Planets move on ellipses — the motion of the sky becomes a formula
Working from the positions of Mars that Tycho Brahe had recorded over some twenty years, Johannes Kepler showed that a planet moves on an ellipse with the Sun at one focus, travelling faster when it is closer to the Sun. He abandoned the assumption, held for nearly two thousand years, that heavenly bodies move in circles, because it disagreed slightly with the observations. In 1619 he added the relation between a planet's period and the size of its orbit (the third law). Every spacecraft trajectory calculated today still starts from these three laws.
- Shape of a planetary orbit circle → ellipse
People and institutions: Johannes Kepler / Tycho Brahe
NoteThe first and second laws appeared in Astronomia nova (1609); the third in Harmonices Mundi (1619).
- Astronomia nova, seu physica coelestis, tradita commentariis de motibus stellae Martis — Heidelberg: Voegelin (1609); digitized by ETH-Bibliothek Zürich, e-rara