Chapter 1 — Gravitation (Detailed, exam-ready notes)

Complete notes with derivations, worked examples, and formula sheet

1. Introduction & Key Ideas

Gravitation: Universal attractive force between every pair of masses. This fundamental force governs a wide range of phenomena from everyday experiences to cosmic events.

Key Applications

  • Responsible for weight and free fall of objects
  • Governs the motion of planets, moons, and stars
  • Causes ocean tides on Earth
  • Holds galaxies and the universe together
  • Main thinker: Sir Isaac Newton (Universal Law of Gravitation, 1687)

2. Newton's Universal Law of Gravitation

Statement: Every particle in the universe attracts every other particle 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.

Mathematical Form:

F = G(m₁m₂)/r²

Where:

  • F = gravitational force (in Newtons, N)
  • m₁, m₂ = masses of the two objects (in kilograms, kg)
  • r = distance between centers of mass (in meters, m)
  • G = universal gravitational constant = 6.674 × 10⁻¹¹ N·m²/kg²

Direction: The force acts along the line joining the centers of the two masses. It is always attractive and follows Newton's Third Law (equal and opposite).

3. Gravitational Field (Intensity) and Potential

Gravitational Field Strength (g)

The gravitational field strength at a point is defined as the force per unit mass experienced by a small test mass placed at that point.

Gravitational Field due to mass M at distance r:

g = F/m = GM/r²

(Units: N/kg or m/s²)

Gravitational Potential (V)

Gravitational potential at a point is the work done in bringing a unit mass from infinity to that point.

Gravitational Potential due to mass M at distance r:

V = -GM/r

(Units: J/kg)

The negative sign indicates that gravitational potential is always negative (work is done by the field).

4. Acceleration due to Gravity on Earth (g)

Standard near-surface value: g ≈ 9.8 m/s² (often approximated as 10 m/s² for calculations).

Relation with G and Earth:

g = GMₑ/Rₑ²

Where Mₑ = mass of Earth (5.97 × 10²⁴ kg), Rₑ = radius of Earth (6.37 × 10⁶ m)

Variation with Altitude (h)

At height h above Earth's surface:

gₕ = g(R/(R+h))²

Worked Example: g at 500 km altitude

Given: R = 6370 km, h = 500 km, g = 9.8 m/s²

gₕ = 9.8 × (6370/(6370+500))²

gₕ ≈ 9.8 × (6370/6870)² ≈ 9.8 × 0.860 ≈ 8.43 m/s²

Variation with Depth (d)

At depth d below Earth's surface (assuming uniform density):

g_d = g(1 - d/R)

Note: g decreases linearly with depth and becomes zero at Earth's center.

5. Free Fall & Equations of Motion

When an object falls under gravity alone (neglecting air resistance), it is in free fall. The acceleration is constant (g = 9.8 m/s²).

Kinematic Equations (Taking downward as positive)

1. v = u + gt

2. s = ut + ½gt²

3. v² = u² + 2gs

Where: u = initial velocity, v = final velocity, s = displacement, t = time

Worked Example: Stone dropped from 80m height

Given: Stone dropped (u = 0), s = 80 m, g = 9.8 m/s²

Find: Time to reach ground (t) and final velocity (v)

Solution:

1. Time: t = √(2s/g) = √(2×80/9.8) ≈ √(16.33) ≈ 4.04 s

2. Final velocity: v = gt ≈ 9.8 × 4.04 ≈ 39.6 m/s

6. Mass vs Weight

Property Mass (m) Weight (W)
Definition Amount of matter in a body Gravitational force on the body
SI Unit Kilogram (kg) Newton (N)
Nature Scalar (magnitude only) Vector (magnitude and direction)
Variation Constant everywhere Varies with location (g changes)
Measuring Device Beam balance, physical balance Spring balance
Relationship W = mg (Weight = mass × acceleration due to gravity)

7. Work, Energy & Orbits

Gravitational Potential Energy (U)

For mass m at distance r from mass M:

U = -GMm/r

The negative sign indicates bound systems; zero potential at infinity.

Orbital (Circular) Velocity (vₒ)

For a small mass m orbiting a large mass M at radius r:

Centripetal force = Gravitational force

mvₒ²/r = GMm/r²

vₒ = √(GM/r)

Escape Velocity (vₑ)

Minimum speed to escape gravitational field (reach infinity with zero velocity):

vₑ = √(2GM/r) = √2 × vₒ

Escape velocity is √2 times orbital velocity at the same point.

8. Satellites — Types & Important Facts

Artificial Satellite: Human-made object placed into orbit by rockets.

Satellite Applications

  • Communication: TV, radio, internet, telephone
  • Navigation: GPS, GLONASS, Galileo
  • Weather Monitoring: Storm tracking, climate data
  • Remote Sensing: Mapping, agriculture, disaster management
  • Scientific Research: Astronomy, Earth observation

Types of Orbits

Geostationary Orbit (GEO)

Altitude: ~35,786 km above Earth

Period: 24 hours (matches Earth's rotation)

Characteristics: Fixed above a point on equator; used for communication, broadcasting

Low Earth Orbit (LEO)

Altitude: 160-2,000 km above Earth

Period: 90-120 minutes

Characteristics: Used for imaging, ISS, Hubble telescope, some communication satellites

Escape Condition: If a satellite's speed ≥ escape velocity at that radius, it will leave Earth's gravitational field.

