MODULE:KNOWLEDGE-BASE
SIMULATION: ACTIVE
RETURN::Orbital Mechanics

Hill Sphere

The Region of Gravitational Dominance

Nested Spheres of Influence

The planet's Hill sphere (green) is where its gravity dominates over the star's. Inside, the moon orbits stably. The moon's own (much smaller) Hill sphere defines the region it dominates. Particles inside are captured; outside, they drift back to the star.

The Formula

r_H ≈ a · (m / 3M)^(1/3)

Where a is the body's semi-major axis around its parent, m is the body's mass, and M is the parent's mass.

The Hill radius is approximately the distance to the L1 and L2 Lagrange points of the body-parent system. Anything orbiting within that radius is gravitationally bound to the body; outside it, the parent dominates.

Stability Limits
Outer ~1/3 r_HPrograde moons stable on long timescales
Outer ~1/2 r_HRetrograde moons remain stable (less perturbed)
Beyond r_HBody drifts free — captured by parent instead
Eccentric orbitsEffective Hill radius shrinks with eccentricity

Earth's Moon orbits at ~26% of Earth's Hill radius — comfortably stable.

ED: Why Some Bodies Have No Moons

The Hill sphere explains a lot of what you see in the system map. Close-in planets have tiny Hill radii — they can't hold large moons against the star's tides.

Outer gas giants have enormous Hill spheres → huge moon collections (Jupiter has 95+, Saturn 100+). ED reflects this — gas giants in cold orbits often host the densest moon systems.

Tightly-bound stellar binaries share Hill spheres with each other. A planet around one star in a close binary lives in a small effective Hill region — explaining why S-type planets in tight binaries are rare.

Hill Spheres in the Solar System
BodyDistance from SunHill RadiusLargest Moon InsideNote
Mercury0.39 AU0.0012 AU (175,000 km)Tiny / none stableSun's tides destabilise even close moons
Venus0.72 AU0.0067 AU (1.0 M km)None observedCaptured moons would be unstable on long timescales
Earth1.0 AU0.010 AU (1.5 M km)Moon at 384,400 kmMoon orbits at ~26% of Hill radius
Mars1.52 AU0.0066 AU (985,000 km)Phobos & Deimos (very close)Both moons well inside Hill radius
Jupiter5.2 AU0.355 AU (53 M km)Callisto at 1.88 M kmHosts 95+ moons, mostly captured asteroids
Saturn9.5 AU0.435 AU (65 M km)Iapetus at 3.56 M kmWide Hill sphere → hundreds of small moons
Neptune30 AU0.77 AU (115 M km)Triton (retrograde capture)Far from Sun → enormous Hill sphere