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When to Use the Mercury Spin-Orbit Resonance 3D Explorer - Best Sessions and Limits


Open Mercury Spin-Orbit Resonance 3D Explorer when you want to see why Mercury settled into a 3:2 spin-orbit resonance instead of the simpler 1:1 tidal lock the Moon has with Earth, and how that alternates which hot pole faces the Sun - not to check a real ephemeris, a ground-track projection, or Mercury's true Kepler's-second-law speed near perihelion.


A before-1965-and-after lesson

A lesson starts by assuming the pre-1965 guess of a 1:1 tidal lock (one face always toward the Sun, like the Moon), then scrubs the day slider through one full 176-day solar day to show the two hot-pole markers swapping instead of staying fixed - the real consequence Pettengill and Dyce's 1965 radar observations first revealed and NASA's MESSENGER mission later confirmed.


Sessions this explorer does not fit

Sessions this page does not fit are checking a different planet's own retrograde, near-1:1 rotation lock - use the Venus Retrograde Rotation 3D Explorer for that - or exploring a general multi-body mean-motion resonance on its own terms - use the Orbital Resonance 3D Explorer. Walk the controls in the step-by-step guide.

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