Gravitational Field Strength (Edexcel A Level Physics)

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Gravitational Field Strength

  • There is a universal force of attraction between all matter with mass
    • This force is known as the ‘force due to gravity’ or the weight
  • The Earth’s gravitational field is responsible for the weight of all objects on Earth

12-2-weight-force_edexcel-al-physics-rn

The Earth's gravitational field produces an attractive force F, which is equal and opposite to the attractive force produced by the person's gravitational field

  • The gravitational field strength g at a point is defined as force F per unit mass m of an object at that point:

Gravitational Field Strength Equation_2

  • Where:
    • g = gravitational field strength (N kg1)
    • F = force due to gravity, or weight (N)
    • m = mass (kg)

 

  • This equation shows that:
    • The larger the mass of an object, the greater its pull on another mass
    • On planets with a large value of g, the gravitational force per unit mass is greater than on planets with a smaller value of g

  • An object's mass remains the same at all points in space
    • However, on planets such as Jupiter, the weight of an object will be a lot greater than on a less massive planet, such as Earth
    • This means the gravitational force would be so high that humans, for example, would not be able to fully stand up (or, even worse...)

gravitational field strength, downloadable AS & A Level Physics revision notes

The weight force on Jupiter would be so large that even standing upright would be difficult

  • Factors that affect the gravitational field strength at the surface of a planet are:
    • The radius (or diameter) of the planet
    • The mass (or density) of the planet

Worked example

Calculate the mass of an object with weight 10 N on Earth.

Examiner Tip

There is a big difference between g and G (sometimes referred to as ‘little g’ and ‘big G’ respectively).

  • g is the gravitational field strength, which varies depending on the size of the mass M producing the gravitational field and the distance r  from its centre of mass
  • G is Newton’s Universal Gravitational Constant, which always has a value of 6.67 × 10–11 N m2 kg–2

In addition, remember the equation density ρ = mass m ÷ volume V, which may come in handy with calculations where the density of some object is given, rather than its mass! 

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Katie M

Author: Katie M

Expertise: Physics

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.