Mechanicsgraduate

Perihelion Precession of Mercury

Also known as: Anomalous perihelion advance · Relativistic perihelion precession · Mercury's 43 arcseconds

Relativity bends spacetime just enough that the orbit's closest point creeps forward each lap.

Δϕ=6πGMa(1e2)c2per orbit\Delta\phi = \frac{6\pi G M}{a\,(1-e^2)\,c^2} \quad \text{per orbit}
Live simulation
warming up the physics…

A planet on an eccentric orbit whose perihelion slowly advances, tracing a rosette of past ellipses. The red marker tracks the drifting closest point; sliders set eccentricity and an (exaggerated) precession rate.

Equivalent forms

Δϕ=24π3a2T2c2(1e2)\Delta\phi = \frac{24\pi^3 a^2}{T^2 c^2 (1-e^2)}
ϖ˙GR=43per century (Mercury)\dot{\varpi}_{\text{GR}} = 43''\,\text{per century (Mercury)}
A pure prediction with zero adjustable knobs reproduced a 56-year-old anomaly to the arcsecond — theory beating epicycle-style fixes.