Mr Toogood's Physics · Gravitational fields
Faraday's iron filings experiment — one of the earliest ways fields were made visible.
A field is a region of space where an object experiences a non-contact force. First introduced by Michael Faraday to explain forces like electricity and magnetism acting at a distance. Fields are considered physically real — they carry energy and momentum, and propagate at a finite speed (light from the Sun takes ~8 minutes to reach Earth via the electromagnetic field), evidenced directly by effects like radiation pressure.
A radial field around a point mass — field strength falls off as lines spread out.
Fields are vectors — always a size and a direction. Direction is defined as the direction a positive test object would accelerate.
Radial: strength falls with distance. Parallel: strength stays constant.
| Source | Field | Notes |
|---|---|---|
| Mass | Gravitational | Always attractive |
| Static charge | Electric | Attract or repel (±) |
| Moving charge | Magnetic | Stationary charge → none |
| Concept | Gravitational | Electrostatic |
|---|---|---|
| Force per... | unit mass (N kg⁻¹) | unit charge (N C⁻¹) |
| Inverse square | F∝1/r² (Newton) | F∝1/r² (Coulomb) |
| Attract/repel | Always attracts | Either, by sign |
Discovered a century apart (Newton, 1687; Coulomb, 1785), yet both follow an identical inverse-square mathematical form — part of what makes fields such a powerful unifying idea.
The two also differ enormously in strength: in a hydrogen atom, the electrostatic force between the proton and electron is around 10³⁹ times stronger than the gravitational force between them — vast enough that gravity is simply ignored in atomic and particle physics.