Skip to main content
Admissions Open 2026-27Ravindra Higher Secondary School (Est. 1988) | Waidhan, Singrauli (MP)
+91 9826986106• Student Portal• Study Notes
Ravindra Higher Secondary School Logo
Ravindra Higher Secondary SchoolWaidhan, Singrauli (M.P.)
Home
Contact
Home
Study Portal
Class 9 Science
Gravitation - Universal law of gravitation, acceleration due to gravity, mass versus weight, and principles of buoyancy
Back to All Study GuidesOpen in Interactive App
ScienceClass 9Gravitation

Gravitation - Universal law of gravitation, acceleration due to gravity, mass versus weight, and principles of buoyancy

2026-09-0810 min readRHS Academic Faculty
Overview & Key Summary:Master Class 9 Science: Gravitation — Unlocking the Secrets of the Universe Have you ever wondered why an apple falls down from a tree instead of floating up into the sky? Why do...

Master Class 9 Science: Gravitation — Unlocking the Secrets of the Universe

Have you ever wondered why an apple falls down from a tree instead of floating up into the sky? Why doesn't the Moon drift away into deep space? Or why huge steel ships float effortlessly on water while a small iron nail sinks right to the bottom?

In this comprehensive tutorial, we will break down all these fascinating phenomena step-by-step!


Visualizing Core Gravitation Concepts

To help you build a clear mental model, let's look at how universal attraction, gravity, weight, and buoyancy interact in our physical world:


1. The Universal Law of Gravitation

In 1687, Sir Isaac Newton proposed a revolutionary idea: The force that makes an apple fall to the Earth is the exact same force that keeps the planets orbiting around the Sun.

What does the Law State?

Every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

Let's break this down algebraically:

  1. Consider two masses, MMM and mmm, separated by a distance ddd.
  2. The gravitational force FFF is directly proportional to the product of masses: F∝M×mF \propto M \times mF∝M×m
  3. The gravitational force FFF is inversely proportional to the square of the distance between them: F∝1d2F \propto \frac{1}{d^2}F∝d21​

Combining both statements: F∝M×md2F \propto \frac{M \times m}{d^2}F∝d2M×m​

To turn this proportion into an equation, we insert the Universal Gravitational Constant (GGG):

F=GM×md2F = G \frac{M \times m}{d^2}F=Gd2M×m​


Key Properties of GGG (Universal Gravitational Constant)

  • SI Unit: N⋅m2/kg2\text{N}\cdot\text{m}^2/\text{kg}^2N⋅m2/kg2
  • Accepted Value: G=6.673×10−11 N⋅m2/kg2G = 6.673 \times 10^{-11} \text{ N}\cdot\text{m}^2/\text{kg}^2G=6.673×10−11 N⋅m2/kg2 (calculated by Henry Cavendish).
  • Why "Universal"? Because its value remains constant everywhere in the universe—whether you are on Earth, Mars, or in deep space!

💡 Teacher's Analogy: Imagine invisible elastic bands connecting every particle in the cosmos. Heavy objects have extra-thick bands pulling strongly, but if you pull objects further apart, the tension weakens rapidly because of the inverse-square rule (d2d^2d2).


2. Acceleration Due to Gravity (ggg)

When an object falls towards the Earth solely under the influence of gravitational force, it is said to be in Free Fall.

During free fall, the direction of motion remains unchanged, but the speed increases every second. This change in velocity produces an acceleration called Acceleration due to Gravity, denoted by ggg.

