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Newton's universal law of gravitation Formula, SPM Physics

Formula: F = G m₁m₂ / r². Not given in the exam, recall it.

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Newton's universal law of gravitation
F = G m₁m₂ / r²

Not given in the exam, recall it.

What it is for

Newton's universal law of gravitation is used in Gravitation (SPM Physics Form 4). Keep the SI units in every line of working. Gravitation

Symbols and SI units

SymbolMeaningSI unit
Fgravitational forceN
Ggravitational constantN m² kg⁻²
m₁mass of first objectkg
m₂mass of second objectkg
rdistance between centresm

Rearrangements

  • m₁ = Fr² / (G m₂)
  • r = √(G m₁m₂ / F)

Worked example

Two masses m₁ = 5 kg and m₂ = 10 kg are r = 2 m apart (G = 6.67 × 10⁻¹¹ N m² kg⁻²). F = G m₁m₂ / r² = (6.67 × 10⁻¹¹ × 5 × 10) / 2² = 8.34 × 10⁻¹⁰ N.

Common trap

r is the distance between the centres of the objects and it is squared. Use G = 6.67 × 10⁻¹¹ N m² kg⁻².

Understanding Newton's universal law of gravitation

Newton’s law states that every pair of masses attracts each other with a force F = G m₁m₂ / r².

Here F is the gravitational force in newtons (N), G is the gravitational constant, 6.67 × 10⁻¹¹ N m² kg⁻², m₁ and m₂ are the two masses in kilograms (kg), and r is the distance between their centres in metres (m). The force grows with either mass but falls off as the square of the distance, so doubling r quarters the force.

To find one mass, rearrange to m₁ = Fr² / (G m₂); to find the separation, use r = √(G m₁m₂ / F). The same pull acts on both masses, in opposite directions.

A worked example, step by step

Two dense spheres of mass m₁ = 1000 kg and m₂ = 2000 kg have their centres r = 5 m apart. Take G = 6.67 × 10⁻¹¹ N m² kg⁻².

Find the gravitational force between them.

Write the formula and substitute with units:

F = G m₁m₂ / r² = (6.67 × 10⁻¹¹ N m² kg⁻² × 1000 kg × 2000 kg) / (5 m)²

F = (1.334 × 10⁻⁴) / 25 = 5.34 × 10⁻⁶ N.

The force is tiny even for tonnes of mass a few metres apart, which is why gravitation between everyday objects is never noticed. The answer is quoted to three significant figures with the newton.

Common mistakes and how this is tested

The most important rule is that r is the distance between the centres of the objects and it must be squared; forgetting the square is the classic error.

Other mistakes: dropping the constant G or misreading its power of ten (6.67 × 10⁻¹¹); measuring r from the surfaces instead of the centres; and mishandling standard form when multiplying the small and large numbers.

This is tested under define (state the law in words), calculate (find F, a mass, or r), and explain (why the force weakens rapidly with distance, or why we do not feel the pull between two people).

Source: DSKP KSSM Physics Form 4 and 5 (Versi English), Sijil Pelajaran Malaysia: Format Pentaksiran mulai 2021, Fizik (4531) (Bahagian Pembangunan Kurikulum (BPK), KPM)

Written by the spmphysics.com.my editorial team.· Updated 5 Sept 2026

Frequently asked questions

Is this formula given in the exam?
No. SPM Physics papers provide no formula sheet, so this must be recalled.
Why is the gravitational force between everyday objects so small?
Because the constant G is extremely small (6.67 × 10⁻¹¹). Even for masses of hundreds of kilograms a few metres apart, the force comes out to only a few micronewtons, far too weak to feel.
Is r measured from the surface or the centre?
From the centre of each object. For a planet that means the radius plus any altitude, not the height above the surface alone. Then r must be squared in the formula.
What happens to the force if the distance doubles?
The force becomes one quarter of its original value, because F is inversely proportional to r². Tripling the distance makes it one ninth.

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