College Physics II – Mechanics, Sound, Oscillations, and Waves
Definition
Aphelion is the point in the orbit of a planet, asteroid, or comet at which it is farthest from the Sun. This term contrasts with perihelion, the point in the orbit where the object is closest to the Sun.
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Aphelion occurs because planetary orbits are elliptical, as described by Kepler's First Law.
At aphelion, a planet's orbital speed is at its minimum due to being furthest from the Sun’s gravitational pull.
The Earth reaches its aphelion around early July each year.
Kepler's Second Law states that a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time; thus, planets move slower at aphelion compared to perihelion.
The difference in distance between aphelion and perihelion affects seasonal variations for planets with significant axial tilt.
Review Questions
What happens to a planet's orbital speed when it reaches aphelion?
How does Kepler's Second Law explain planetary motion at aphelion?