Derivation of ggg

According to Newton's Second Law of Motion: Force (F)=mass (m)×acceleration (g)\text{Force } (F) = \text{mass } (m) \times \text{acceleration } (g)Force (F)=mass (m)×acceleration (g)

From the Universal Law of Gravitation: F=GMmR2F = \frac{G M m}{R^2}F=R2GMm​ (where MMM is the mass of Earth, mmm is the mass of the object, and RRR is the radius of Earth)

Equating both expressions for force: m⋅g=GMmR2m \cdot g = \frac{G M m}{R^2}m⋅g=R2GMm​

Canceling mmm from both sides:

g=GMR2g = \frac{G M}{R^2}g=R2GM​

Key Observations about ggg:

  1. Independent of Object's Mass: The value of ggg does not depend on the mass (mmm) of the falling body. A heavy stone and a light feather dropped in a vacuum will hit the ground at the exact same instant!
  2. Value on Earth Surface: Substituting G=6.67×10−11 N m2/kg2G = 6.67 \times 10^{-11} \text{ N m}^2/\text{kg}^2G=6.67×10−11 N m2/kg2, M=6×1024 kgM = 6 \times 10^{24} \text{ kg}M=6×1024 kg, and R=6.4×106 mR = 6.4 \times 10^6 \text{ m}R=6.4×106 m: g≈9.8 m/s2g \approx 9.8 \text{ m/s}^2g≈9.8 m/s2

Distinguishing GGG vs ggg

FeatureUniversal Gravitational Constant (GGG)Acceleration due to Gravity (ggg)
TypeScalar quantityVector quantity
ValueConstant (6.673×10−11 N m2/kg26.673 \times 10^{-11} \text{ N m}^2/\text{kg}^26.673×10−11 N m2/kg2)Variable (9.8 m/s29.8 \text{ m/s}^29.8 m/s2 on Earth's surface)
Location DependenceSame everywhere in the universeChanges from place to place (e.g., zero at Earth's center, lower at poles/equator)

3. Mass versus Weight

In everyday language, we often mix up mass and weight. But in Physics, they are completely different quantities!

                  MASS                                     WEIGHT
       [ Total matter contained ]              [ Force of gravitational pull ]
       • Measured in kilograms (kg)            • Measured in Newtons (N)
       • Scalar quantity (constant)            • Vector quantity (changes with g)

Detailed Comparison

  1. Mass (mmm):

    • The measure of inertia and quantity of matter contained in an object.
    • SI Unit: Kilogram (kg\text{kg}kg).
    • Constant everywhere (remains 50 kg50\text{ kg}50 kg on Earth, Moon, or Space).
  2. Weight (WWW):

    • The force with which an object is pulled towards Earth's center.
    • Formula: W=m×gW = m \times gW=m×g
    • SI Unit: Newton (N\text{N}N).
    • Variable because ggg varies.

Weight of an Object on the Moon

The Moon's mass is much smaller than Earth's. As a result, its gravitational attraction is weaker.

WMoon=16×WEarthW_{\text{Moon}} = \frac{1}{6} \times W_{\text{Earth}}WMoon​=61​×WEarth​

If you weigh 600 N600\text{ N}600 N on Earth, you will weigh only 100 N100\text{ N}100 N on the Moon!


4. Thrust, Pressure, and Principles of Buoyancy

Have you noticed why a sharp knife cuts vegetables effortlessly while a blunt knife fails? Or why camel feet are broad so they don't sink in desert sand?

Thrust and Pressure

  • Thrust: The net force acting perpendicular (at 90∘90^\circ90∘) to a surface. Unit: Newton (N\text{N}N).
  • Pressure: The thrust per unit area.

Pressure (P)=ThrustArea=FA\text{Pressure } (P) = \frac{\text{Thrust}}{\text{Area}} = \frac{F}{A}Pressure (P)=AreaThrust​=AF​

  • SI Unit: N/m2\text{N/m}^2N/m2 or Pascal (Pa\text{Pa}Pa).
  • Rule: For a fixed force, smaller surface area creates higher pressure!

Buoyancy and Upthrust

When an object is immersed in a liquid (water, oil, etc.), it experiences an upward force exerted by the fluid. This upward force is called Buoyant Force or Upthrust.

Why do objects float or sink?

  • Sinks: If the object's density is greater than the liquid's density (Weight of object > Upthrust).
  • Floats: If the object's density is less than or equal to the liquid's density (Upthrust ≥\ge≥ Weight of object).

Archimedes' Principle

When a body is immersed fully or partially in a fluid, it experiences an upward force that is equal to the weight of the fluid displaced by it.

