational force in assembling the system from infinity, is called 'gravitational potential energy'.
U = −\[\frac {Gm_1m_2}{r}\]
Definition: Potential Energy
"Potential energy is the work done against conservative force (or forces) in achieving a certain position or configuration of a given system."
OR
The energy stored in an object because of its position or state is called potential energy.
OR
The amount of work done against conservative forces which causes a change in P.E. is called potential energy.
Definition: Escape velocity
"The minimum velocity with which a body should be thrown vertically upwards from the surface of the Earth so that it escapes the Earth’s gravitational field is called the escape velocity (vₑ) of the body."
Formula: Centripetal Force
\[F_C=\frac{mv^2}{r}=mr\omega^2=mv\omega\quad(v=r\omega)\]
Formula: Kepler's Second Law
The area swept by the planet of mass m in a given interval Δt is:
\[\Delta\vec{A}=\frac{1}{2}(\vec{r}\times\vec{v}\Delta t)\]
- \[\vec r\]: Position vector of the planet (distance from Sun).
- \[\vec v\]: Velocity vector of the planet.
- Δt: Time interval.
- \[\vec p\]: Linear momentum (\[\vec p\] = m\[\vec v\])
- \[\vec L\]: Angular momentum (\[\vec L\] = \[\vec r\] × \[\vec p\])
Formula: Kepler's Third Law
Formula: Universal Law of Gravitation
The gravitational force of attraction (F) between two bodies of mass m1 and m2 separated by a distance r is:
\[\mathbf{F} = \mathbf{G}\frac{m_1 m_2}{r^2}\]
- F: Gravitational Force of attraction (in Newtons, N).
- \[m_1, m_2\]: Masses of the two objects (in kilograms, kg).
- r (or d in the first part): Distance between the two objects (in meters, m).
- G: The constant of proportionality, called the Universal gravitational constant.
- Value in SI units: \[G=6.67\times10^{-11}\mathrm{N}\cdot\mathrm{m}^2/\mathrm{kg}^2\]
- Dimensions: \[[G]=[\mathrm{L}^3\mathrm{M}^{-1}\mathrm{T}^{-2}]\]
Formula: Potential Energy
Based on the relationship between work and energy, the change in potential energy is given by:
\[\vec F\] · d\[\vec x\] = dU
- \[\vec{F}\]: The force acting on the object (external force applied against the conservative force).
- \[d\vec{x}\]: The small displacement of the object.
- dU: The change (increase) in the potential energy of the system.
Formula: Escape velocity
\[v_e=\sqrt{\frac{2GM}{R}}\]
- ve = Escape velocity (minimum speed needed to escape Earth’s gravity)
- G = Universal gravitational constant (6.674 × 10−11 Nm2/kg2)
- M = Mass of the Earth (or celestial body)
- R = Radius of the Earth (or distance from the centre of the mass to the object)
- Kepler’s first law: The orbit of a planet is an ellipse with the sun at one of the foci.
- Kepler’s second law: The line joining the planet and the sun sweeps equal areas in equal intervals of time.
- Kepler’s third law: The square of the orbital period of revolution of a planet around the Sun is directly proportional to the cube of the mean distance of the planet from the Sun.
Law: Kepler's First Law
Kepler's First Law (Law of Ellipses)
- Each planet moves in an elliptical orbit with the Sun at one focus.
- This means planetary orbits are stretched circles, not perfect circles.
- The ellipse has two foci; the Sun occupies one of these.
Law: Kepler's Second Law
Kepler's Second Law (Law of Equal Areas)
- A line joining the planet and the Sun sweeps out equal areas in equal time intervals.
- When the planet is nearer the Sun (perihelion), it moves faster.
- When the planet is farther from the Sun (aphelion), it moves more slowly.
- This law reflects conservation of angular momentum.
Law: Kepler's Third Law
Kepler's Third Law (Law of Periods)
- The square of the time period of revolution of a planet is proportional to the cube of the semi-major axis of its orbit.
- This means a planet farther from the Sun takes a longer time to complete an orbit.
Write the answer of the question with reference to laws of gravitation.
State the universal law of gravitation.
The universal law of gravitation states that every object in the universe attracts every other object with a force called the gravitational force. The force acting between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres.
F ∝ m M (masses of two bodies m and M)
F ∝ `1/"d"^2` (d is the distance between the two bodies.)

A and B are two bodies, the distance between which is given as d.
F = force with which one body is attracting the other.
G = proportionality constant.
Law: Universal Law of Gravitation
Statement:
The law which states that every particle of matter attracts every other particle in the universe with a force whose magnitude is directly proportional to the product of masses and inversely proportional to the square of the distance between them is called Newton's Law of Gravitation.
Derivation:
Newton's Universal Law of Gravitation states that every particle of matter attracts every other particle of matter with a force which is the following:
- Directly proportional to the product of their masses: F ∝ m₁ ⋅ m₂
- Inversely proportional to the square of the distance between them: F ∝ \[\frac {1}{r^2}\]
Combining both, the gravitational force is expressed as follows:
F = G\[\frac{m_1m_2}{r^2}\]
where G is the universal gravitational constant, measured by Henry Cavendish using the Cavendish balance, with the value:
G = 6.67 × 10⁻¹¹ Nm2/kg2