Professor Sharon Kay Evanshine

History Web Site

Timeline of interesting calendar facts

Length of the tropical year, defined as the average interval between vernal equinoxes. This calendar year was the objective of the Gregorian calendar reform, which finalized the calendar as we use it today.

  

  

365 days, 5 hours, 49 minutes (365.2424 Universal days)

Lengthening of the vernal equinox year over the last two millennia

 

 

About 10 seconds
(0.0001 universal days per year)

Variation of this length in the next few millennia

 

 

less than 5 seconds

Lunar month in 2000 C.E.

 

 

29 days, 12 hours, 44 minutes, 2.9 seconds

The earliest known date

 

 

4236 B.C.E., the founding of the Egyptian calendar

Ancient Egyptian calendar year

 

 

365

Date Emperor Huangdi invented the Chinese calendar (legend)

 

 

2637 B.C.E.

Early Chinese year

 

 

354 days (lunar year) with days added at intervals to keep the Chinese lunar calendar aligned with the seasons

Early Greek year

 

 

354 days, with days added

Jewish Year

 

 

354 days, with days added

Early Roman year

 

 

304 days, amended in 700 C.E. to 355 days

The year according to Julius Caesar (The Julian calendar)

 

 

365 1/4 days

Date Caesar changed Roman year to Julian calendar

 

 

January 1, 45 B.C.E

Time the old Roman calendar was misaligned with the solar year as designated by Caesar

 

 

80 days

Total length of 45 B.C.E., known as the "Year of Confusion," after adding 80 days

 

 

445 days

Date Sanhedrin president Hillel II codified the Jewish calendar

 

 

ca. C.E. 359

The year as amended by Pope Gregory XIII (Gregorian calendar year)

 

 

365 days, 5 hours, 49 minutes, 12 seconds

Date Pope Gregory reformed the calendar

 

 

1582

Length of time the Julian calendar overestimates our calendar year per year, as determined by Pope Gregory

 

 

10 minutes 48 seconds

Days Pope Gregory removed to correct the calendar's drift

 

 

10 days

Dates Gregory eliminated by Papal bull to realign his calendar with the solar year

 

 

October 5-14, 1582

Dates most Catholic countries accepted the Gregorian calendar

 

 

1582-1584

Date Protestant Germany accepted the Gregorian calendar

 

 

partial acceptance in 1700, full acceptance in 1775

Date Great Britain (and the American colonies) accepted the Gregorian calendar

 

 

1752

Date Benjamin Franklin first proposed Daylight Saving Time

 

 

1784

Days eliminated by the British Parliament to realign the old calendar (Julian) with the Gregorian calendar

 

 

11 days

Dates Parliament eliminated

 

 

September 3-13, 1752

Date Japan accepted the Gregorian calendar

 

 

1873

Date Russia accepted the Gregorian calendar

 

 

1917 (and again in 1940)

Date China accepted the Gregorian calendar

 

 

1949

Date the Eastern Orthodox Church last voted to reject the Gregorian calendar and retain the Julian calendar

 

 

1971

Length of time the Gregorian calendar is off from the average vernal equinox year

 

 

about 12 seconds per year

Length of time the Gregorian calendar has become misaligned with the vernal equinox over the 414 years since Gregory's reform in 1582

 

 

1 hour and 20 minutes

When the Gregorian calendar will become twelve calendar hours ahead of the astronomer's mean tropical year

 

 

4th or 5th millennium C.E.

When the Gregorian calendar will become twelve calendar hours ahead of the mean vernal-equinox year

 

 

beyond the 7th millennium C.E.

Date Atomic Time replaced Earth Time as the world's official scientific time standard

 

 

1972

Current official definition of the second

 

 

time it takes for 9,192,631,770 oscillations of the Cesium atom at zero magnetic field

The mean vernal equinox year expressed in oscillations of atomic cesium at the year 2000

 

 

 

 

290,091,329,207,984,000

 

Notes:

  Slowing of the vernal equinox year

The length of the year has increased slightly over the millennia for a variety of reasons. These include: the gradual slowing of the Earth's rotation, slow changes in the Earth's orbit due to other planets and the moon, as well as regular effects due to precession of the Earth's axis of rotation every 26,000 years.

 

  Measures of the year

There is a subtle but important difference in two primary measures of the year, used by our calendar and by astronomers. The year mentioned above is the length of the tropical year defined as the mean interval between vernal equinoxes (1582-2000 C.E.) : 365 days, 5 hours, 49 minutes (365.2424 Universal days). Another measure of the year often used is the astronomer's mean tropical year, defined as 365 days, 5 hours, 48 minutes, 45 seconds.

 

  Atomic time

The measurement of time is currently determined by an international consortium based in France which averages the time from approximately 220 atomic clocks in over two dozen countries. The atomic clock is the only object that both tells time and generates a precise time scale.

 

Historically, the calculation of time has been based on the position of the earth relative to the sun using noon, when the sun is highest in the sky, as a marker. The length of the second, which corresponds to the length of time required for 9,192,631,770 cycles of the Cesium atom at zero magnetic field, was determined near the end of the 19th century; this second is thus equivalent to the second defined by the fraction 1/31 556 925.97 47 of the year 1900. In 1967, the official second was set as equal to an average second of Earth's rotation time; the calculation of the average is necessary due to the fact that the earth rotates at a slightly irregular rate.

 

Today, time is determined by counting official seconds. This is subject to slight measurement inaccuracies; thus, the international community calculates a stable time by averaging accumulated seconds from several clocks worldwide. Next, this figure is compared to a few highly accurate laboratory measurements of the second. Every month, the official world time is adjusted by a few nanoseconds. Politically, time is a cooperative venture; and, by making time an international endeavor, the international community benefits from the combined resources of many laboratories.