Every point mass attracts every other with a force along the line joining them, proportional to the product of masses and inversely proportional to the square of their distance.
Newton's law of universal gravitation
Related concepts
- Newtonian gravitational constant (G)
- Newton's second law (F=ma)
- Einstein field equations
- Einstein field equations
- Stellar structure equations
- Eddington luminosity
- N-body simulation
- Gravity anomaly
- Einstein field equations
- Einstein field equations
- Einstein field equations
- Restricted three-body problem
- Gravity anomalies & isostasy
- Kepler third law: T² = (4π²/GM)·a³ from two-body Hamiltonian
- Radial-velocity K ∝ m_p sin i / M_s^{2/3}: stellar Doppler wobble