Callippus (c. 370 BCE – c. 300 BCE) was a Greek astronomer and mathematician, remembered for refining the work of Meton of Athens and creating the Callippic Cycle — a more accurate system for reconciling the solar year with the lunar calendar. He worked in Athens alongside Eudoxus of Cnidus and later collaborated with Aristotle in the Lyceum, where his observations contributed to the understanding of celestial motion.
Born in Cyzicus, on the coast of Asia Minor (modern-day Turkey), Callippus traveled to Athens, where he joined Eudoxus and studied astronomy in detail. His careful observations of the Sun, Moon, and stars allowed him to detect small errors in existing astronomical cycles.
The Greeks faced a fundamental challenge: the lunar month (~29.53 days) does not divide evenly into the solar year (~365.24 days). To align the lunar and solar calendars, Meton (432 BCE) proposed the Metonic Cycle, where:
\[ 19 \text{ solar years } \approx 235 \text{ lunar months} \]
However, this approximation was slightly inaccurate, drifting by about 7 hours over 19 years.
Callippus refined this with his Callippic Cycle:
Thus, in Callippus’s system:
\[ 76 \text{ solar years } = 940 \text{ lunar months } = 27,759 \text{ days.} \]
This cycle was far more accurate and was used for centuries in Greek and later Babylonian astronomy.
Callippus also improved upon Eudoxus’s model of homocentric spheres, which attempted to describe planetary motion using concentric spheres.
This refinement helped Aristotle incorporate more accurate astronomical models into his philosophy of the cosmos.
Callippus of Cyzicus is remembered as a meticulous observer and practical mathematician who improved both astronomical modeling and calendar accuracy. By refining cycles of time and planetary motion, he helped bridge the gap between early Greek cosmology and the more systematic astronomy that followed.