Buoyant Force=Weight of Fluid Displaced\text{Buoyant Force} = \text{Weight of Fluid Displaced}Buoyant Force=Weight of Fluid Displaced

    [ Immersed Object ] ---> Displaces Fluid 
                                  │
                                  ▼
    Upward Buoyant Force = Weight of that Displaced Fluid

Applications of Archimedes' Principle:

  1. Designing ships and submarines.
  2. Lactometers (used to determine the purity of milk).
  3. Hydrometers (used to measure the density of liquids).

Guided Practice Questions with Detailed Solutions

Let's test our understanding with three classic numerical and conceptual problems step-by-step.


Question 1: Gravitational Force Calculation

Mass of Earth is 6×1024 kg6 \times 10^{24}\text{ kg}6×1024 kg and mass of the Moon is 7.4×1022 kg7.4 \times 10^{22}\text{ kg}7.4×1022 kg. If the distance between Earth and Moon is 3.84×105 km3.84 \times 10^5\text{ km}3.84×105 km, calculate the force exerted by Earth on the Moon. (Take G=6.7×10−11 N⋅m2/kg2G = 6.7 \times 10^{-11}\text{ N}\cdot\text{m}^2/\text{kg}^2G=6.7×10−11 N⋅m2/kg2)

Solution:

Step 1: Write down the given values in standard SI units.

  • Mass of Earth (MMM) = 6×1024 kg6 \times 10^{24}\text{ kg}6×1024 kg
  • Mass of Moon (mmm) = 7.4×1022 kg7.4 \times 10^{22}\text{ kg}7.4×1022 kg
  • Distance (ddd) = 3.84×105 km=3.84×108 m3.84 \times 10^5\text{ km} = 3.84 \times 10^8\text{ m}3.84×105 km=3.84×108 m
  • Gravitational Constant (GGG) = 6.7×10−11 N⋅m2/kg26.7 \times 10^{-11}\text{ N}\cdot\text{m}^2/\text{kg}^26.7×10−11 N⋅m2/kg2

Step 2: Apply Universal Law Formula. F=G⋅M⋅md2F = \frac{G \cdot M \cdot m}{d^2}F=d2G⋅M⋅m​

Step 3: Substitute values and calculate. F=6.7×10−11×6×1024×7.4×1022(3.84×108)2F = \frac{6.7 \times 10^{-11} \times 6 \times 10^{24} \times 7.4 \times 10^{22}}{(3.84 \times 10^8)^2}F=(3.84×108)26.7×10−11×6×1024×7.4×1022​

F=297.48×103514.7456×1016F = \frac{297.48 \times 10^{35}}{14.7456 \times 10^{16}}F=14.7456×1016297.48×1035​

F≈2.017×1020 NF \approx 2.017 \times 10^{20}\text{ N}F≈2.017×1020 N

Answer: The force exerted by the Earth on the Moon is 2.02×1020 N2.02 \times 10^{20}\text{ N}2.02×1020 N.


Question 2: Free-Fall Motion Equations

A ball is thrown vertically upwards and rises to a height of 20 m20\text{ m}20 m. Calculate:

  1. The velocity with which the object was thrown upwards.
  2. The total time taken by the object to reach the highest point. (Take g=9.8 m/s2g = 9.8\text{ m/s}^2g=9.8 m/s2)

Solution:

Step 1: Identify given conditions.

