A gravitational field is a region around a mass where another mass feels a force.
The field is described by the vector field \$\mathbf{g}\$:
\$\mathbf{g} = -\,G\,\frac{M}{r^{2}}\;\hat{\mathbf{r}}\$
where \$G\$ is the gravitational constant, \$M\$ the source mass, \$r\$ the distance, and \$\hat{\mathbf{r}}\$ the radial unit vector pointing away from the source.
Think of the field like invisible “gravity waves” that spread out from every mass.
🔍 Analogy: Imagine a crowd of people walking toward a stadium. The crowd density is higher near the stadium entrance – that’s like field line density.
💡 Tip: Use a ruler or a straightedge to keep lines straight and evenly spaced.
For a single spherical mass, field lines are radial and evenly spaced.
The field strength at a distance \$r\$ is:
\$|\mathbf{g}| = G\,\frac{M}{r^{2}}\$
🪐 Visual: Imagine a set of concentric circles around Earth, each circle representing a constant field strength.
Field lines start at infinity, bend toward each mass, and converge at the centre of mass.
Between the masses, lines are denser, showing a stronger combined field.
⚖️ Analogy: Two magnets pulling a metal ball toward the middle.
??
Remember: Clear, neat drawings with consistent spacing score higher.
| Property | Field Line Feature |
|---|---|
| Direction | Toward the mass |
| Density | Higher where field is stronger |
| Crossing | Never cross |
| Start/End | From infinity to the mass |