9. Pressure, Fluids and Buoyancy

Pressure (P)

P = Force (thrust) perpendicular / Area

SI Unit: Pascal (Pa) = N/m²

Archimedes' Principle (Buoyancy)

Statement: A body immersed in a fluid experiences an upward buoyant force equal to the weight of the fluid displaced.

Buoyant Force (F_b) = Weight of displaced fluid = ρVg

Where: ρ = density of fluid, V = volume of displaced fluid, g = acceleration due to gravity

Floating and Sinking Conditions

Worked Example: Buoyancy Problem

Given: Block volume = 0.02 m³, density = 800 kg/m³, Water density = 1000 kg/m³

Find: Will it float? If yes, what fraction is submerged?

Solution:

1. Mass of block = density × volume = 800 × 0.02 = 16 kg

2. Weight of block = mg = 16 × 9.8 ≈ 156.8 N

3. Buoyant force if fully immersed = ρ_water × V × g = 1000 × 0.02 × 9.8 = 196 N

4. Since 196 N > 156.8 N, the block floats

5. Fraction submerged = ρ_block/ρ_water = 800/1000 = 0.8 or 80%

10. Typical Board Numericals & How to Solve

Problem-Solving Strategies

  • 1. Find time of fall → Use s = ut + ½gt²
  • 2. Find velocity after time t → Use v = u + gt (if dropped, u=0)
  • 3. Gravity at altitude → Use gₕ = g(R/(R+h))²
  • 4. Escape/orbital velocity → Use vₑ = √(2GM/r), vₒ = √(GM/r)
  • 5. Buoyancy problems → Compare weight and buoyant force; for floating object: submerged fraction = ρ_object/ρ_fluid

11. Worked Numerical Summary (Important Results)

Quantity Formula Value (for Earth)
Escape Velocity vₑ = √(2GM/R) ≈ 11.18 km/s
Orbital Velocity at surface vₒ = √(GM/R) ≈ 7.91 km/s
g at 500 km altitude gₕ = g(R/(R+h))² ≈ 8.43 m/s²
Stone from 80 m height t = √(2s/g) t ≈ 4.04 s, v ≈ 39.6 m/s
Block buoyancy example Fraction submerged = ρ_block/ρ_water 80% submerged

12. Common Board Questions (with Answering Tips)

Answering Guidelines

Q1. State Newton's law of gravitation

Answer: Write the statement, formula (F = Gm₁m₂/r²), and explain all symbols with units.

Q2. Derive escape velocity

Answer: Equate kinetic energy (½mv²) to the gain in potential energy to reach infinity (GMm/R). Show steps clearly: ½mv² = GMm/R → v = √(2GM/R).

Q3. Explain Archimedes' principle

Answer: State the principle, give mathematical form (F_b = ρVg), and mention one application (ship design, hydrometers, submarines).

Q4. Why does g change with altitude?

Answer: Give formula gₕ = g(R/(R+h))² and explain: As altitude increases, distance from Earth's center increases, reducing gravitational force and thus g.

Q5. Compare mass & weight

Answer: Use a table format comparing definition, SI unit, nature, variation, and measuring device.

13. Quick Formula Sheet (One-Page Revision)

Gravitation Formula Sheet

Newton's Law

F = G(m₁m₂)/r²

G = 6.674×10⁻¹¹ N·m²/kg²

Gravitational Field

g = GM/r²

Units: N/kg or m/s²

Gravitational Potential

V = -GM/r

Units: J/kg

g at height h

gₕ = g(R/(R+h))²

g at depth d

g_d = g(1 - d/R)

Orbital Velocity

vₒ = √(GM/r)

Escape Velocity

vₑ = √(2GM/r)

vₑ = √2 × vₒ

Potential Energy

U = -GMm/r

Weight

W = mg

Buoyant Force

F_b = ρVg

ρ = fluid density

Free Fall

v = u + gt

s = ut + ½gt²

v² = u² + 2gs

Floating Condition

ρ_object/ρ_fluid

= Fraction submerged

14. Exam Tips & Presentation

Top Exam Preparation Tips

  • Start with clear definitions and formulas in every answer.
  • For numerical problems: Write given data, choose appropriate formula, show all calculation steps, give final answer with proper units.
  • Draw neat, labeled diagrams for orbits, free fall, buoyancy - even if not asked, it often earns extra marks.
  • Use tables for comparisons (mass vs weight, g vs G, different orbits).
  • Practice 6-8 numericals covering all types: free fall, g at height, orbital/escape velocities, buoyancy.
  • Memorize key values: G = 6.67×10⁻¹¹, g = 9.8 m/s², Earth radius = 6400 km, escape velocity = 11.2 km/s.
  • Time management: Allocate time based on marks; don't spend too long on one question.
  • Review common derivations: Escape velocity, variation of g with height/depth, orbital velocity.