  • Final velocity (vvv) at highest point = 0 m/s0\text{ m/s}0 m/s
  • Distance/Height (sss) = 20 m20\text{ m}20 m
  • Acceleration (aaa) = −g=−9.8 m/s2-g = -9.8\text{ m/s}^2−g=−9.8 m/s2 (Negative because moving upwards against gravity)

Step 2: Solve part (1) using the third equation of motion (v2=u2+2asv^2 = u^2 + 2asv2=u2+2as). 02=u2+2(−9.8)(20)0^2 = u^2 + 2(-9.8)(20)02=u2+2(−9.8)(20) 0=u2−3920 = u^2 - 3920=u2−392 u2=392u^2 = 392u2=392 u=392≈19.8 m/su = \sqrt{392} \approx 19.8\text{ m/s}u=392​≈19.8 m/s

Step 3: Solve part (2) using the first equation of motion (v=u+atv = u + atv=u+at). 0=19.8+(−9.8)t0 = 19.8 + (-9.8)t0=19.8+(−9.8)t 9.8t=19.89.8t = 19.89.8t=19.8 t=19.89.8≈2.02 secondst = \frac{19.8}{9.8} \approx 2.02\text{ seconds}t=9.819.8​≈2.02 seconds

Answer:

  1. Initial throw velocity u=19.8 m/su = \mathbf{19.8\text{ m/s}}u=19.8 m/s
  2. Time taken to reach peak t=2.02 st = \mathbf{2.02\text{ s}}t=2.02 s

Question 3: Density, Buoyancy & Floating Condition

A sealed block of volume 500 cm3500\text{ cm}^3500 cm3 has a mass of 600 g600\text{ g}600 g. Will the block float or sink in water? (Density of water = 1 g/cm31\text{ g/cm}^31 g/cm3)

Solution:

Step 1: Formula for Density. Density=MassVolume\text{Density} = \frac{\text{Mass}}{\text{Volume}}Density=VolumeMass​

Step 2: Compute density of the block. Density of block=600 g500 cm3=1.2 g/cm3\text{Density of block} = \frac{600\text{ g}}{500\text{ cm}^3} = 1.2\text{ g/cm}^3Density of block=500 cm3600 g​=1.2 g/cm3

Step 3: Compare with liquid density.

  • Density of Block = 1.2 g/cm31.2\text{ g/cm}^31.2 g/cm3
  • Density of Water = 1.0 g/cm31.0\text{ g/cm}^31.0 g/cm3

Since the density of the block (1.2 g/cm31.2\text{ g/cm}^31.2 g/cm3) is greater than the density of water (1.0 g/cm31.0\text{ g/cm}^31.0 g/cm3), the gravitational force pulling it down exceeds the maximum upthrust force of the water.

Answer: The block will sink in water.


Chapter Summary Checklist

  • Universal Law: F=GMmd2F = G\frac{Mm}{d^2}F=Gd2Mm​ connects mass, distance, and gravity everywhere.
  • Gravity Acceleration: g=9.8 m/s2g = 9.8\text{ m/s}^2g=9.8 m/s2 at Earth's surface; independent of mass mmm.
  • Mass vs Weight: Mass (kg\text{kg}kg) stays fixed; Weight (N\text{N}N) changes with ggg.
  • Buoyancy: Objects float if their density is lower than the fluid's density due to net upward upthrust force.

Keep practicing your NCERT numericals, stay inquisitive, and keep reaching for the stars! Happy learning!

Common Student Mistakes to Avoid

  1. Confusing Key Terminology: Interchanging closely related scientific terms (e.g. mass vs. weight, reflection vs. refraction, or oxidation vs. reduction).
  2. Incomplete Chemical Equations or Formulas: Forgetting to balance chemical equations or omitting physical states (s, l, g, aq) in reaction steps.
  3. Diagram Labeling Errors: Drawing scientific diagrams without proper arrows showing light rays, electric current flow, or organ functions.
  4. Neglecting SI Units in Physics Problems: Calculating work, force, or energy without converting values into standard SI units first.

Exam Preparation & Frequently Asked Questions (FAQ)

Q1. How should I revise Gravitation for the Class 9 Science examination?

Focus on mastering core textbook definitions, practicing 3-4 numerical problems daily with pen and paper, and reviewing previous year CBSE/NCERT board exam questions.

Q2. What are the key concepts that carry maximum marks in this chapter?

Pay special attention to core definitions, step-by-step derivations, solved textbook examples, and practical real-world applications outlined in your NCERT curriculum.

Q3. How can I avoid losing marks in long answer questions?

