Physics · Ch 6 — Gravitation
Universal Law of Gravitation
Universal Law of Gravitation
Kepler's laws described planetary motion perfectly but gave no reason why planets move that way. Newton supplied the reason: a single, universal force law.
The law itself. A particle of mass attracts any other particle of mass in the universe with a force that is directly proportional to the product of the two masses and inversely proportional to the square of the distance between them:
Here is the unit vector from towards , and is the universal gravitational constant. The negative sign is essential: it says the force on always points back toward , i.e. gravity is always attractive. By Newton's third law, -- the force feels from is equal and opposite to the force feels from .
Worked check (Example 6.1 style). Two masses and are apart. The force of attraction is
This is an extremely small force -- which is exactly why we never feel the gravitational attraction of ordinary nearby objects; only when one of the masses is planet-sized does the force become significant.
Important features.
- The force falls off as : double the separation and the force drops to a quarter. This is why Uranus, much farther from the Sun than Earth, feels a far weaker solar pull than Earth does.
- Gravitational forces always occur as action-reaction pairs: the Sun pulls the Earth toward itself, and the Earth pulls the Sun toward itself with an equal and opposite force.
- The formula strictly treats both masses as point masses. This is an excellent approximation whenever the separation is much larger than the sizes of the bodies (true for Sun-Earth). One special extended-body case does work out exactly like a point mass, though: a uniform hollow sphere of mass attracts an external point mass exactly as if all of were concentrated at the sphere's centre. And remarkably, a mass placed inside a hollow shell feels zero net force from the shell, from any position inside it (Figure 6.5) -- a result whose full proof is left to higher classes, but which becomes important later when we calculate at a depth below Earth's surface.
- The famous insight that "the falling apple and the orbiting Moon obey the same force" is the whole triumph of the law: comparing the apple's measured acceleration () against the Moon's centripetal acceleration (from its 27.3-day orbit at Earth radii) gives a ratio of almost exactly , precisely matching the inverse-square prediction . …
What this figure shows. Two point masses M1 and M2 are shown separated by a distance r, with a force arrow F drawn on M2 pointing toward M1. The unit vector r-hat is defined as pointing from M1 toward M2, and the force on M2 is written with a leading negative sign to show that the force always points opposite to r-hat, i.e. back toward the attracting mass -- gravity is always attractive, never repulsive, and always acts along the straight line j …
What this figure shows. Two companion diagrams. In the first, a point mass m sits outside a hollow spherical shell of mass M; the force it feels is exactly the same as if all of M were concentrated at the sphere's centre O. In the second diagram, a point mass m is placed inside the same hollow shell; the diagram shows that the net gravitational pull on it from every part of the shell cancels out perfectly, so the mass inside experiences precisely zero net force, no matter where inside the s …