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Johannes Kepler

German mathematician and astronomer (1571–1630) who, working from Tycho Brahe's unprecedentedly precise Mars observations, derived the three laws of planetary motion — orbits are ellipses with the Sun at one focus, equal areas are swept in equal time, and a planet's orbital period relates to its orbital distance by a fixed power law — replacing circle-and-equant astronomy with a dynamical account later shown (by Newton) to follow from gravity.

Matters to this vault as the figure whose own working papers and whose laws anchor a 2026 paper's central question: claim-astronomia-ova-orbit-family-satisfies-keplers-second-law-and-exact-equant asks whether an orbit can satisfy Kepler's second law exactly at one point while also having a true equant at another; claim-kepler-1609-astronomia-nova-rejected-puffy-cheeked-via-buccosa-oval-orbit records his own 1609 Astronomia Nova documenting the trial-and-error — including a near-elliptical "puffy-cheeked" orbit he explicitly rejected — on the way to the ellipse; claim-ptolemy-equant-mars-error-8-arcminutes-tycho-precision-forced-kepler-to-abandon-it records the specific Mars data that forced him to abandon Ptolemy's equant rather than reject it on philosophical grounds alone.

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