Class 9th- GRAVITATION (Prashant Kirad)
Introduction
Class: 9th
Topic: Gravitation
Presenter: Prashant Bhaiya
Overview of Gravitation
Covers key topics:
Universal Law of Gravitation
Free Fall
Value of g
Mass and Weight
Weight on the Moon
Thrust and Pressure
Buoyancy
Archimedes’ Principle
Historical Context
In 1666, Isaac Newton observed an apple fall, leading him to the concept of gravity.
Recognized gravity as a universal force acting on objects towards Earth and keeping planets in orbit.
Centripetal Force
Definition: Force that acts on an object moving in a circular path, directing it towards the center.
Example: Earth's gravity provides centripetal force that maintains the Moon's orbit.
Key aspect of circular motion is constant change in direction and velocity.
Definition of Gravitation
Gravitation: The force of attraction between any two bodies.
Examples:
Gravity causes a ball to fall to the ground.
Keeps planets in orbit around the Sun.
Causes disturbance in the motion of objects rolling downhill.
Newton’s Law of Gravitation
States that every object attracts every other object with a force:
Directly proportional to the product of their masses.
Inversely proportional to the square of the distance between them.
Gravitational Force Case Studies
Earth is affected by the Sun's gravity but does not fall into it due to its orbital velocity.
Equal and opposite forces exist between a stone and the Earth, yet only the stone visibly moves downward due to Earth's greater mass.
The force of gravitation doubles if the distance between two objects is halved.
Calculating Gravitational Force
Example Calculation:
If masses are 80 kg and 200 kg separated by 6m, apply Newton’s Law.
Importance of Universal Law of Gravitation
Fundamental to understanding:
Binding force keeping us on Earth.
The Moon's motion around Earth.
Earth’s motion around the Sun.
Relation to ocean tides influenced by the Moon.
Acceleration Due to Gravity (g)
Formula: g = G * (M/R²)
Defined variables:
G = gravitational constant (6.673 × 10⁻¹¹ Nm²/kg²)
M = mass of Earth (6 × 10²⁴ kg)
R = radius of Earth (6.37 × 10⁶ m)
Final calculated value: g ≈ 9.8 m/s²
Variation of g
Altitude: g decreases with greater height from Earth's surface.
Depth: g decreases deeper into the Earth due to mass distribution.
Latitude: g is highest at the poles (due to shape of Earth) and lowest at the equator.
Question on quicker drop at poles vs. equator due to variations in g.
Mass vs. Weight
Mass
Defined as the amount of matter, SI unit: kilogram (kg)
Scalar quantity, constant regardless of location.
Weight
Measure of gravitational force on an object, SI unit: Newton (N)
Vector quantity, varies with acceleration due to gravity.
On the Moon, weight is 1/6 of weight on Earth.
Differences between Mass and Weight
Mass:
Scalar, constant everywhere, measured in kg.
Does not change based on location.
Weight:
Vector, varies with gravity, measured in N.
Can be zero in free-fall or at Earth's center.
Weight on the Moon
Weight calculation using the universal law of gravitation.
Comparative calculation of weight on Moon vs. Earth, yielding approximately 1/6 of Earth’s weight.
Free Fall Definition
Motion of an object where gravity is the only force acting upon it, leading to acceleration downwards.
Motion Equations
Forms of motions affected by gravity:
First Equation: v = u + g*t
Second Equation: s = ut + 0.5gt²
Third Equation: v² = u² + 2gs
Characterization of Pressure
Definition: Thrust acting on a unit area, and its effect varies by contact area.
SI Unit: Pascal (Pa) or N/m².
Thrust and its Effects
Thrust's impact based on area of contact, illustrated in various scenarios (e.g., knife cutting, carrying heavy objects).
Thrust on loose sand vs. lying down: Larger contact area leads to less pressure.
Archimedes’ Principle
States the buoyant force on an object is equal to the weight of the fluid it displaces.
Applications in submarines, hot-air balloons and ships discussed.
Conclusion
Essential understanding of gravitation is foundational for recognizing its relevance across diverse physical phenomena.