Gravitational fields
| English | Chinese | Pinyin |
|---|---|---|
| gravitational field | 重力场 | zhòng lì chǎng |
| gravitational field strength | 重力场强度 | zhòng lì chǎng qiáng dù |
| field line | 场线 | chǎng xiàn |
| point mass | 质点 | zhì diǎn |
| radial | 径向 | jìng xiàng |
| uniform field | 匀强场 | yún qiáng chǎng |
The same pull, near and far
- An apple falls; the Moon circles the Earth. Both feel the same pull.
- A gravitational field 重力场 is any region where a mass feels a gravitational force.
- We measure its strength with one simple idea.
Field strength
- Gravitational field strength 重力场强度 is the force per unit mass: $g = \dfrac{F}{m}$.
- It is a vector, pointing toward the source mass.

Saturn, its rings and moons all held in orbit by gravity
Gravitational fields
g ∝ M / r²
Gravitational field strength obeys the inverse-square law — halve the distance and it quadruples.
Gravitational field strength is the force per unit:
$g = \dfrac{F}{m}$ — the gravitational force on each kilogram of a small test mass.
A familiar number
- The unit is $\dfrac{\text{N}}{\text{kg}}$ — exactly the same as $\dfrac{\text{m}}{\text{s}^2}$.
- So $g$ is just the acceleration of free fall in the field.
A $2.0\ \text{kg}$ mass feels a gravitational force of $20\ \text{N}$. What is $g$ there?
$g = \dfrac{F}{m} = \dfrac{20}{2.0} = 10\ \dfrac{\text{N}}{\text{kg}}$.
The unit N/kg is the same as m/s².
Yes — $g$ is also the acceleration of free fall, so its units are equivalent.
Field lines 场线
- Around a point mass 质点 or sphere: lines are radial 径向, pointing inward.
- Near a surface (small region): lines are parallel — a uniform field 匀强场. Closer lines = stronger field.

Around a sphere (seen from outside), the gravitational field lines are:
Gravity always attracts, so the lines point inward toward the centre, like a point mass.
Field lines drawn closer together represent a ____ field.
Line spacing shows strength — closer lines mean a stronger field.
You've got it
- gravitational field strength $g = \dfrac{F}{m}$ (a vector toward the mass)
- $\dfrac{\text{N}}{\text{kg}} = \dfrac{\text{m}}{\text{s}^2}$ — $g$ is the free-fall acceleration
- field lines: radial for a sphere, uniform near a surface; closer = stronger