Newton’s Law of Gravitation (DP IB Physics: SL)

• The gravitational force between two bodies outside a uniform field, e.g. between the Earth and the Sun, is defined by Newton’s Law of Gravitation
  • Recall that the mass of a uniform sphere can be considered to be a point mass at its centre

• Newton’s Law of Gravitation states that:

The gravitational force between two point masses is proportional to the product of the masses and inversely proportional to the square of their separation

• In equation form, this can be written as:

The gravitational force between two masses outside a uniform field is defined by Newton’s Law of Gravitation

• Where:
  • F= gravitational force between two masses (N)
  • G = Newton's Gravitational Constant
  • m and M = two points masses (kg) (These are sometimes labelled m₁ and m₂)
  • r = distance between the centre of the two masses (m)

• Although planets are not point masses, their separation is much larger than their radius
  • Therefore, Newton’s law of gravitation applies to planets orbiting the Sun

• The 1/r² relation is called the ‘inverse square law’
• This means that when a mass is twice as far away from another, its force due to gravity reduces by (½)² = ¼