The Gregorian calendar: a 16th-century fix we still live inside
The Gregorian calendar, adopted in 1582 and adopted at different dates across the world (Britain in 1752, Greece in 1923, Saudi Arabia in 2016), is the civil calendar almost everywhere on Earth. Its design goals are worth restating because its quirks all follow from them: the year must stay aligned with the Sun's seasons, and the correction must be simple enough to apply by rule.
Its predecessor, the Julian calendar, used a strict every-four-years leap rule producing an average year of 365.25 days. The true tropical year is about 365.2422 days — a gap of roughly 11 minutes per year. Those minutes compound: about 3 days every 400 years. By the 16th century the spring equinox had drifted far enough from March 21 to destabilise the church's calculation of Easter, and the Gregorian correction arrived with its three-part rule (leap every 4 years, skip century years, restore every 400th).
The remaining discrepancy of ~0.0003 days per year means the Gregorian calendar still gains a day roughly every 3,236 years — a drift nobody alive will notice, and the reason proposals for a 4,000-year correction exist mostly as academic sport.
Structural details worth knowing when dates must line up:
- Months are deliberately unequal (28–31 days) because they descend from lunar months compressed by decree; quarter lengths are unequal too (90/91/92 days), so quarterly comparisons need day-count normalization.
- Weekday alignment drifts by one day per common year and two per leap year — which is why fixed-date holidays and anniversaries land on different weekdays over a 28-year cycle (the Meeus cycle).
- Day-of-year and week-number outputs inherit every one of these rules and must declare their starting convention to be reproducible.