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Acceleration due to gravity
Beginner
Near Earth's surface all objects fall with the same acceleration.
g ≈ 9.8 m/s²Near Earth's surface g ≈ 9.8 m/s² downward, varying slightly with latitude and altitude (9.78 at the equator, 9.83 at the poles). It is the same for all objects in free fall. On the Moon g ≈ 1.6 and on Jupiter ≈ 24.8 m/s².
On the Moon you could jump about six times higher with the same effort.
g is an acceleration, not a force; the weight is mg.
In more detail
The acceleration due to gravity, g, is about 9.8 m/s² at Earth's surface. It varies with height, latitude and local rock density.
How to solve it
- Write g = GM/R² for a spherical body, using its mass M and radius R.
- Insert the mass and radius in SI units, using scientific notation for both.
- Compute the result and compare it with the 9.8 m/s² value for Earth.
- For a height h above the surface, replace R with R + h, or use g = g0(R/(R + h))².
Worked examples
g = (6.67 × 10⁻¹¹)(7.35 × 10²²) / (1.74 × 10⁶)² = 4.90 × 10¹² / 3.03 × 10¹² = 1.62 m/s², about one-sixth of Earth's value.
g = g0 (R/(R + h))² = 9.8 × (6371/7371)² = 9.8 × 0.747 = 7.32 m/s².
Checking your answer
Gravity should be weaker on smaller or less massive bodies, and weaker farther from the centre. Both examples follow that pattern.
Real-world uses
- Pendulum clocks and gravimeters measure g to map underground structures.
- Engineers use the local value of g when designing lifts and cranes.
- Engineers use g to design structures such as lifts and cable cars, where gravity drives the loads on cables and supports.
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Frequently asked questions
Is g the same everywhere on Earth?
No. It is slightly larger at the poles than at the equator, and it decreases with altitude.
Is 9.8 m/s² exact?
It is a standard value, rounded for convenience. Precise measurements give slightly different values.
Why does g vary across Earth?
It is slightly larger at the poles than at the equator, and it decreases with altitude and depends on local rock density.
Related topics in Kinematics
Equations of motion: s = ut + ½at² · Equations of motion: v² = u² + 2as · Free fall · Vertical throw upward · Time of flight (vertical) · Relative velocity in 1D