More practice questions

  1. Q4. Treating the Earth as a uniform sphere, find the gravitational force on a 1 kg mass halfway to the centre, r = RE/2, in terms of its weight at the surface.

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    Inside a uniform Earth the force is proportional to r: F = GmMEr/RE3. At r = RE/2 it is half its surface value, mg/2, about 4.9 N for 1 kg.

  2. Q5. A planet has twice the Earth’s radius but only a quarter of its mean density. Find its surface gravity.

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    g = (4/3)πGρR is proportional to ρR, so the factor is ¼ × 2 = ½: about 4.9 m s.

  3. Q6. Jupiter has mass 1.90 × 10 kg and radius 6.99 × 10 m. Find g at its cloud tops. Take G = 6.67 × 10 N m kg.

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    GM is about 1.267 × 10 m s and R about 4.886 × 10 m, so g is about 25.9 m s, roughly 2.6 times the Earth’s.