Seen through Galileo’s telescope, the moons of Jupiter appeared as mere points of light, indistinguishable from one another. Even so, they fomented an instant scientific revolution. Their existence gave evidence for what Copernicus had merely intuited: Not all heavenly bodies circle Earth.
The first morning’s session focused on the moons’ entry into 17th-century society. Although today we know these bodies—Io, Europa, Ganymede, and Callisto—as the Galilean satellites of Jupiter, Galileo himself wanted to call them the Cosmian Stars, in honor of his potential patron, Cosimo de’ Medici, the grand duke of Tuscany. Cosimo accepted the moons as a gift but preferred the name Medicean to describe them. Galileo of course complied, in a calculated move that won him a lifetime appointment as court mathematician and philosopher, plus generous Medici support for his research. I saw several scientists in the audience nod on that note, sympathetic with the time-honored need for government funding of big science.
After the initial discovery, Galileo faced the tougher job of studying and timing the moons’ regular orbits. He noted how they were periodically occulted by Jupiter or eclipsed in the planet’s shadow, and he applied these data to the practical problem of determining longitude at sea. (A navigator could compare the precise times at which these phenomena were observed from shipboard with the times they were predicted to occur if seen from a place of known longitude, such as Padua, then use the time difference to calculate his position east or west.) Although sailors never adopted Galileo’s technique, the moons proved a boon to cartography, helping to redraw land maps all over Europe.
Galileo’s successors followed the moons to other new conclusions about nature. Danish astronomer Ole Roemer, for example, watching the moons from the Paris Observatory, noted how their eclipses preceded the predicted times when Jupiter and Earth came nearest each other. Similarly, the moons’ eclipses fell minutes behind predicted times when Jupiter and Earth lay farthest apart. Roemer attributed these discrepancies to the time needed for light to travel across space from Jupiter to earthly observers. With the moons as his touchstone, he clocked the speed of light for the very first time, in 1676. His answer fell 25 percent below the modern value but greatly improved on the previous estimates of “infinite” and “immeasurable”…