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On the surface (or near it!) it's 9.81m per second squared. More generally it's; a=f/m1, and f=Gm1m2/r2 where; a = acceleration

f = force

m1 = mass 1 (ie falling body)

m2 = mass 2 (ie attracting planet)

G = gravitational constant = 6.67300 × 10-11 m3 kg-1 s-2

r2 = distance from centre of m2 to falling body (m1) squared (ir radius squared)

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17y ago

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