Class IX · Chapter 9 Physics

CHAPTER 09

Gravitation

Universal Gravitation, Weight & Archimedes'

The same force that pulls an apple from a tree keeps the Moon in orbit — Newton's law of universal gravitation unifies Earth and sky.

\(F = Gm₁m₂/r² | g = 9.8 m/s² | W = mg\)
10 CBSE Marks
Difficulty
10 Topics
Very High Board Weight

Topics Covered

10 key topics in this chapter

Gravitation & Universal Law
Universal Gravitational Constant G
Free Fall & Acceleration due to Gravity g
Mass & Weight
Weight on Moon
Thrust & Pressure
Archimedes' Principle
Buoyancy & Upthrust
Relative Density
Applications of Archimedes'

Study Resources

Key Concepts

01. Universal Law of Gravitation

Every object in the universe attracts every other object with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them. F = Gm₁m₂/r². G = 6.674 × 10⁻¹¹ N·m²/kg².

02. Acceleration due to Gravity (g)

g = GM_Earth / R²Earth ≈ 9.8 m/s² at Earth's surface. g decreases as altitude increases (r increases). g on moon ≈ 1.63 m/s² (≈ g_Earth/6). Free fall: any object falling under gravity alone (ignoring air resistance).

03. Mass vs Weight

Mass (m) is the amount of matter — scalar, constant everywhere. Weight (W = mg) is the gravitational force on a body — vector, varies with g. An astronaut's mass is constant; weight changes on Moon or in space.

04. Thrust & Pressure

Thrust is the force acting perpendicular to a surface. Pressure = Thrust / Area (P = F/A). SI unit: Pascal (Pa = N/m²). Pressure depends on area — sharp knives cut better (small area → large pressure).

05. Archimedes' Principle

When a body is immersed in a fluid (partially or fully), it experiences an upward buoyant force equal to the weight of the fluid displaced. Buoyancy = weight of fluid displaced. This explains why ships float and hot air balloons rise.

06. Relative Density

Relative density = density of substance / density of water. If RD > 1, object sinks; RD < 1, object floats. RD of water = 1 (at 4 °C). RD has no unit (it is a ratio).

Formulas at a Glance

# Name Expression Notes
01 Gravitational Force F = Gm₁m₂/r² G = 6.674 × 10⁻¹¹ N·m²/kg²
02 g at surface g = GM/R² g on Earth ≈ 9.8 m/s²
03 Weight W = mg SI unit: Newton (N)
04 Pressure P = F/A SI unit: Pascal (Pa = N/m²)
05 Buoyant Force F_b = ρ_fluid × V_displaced × g Archimedes' principle
06 Relative Density RD = ρ_substance / ρ_water Dimensionless ratio

Important Notes

G (universal gravitational constant) is always 6.674 × 10⁻¹¹ N·m²/kg² — it does not change anywhere in the universe.
g varies: decreases at altitude, at poles g is slightly greater than equator (Earth is oblate), g on Moon is 1/6th of Earth.
An object in a satellite orbiting Earth is in free fall — it experiences weightlessness because both the satellite and the person inside fall at the same rate.
Archimedes'Principle: buoyant force = weight of fluid displaced — this is what makes a steel ship float (hollow → large displaced volume → large upthrust).

Exam Tips & Common Mistakes

1

Always state the universal law in words first, then give the formula F = Gm₁m₂/r² with all symbols defined.

2

"What is the weight of a body of mass 5 kg on Moon?" → W = m × g_moon = 5 × 1.63 ≈ 8.15 N. A standard 2-mark numerical.

3

Pressure: smaller area → higher pressure. Explain camel's feet (large area → low pressure on sand) as an example.

4

"Why does a boat float but an iron nail sink?" — boat has hollow shape displacing more water; weight < buoyancy. Iron nail is solid; weight > buoyancy.

5

Distinguish between G (constant, universal) and g (varies with location, acceleration). This distinction appears in 1-mark and 3-mark questions.

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