Gravity near the Earth: the value of g · Physics Class 9–10 | StemPy Lab
Course 3.1·Lesson 2 of 3
Gravity near the Earth: the value of g
Near the Earth, every falling object has the same acceleration, g. We find its value from the law of gravitation.
about 20 min1 simulation2 practice questions1 Python program4 questions to check yourself
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The same acceleration for everything
Drop a heavy stone and a light one together: without air they land together. Every object near the Earth falls with the same acceleration, g.
Finding g
The Earth's pull on a mass m is F=R2GMm, and F=mg. So the m cancels:
g=R2GM
That is why every object falls the same way: g does not depend on the object's own mass.
The value of g
With M=6.0×1024kg and R=6.4×106m, g=9.8m/s2.
A bar chart of g on four bodies: the Moon 1.62, Mars 3.73, the Earth 9.81 and Jupiter 24.8 metres per second squared.
Does g change?
It is a little less at the equator than at the poles, because the Earth bulges.
It falls as you go up, because R becomes the distance from the centre.
Other worlds have other values: 1.6m/s2 on the Moon, about 25m/s2 on Jupiter.
You should find that g grows in step with the mass but falls with the square of the radius. A planet with twice the mass and 2 times the radius has the Earth's g.
Watch out.g (small, 9.8m/s2) is an acceleration. G (capital, 6.67×10−11N m2/kg2) is a constant. Do not mix them up.
A worked example
Find g on the Moon, Mars, the Earth and Jupiter from their masses and radii.
Moon. With G=6.67×10−11N m2/kg2, g=(1.74×106m)2G×7.35×1022kg=1.62m/s2.