Physics lab · mechanics · oscillation + gravitation

Hooke’s law &
orbital motion

Stretch the spring: it pulls back with F = −kx, and damping bleeds the energy away. Fling the planet: gravity bends it into an ellipse — Kepler’s laws, live. Every number is computed, softly lit.

Hooke’s law says the restoring force of a spring is F = −kx. The stretch x is how far the mass sits from its rest point, k is the stiffness, and the minus sign means the force points back toward rest. Gravity pulls a planet toward the sun with F = GMm/r², and a sideways speed turns that fall into an ellipse.

In the world

An automotive suspension engineer chooses the stiffness k so a car settles a comfortable amount under the passengers and still presses the tires back onto the road after a bump. A product engineer sets the stiffness of a bathroom or kitchen scale so a known stretch matches a known weight. A satellite engineer sets a satellite’s height and speed together, because a larger orbit needs a longer period. GPS satellites orbit about 20,200 km above Earth and take about 12 hours to go around once.

Common mistakes

  • The minus sign in F = −kx is a direction. It means the pull points back toward rest, not that the spring is weaker.
  • A heavier mass does not change k. The same spring stretches farther at rest, Δ = mg/k, and it swings with a longer period.
  • Speeding a planet up does not always make a bigger closed orbit. Past escape speed, the path does not come back.
  • Kepler’s third law keeps T²/a³ the same for one sun. A longer period and a larger orbit change together, and the ratio does not.

Lesson 1/9 · Hooke’s law

pull the mass to stretch the spring · release
fling a planet · new speed → new orbit · drag empty space to lean

Hooke’s law · F = −kx − cv

spring constant k—
mass m—
damping c—
damping ratio ζ—
period T = 2π/ωd—
displacement x—

Gravity · F = GMm/r²

GM (central mass)—
semi-major axis a—
eccentricity e—
period T = 2π√(a³/GM)—
r · speed v—
g = GM/r²—
Kepler III T²/a³—