Working Through Examples
Let's tackle some real calculations to see how this works in practice. These examples show you exactly what examiners expect in your working.
For a minor planet with mass 2 × 10²² kg and radius 1200 km, we use g = GM/r². First convert the radius to metres (1,200,000 m), then substitute: g = (6.67 × 10⁻¹¹)(2 × 10²²)/(1.2 × 10⁶)² = 0.9 N/kg.
When comparing two stars with the same mass but different radii, you can use ratios. If star 2 has 10 times the radius of star 1, then g₂ = g₁r1/r2². So g₂ = 300(1/10)² = 3 N/kg.
The trickiest question involves showing that g = ⁴⁄₃πGρr for planets. Start with g = GM/r², substitute M = ρ × ⁴⁄₃πr³ (density times volume), and simplify. The r² cancels with one r from the volume term.
Exam Tip: Always convert units first - kilometres to metres is the most common mistake in gravitational field calculations!