Always structure your answers with clear subheadings, write step-by-step working for numerical problems, state given values clearly, and highlight your final answers with correct SI units.

Verified NCERT & Board Exam Aligned Material
Ravindra Higher Secondary School, Waidhan
Previous GuideSound - Production and propagation of sound, amplitude, frequency, pitch, and audible sound rangeNext GuideForce and Laws of Motion - Newton's three laws of motion, concept of inertia, momentum, and real-life applications

Related Study Notes

ScienceClass 9

Structure of the Atom

Structure of the Atom - Thomson and Rutherford atomic models, Bohr model of the atom, distribution of electrons in orbits, valency, atomic number, mass number, and isotopes

Read Article
ScienceClass 8

Friction

Friction - Types of friction including static, sliding, and rolling friction, factors affecting friction, and fluid friction

Read Article
ScienceClass 9

Atoms and Molecules

Atoms and Molecules - Laws of chemical combination, atomic and molecular mass, writing chemical formulae, and the mole concept

Read Article

NCERT Study Guide Directory

Textbook solutions, chapter notes & practice worksheets by grade

Interlinked Syllabus
Class 10 NCERT Guides14 chapters
  • Triangles
  • Circles
  • The Human Eye and the Colourful World
  • Carbon and its Compounds
  • Magnetic Effects of Electric Current
  • Arithmetic Progressions
  • Electricity
  • Light - Reflection and Refraction
  • Life Processes
  • Acids, Bases and Salts
  • Chemical Reactions and Equations
  • Introduction to Trigonometry
  • Quadratic Equations
  • Real Numbers
Class 9 NCERT Guides11 chapters
  • Structure of the Atom
  • Atoms and Molecules
  • Work and Energy
  • → Gravitation (Science)
  • Force and Laws of Motion
  • Motion
  • The Fundamental Unit of Life
  • Matter in Our Surroundings
  • Coordinate Geometry
  • Number Systems
  • Polynomials
Class 8 NCERT Guides11 chapters
  • Algebraic Expressions and Identities
  • Friction
  • Squares and Square Roots
  • Practical Geometry
  • Sound
  • Combustion and Flame
  • Coal and Petroleum
  • Microorganisms: Friend and Foe
  • Linear Equations in One Variable
  • Understanding Quadrilaterals
  • Rational Numbers
Class 7 NCERT Guides8 chapters
  • Acids, Bases and Salts
  • Heat
  • Nutrition in Animals
  • Nutrition in Plants
  • Perimeter and Area
  • Integers
  • Rational Numbers
  • Simple Equations
Class 6 NCERT Guides8 chapters
  • Algebra
  • Decimals
  • Fractions
  • Knowing Our Numbers
  • Electricity and Circuits
  • Components of Food
  • Getting to Know Plants
  • Separation of Substances
Ravindra Higher Secondary School Logo

Ravindra Higher Secondary School

Waidhan, Singrauli (M.P.)

We Serve Society By Serving People

Established in 1988, Ravindra Higher Secondary School (RHS Waidhan) is dedicated to delivering excellence in education, character building, and holistic growth for students in Waidhan, Singrauli (MP).

Quick Links

  • Home Page
  • About RHS & Leadership
  • Academic Programs & Curriculum
  • Admissions Process 2026-27
  • Campus & Facilities
  • Faculty & Staff Members
  • Photo & Video Gallery
  • Notice Board & Announcements
  • Contact & Location

Shift & Office Hours

KG to Class 5th (Morning Shift)

07:30 AM – 11:30 AM

Class 6th to 12th (Afternoon Shift)

12:00 PM – 05:00 PM

Administrative Office Hours

Mon – Sat: 09:00 AM – 04:00 PM

Address & Location

  • Ravindra Higher Secondary School, Main Campus, Waidhan, Singrauli, Madhya Pradesh – 486886
  • +91 9826986106
  • rhswaidhan@gmail.com

© 2026 Ravindra Higher Secondary School, Waidhan, Singrauli. All rights reserved.

Privacy Policy•Contact Us•Student Portal