Observing the comet from Denmark, Brahe noticed that its position in the sky differed very little from similar measurements performed by other astronomers across Europe. If the comet was something in the atmosphere, its apparent position should depend on which location it is viewed from. Seeing as this wasn’t the case, Brahe deduced that the comet must be at least four times farther than the Moon.
This started a new era of inquiry about comets, planets, and the fundamental physics that governs their motions. Galileo Galilei’s telescope observations and Johannes Kepler’s laws of planetary motion made it clear that not Earth, but the Sun lies at the centre of the Solar System. Isaac Newton published his universal theory of gravity in 1687, cementing this view in a firm theoretical foundation.
Soon after, Edmund Halley used Newton's theory to calculate the orbits for several comets – some of which he had observed during his lifetime, and many more that he had retrieved from ancient records. He deduced that the comet he had seen in 1682 was in fact the same one observed by others in 1607 and 1531. He predicted that this comet – now called Comet Halley in his honour – would appear again in 1758. Halley died before he could view it with his own eyes, but others were able to confirm his conjecture and, with it, that comets orbit the Sun just like planets do.