+---------------------------------------------+-------------+-------------+ | | Sun’s Long. | Sun’s Anom. | | The year next less than 1757 in the Table +-------------+-------------+ | is 1753, at the beginning of which, the | s ° ʹ ʺ | s ° ʹ | | Sun’s mean Longitude from the beginning +-------------+-------------+ | of Aries, and his mean Anomaly, is | 9 10 16 52 | 6 1 38 | | To which add his mean Mot. and Anom. for | | | | four years to make 1757 | 0 0 1 49 | 11 29 58 | | { _April_ | 2 28 42 30 | 2 28 42 | | { days 29 | 0 28 35 2 | 0 28 35 | | And likewise his mean Mot. and { hours 22 | 0 54 13 | 0 54 | | Anom. for { min. 18 | 0 44 | 1 | | { sec. 49 | 2 | 0 | | | ----------- |-------------+ | Sun’s mean Longitude and Anomaly for the | | | | given time is | 1 8 31 12 | 9 29 48 | | To which add the Equation of the Sun’s | | | | mean Place | 1 40 14 +-------------+ | | ----------- | Sun’s Eq. | | And it gives his true Place, _viz._ | | 1° 40ʹ 14ʺ | | ♉ Taurus 10° 11ʹ 26ʺ | 1 10 11 26 | | +---------------------------------------------+-------------+-------------+ N. B. _In leap-years after_ February, _the Sun’s mean Motion and Anomaly must be taken out for the day next after the given one._ 361. _To calculate the Sun’s true Place for any time in a given year before the first year of_ CHRIST: subtract the mean Motions and Anomalies for the compleat hundreds next above the given year; to the remainder add those for the residue of years, months, _&c._ and then work in all respects as above taught. EXAMPLE. _To find the Suns true Place_ May _the 28th at 4 hours 3 min. 42 sec. in the afternoon, the year before Christ 585, which was a Leap year_[82].