Newton's Law of Gravitation (AQA A Level Physics) : Revision Note

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Katie M

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Newton's Law of Gravitation

  • 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

  • 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:

F space equals space fraction numerator G m subscript 1 m subscript 2 over denominator r squared end fraction

  • Where:

    • F = gravitational force between two masses (N)

    • G = Newton’s gravitational constant

    • m1 and m2 = two points masses (kg)

    • r = distance between the centre of the two masses (m)

Gravitational force between two point masses

Newton's law of gravitation, downloadable AS & A Level Physics revision notes

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

  • Newton’s law of gravitation applies to orbiting bodies, e.g. planets orbiting the Sun

  • Although stars and planets are very large, they can be considered to be point masses as:

    • they are approximately uniform spheres

    • their separation is much larger than their radii

  • The 1 over r squared relation is called the inverse square law

  • This means that when a mass is twice as far away from another, the gravitational force reduces by a quarter, i.e. open parentheses 1 half close parentheses squared space equals space 1 fourth

Worked Example

A satellite of mass 6500 kg is orbiting the Earth at 2000 km above the Earth's surface. The gravitational force between them is 37 kN.

Calculate the mass of the Earth.

Radius of the Earth = 6400 km.

Answer:

Step 1: List the known quantities

  • Mass of satellite, m1 = 6500 kg

    • m1 and m2 can be either way around

  • Distance of satellite above Earth's surface = 2000 km

  • Gravitational force, FG = 37 kN

  • Radius of Earth = 6400 km

Step 2: State the equation for Newton's Law of Gravitation and rearrange for the mass of the Earth

F subscript G space equals fraction numerator space G m subscript 1 m subscript 2 over denominator r squared end fraction

m subscript 2 space equals fraction numerator space r squared F subscript G over denominator G m subscript 1 end fraction

Step 3: Calculate the distance, r

  • r is the distance between the centre of the Earth and the satellite

  • r = distance of satellite above Earth's surface + radius of Earth

13-2-2-we-newtons-law-of-gravitation-answer--cie-new

r space equals space 2000 space plus space 6400 space equals space 8400 cross times 10 cubed space straight m

Step 4: Substitute the known values into Newton's Law of Gravitation to calculate the mass of the Earth

m subscript 2 space equals space fraction numerator open parentheses 8400 cross times 10 cubed close parentheses squared space cross times space open parentheses 37 cross times 10 cubed close parentheses over denominator open parentheses 6.67 cross times 10 to the power of negative 11 end exponent close parentheses space cross times space 6500 end fraction

m subscript 2 space equals space 6.0 cross times 10 to the power of 24 space end exponent kg space open parentheses 2 space straight s. straight f. close parentheses

Examiner Tips and Tricks

A common mistake in exams is to forget to add together the distance from the surface of the planet and its radius to obtain the value of r. The distance r is measured from the centre of the mass, which is from the centre of the planet.

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Katie M

Author: Katie M

Expertise: Physics Content Creator

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.