Answers · The physics underneath
Why does a planet speed up when it gets closer to the Sun?
In shortA planet speeds up near the Sun because its fixed angular momentum forces its sideways speed up as its distance falls, and gravity does work as it falls inward.
A planet speeds up as it approaches the Sun because the product of its distance from the Sun and the sideways component of its speed is fixed, so a smaller distance forces a larger sideways speed. Gravity also does work on the planet as it falls inward, so the total speed rises even when the sideways component alone does not account for all of it.
The sideways part
Write the planet's position from the Sun as and its velocity as . The combination is large when the planet is moving across the line to the Sun and zero when it is moving straight at or away from the Sun. For a planet with sideways speed at distance , this reduces to , because the sideways velocity is times the rate at which the angle changes. A force aimed at the Sun has no sideways component at the planet's position, so it cannot change . If is fixed and is fixed, then is fixed. Halve and must double. The rate of turning, , goes as , so it rises by four when halves.
| point | distance | sideways speed | turn rate | kinetic energy |
|---|---|---|---|---|
| aphelion | 1 | 0.8 | 0.8 | 0.32 |
| perihelion | 0.5 | 1.6 | 3.2 | 1.28 |
The natural guess is that a pull toward the Sun should only produce motion toward the Sun. That guess treats the planet as starting from rest. It does not. The planet already has sideways motion, and the pull is at right angles to that sideways direction, so it bends the path without directly cancelling the circulation. What changes the sideways speed is not a sideways force; it is the shrinking of in the fixed product . If the Sun were switched off, the planet would fly in a straight line at constant speed. With the Sun on, the inward fall converts stored gravitational energy into kinetic energy, so the total speed rises, but the sideways part is forced up by geometry as well.
The pull does work too
Angular momentum alone does not give the whole speed at every point on an ellipse. It gives the sideways part. The radial part is set by energy. At the two ends of the orbit the radial speed is zero, so the total speed is the sideways speed, and the comparison is clean. Take an orbit with aphelion at and perihelion at , with and . At aphelion ; at perihelion . The kinetic energies are and . The difference is . Matching the two ends with a potential gives , so . The potential energies are and , and the totals are both . Gravity has done of work, which is exactly the rise in kinetic energy.
Where it stops
This stops being true if the force is not aimed at the Sun. A drag force, a rocket burn, or the sideways pull of another body can change . Then need not stay fixed, and the planet can speed up or slow down without the distance accounting for it. The point about which is measured also matters: is conserved about the Sun only because the force points there. Measured about some other point, the same force generally has a sideways component and changes. The inverse square law is not needed for the angular momentum argument; a spring or a constant central pull gives the same trade. What the inverse square law fixes is the shape of the orbit and the relation between speed and distance through energy.
The short statement to keep is that a central force cannot change circulation about its centre, and circulation is distance times sideways speed. That is why the closest part of an orbit is the fastest part, and why the equal-area law is the same fact written as area swept per unit time.
Worth keeping
- A force aimed at a point cannot change angular momentum about that point, whatever its strength law.
- For a planet, angular momentum is proportional to distance times sideways speed, so halving the distance doubles the sideways speed.
- The total speed also rises because gravity does work as the planet falls inward.
Where this goes next
This question is one step of Motion and What Is Conserved, a course that works through its subject from the beginning. The page that teaches this part of it is Going Round, and Staying Round, and it reads the whole way through whether or not you have an account.
What an account changes is the practice: problems standing under every idea, marked with a reason rather than a tick, in a copy of the course that is yours.
Read that pageThe whole courseOther questions people ask about this
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