Hipparchus proposed a correction to the Calippic cycle, which itself was proposed as a correction to the Metonic cycle. He may have published it in the book "On the Length of the Year", which is lost. From solstice observations, Hipparchus found that the tropical year is about of a day shorter than the days that Calippus used. So he proposed to make a 1-day correction after 4 Calippic cycles, such that 304 years = 3760 lunations = 111035 days. This is a very decent approximation for an integer number of lunations in an integer number of days. But it is in fact 1.37 days longer than 304 tropical years: the mean tropical year is actually about day shorter than the Julian calendar year of days. These differences cannot be corrected with any cycle that is a multiple of the 19-year cycle of 235 lunations: it is an accumulation of the mismatch between years and months in the basic Metonic cycle, and the lunar monthsneed to be shifted systematically by a day with respect to the solar year after every 228 years. Indeed, from the values of the tropical year and the synodic month cited in the respective articles of Wikipedia, it follows that the length of 228=12*19 tropical years is about 83275.22 days, shorter than the length of 12*235 synodic months, namely about 83276.26 days, by one day plus about one hour. In fact, an even better correction would be to correcting by two days every 437 years, rather than one day every 228 years. The length of 437=23*19 tropical years, about 159610.837 days, is shorter than that of 23*235 synodic months, about 159612.833 days, by almost exactly two days, up to only six minutes. It corresponds to:
An eclipse cycle constructed by Hipparchus is described in Ptolemy's Almagest IV.2. Hipparchus constructed a cycle by multiplying by 17 a cycle due to the Chaldean astronomerKidinnu, so as to closely match an integer number of synodic months, anomalistic months, years, and days ; it is also close to a half-integer number of draconic months. By comparing his own eclipse observations with Babylonian records from 345 years earlier, he could verify the accuracy of the various periods that the Chaldean astronomers used. The Hipparchic eclipse cycle is made up of 25 inex minus 21 saros periods. There are only three or four eclipses in a series of eclipses separated by Hipparchic cycles. For example, the solar eclipse of August 21, 2017 was preceded by one in 1672 and will be followed by one in 2362, but there are none before or after these.
