Julian day number

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The Julian date (JD) is the interval of time in days and fractions of a day since January 1, 4713 BC Greenwich noon, Julian proleptic calendar.^[1] In precise work, the timescale, e.g., Terrestrial Time (TT) or Universal Time (UT), should be specified.^[2]

The Julian day number (JDN)^[3] is the integral part of the Julian date (JD).^[4] The day commencing at the above-mentioned epoch is JDN 0. Negative values can be used for preceding dates, though they predate all recorded history. Now, at 21:39, Saturday January 2, 2010 (UTC) the Julian day number is 2455199.

A Julian date of 2454115.05486 means that the date and Universal Time is Sunday January 14, 2007 at 13:18:59.9.

The decimal parts of a Julian date:
0.1 = 2.4 hours or 144 minutes or 8640 seconds
0.01 = 0.24 hours or 14.4 minutes or 864 seconds
0.001 = 0.024 hours or 1.44 minutes or 86.4 seconds
0.0001 = 0.0024 hours or 0.144 minutes or 8.64 seconds
0.00001 = 0.00024 hours or 0.0144 minutes or 0.864 seconds.

Almost 2.5 million Julian days have elapsed since the initial epoch. JDN 2,400,000 was November 16, 1858. JD 2,500,000.0 will occur on August 31, 2132 at noon UT.

If the Julian date of noon is applied to the entire midnight-to-midnight civil day centered on that noon,^[5] rounding Julian dates (fractional days) for the twelve hours before noon up while rounding those after noon down, then the remainder upon division by 7 represents the day of the week, with 0 representing Monday, 1 representing Tuesday, and so forth. Now at 21:39, Saturday January 2, 2010 (UTC) the nearest noon JDN is 2455199 yielding a remainder of 5.

The Julian day number can be considered a very simple calendar, where its calendar date is just an integer. This is useful for reference, computations, and conversions. It allows the time between any two dates in history to be computed by simple subtraction.

The Julian day system was introduced by astronomers to provide a single system of dates that could be used when working with different calendars and to unify different historical chronologies. Apart from the choice of the zero point and name, this Julian day and Julian date are not directly related to the Julian calendar, although it is possible to convert any date from one calendar to the other.

Julian Date

Historical Julian dates were recorded relative to GMT or Ephemeris Time, but the International Astronomical Union now recommends that Julian Dates be specified in Terrestrial Time, and that when necessary to specify Julian Dates using a different time scale, that the time scale used be indicated when required, such as JD(UT1). The fraction of the day is found by converting the number of hours, minutes, and seconds after noon into the equivalent decimal fraction.

The term Julian date is also used to refer to:

• Julian calendar dates
• ordinal dates (day-of-year)

The use of Julian date to refer to the day-of-year (ordinal date) is usually considered to be incorrect although it is widely used that way in the earth sciences and computer programming.

Alternatives

Because the starting point is so long ago, numbers in the Julian day can be quite large and cumbersome. A more recent starting point is sometimes used, for instance by dropping the leading digits, in order to fit into limited computer memory with an adequate amount of precision. In the following table, times are given in 24 hour notation.

• The Modified Julian Day is found by rounding downward. The MJD was introduced by the Smithsonian Astrophysical Observatory in 1957 to record the orbit of Sputnik via an IBM 704 (36-bit machine) and using only 18 bits until August 7, 2576. MJD is the epoch of OpenVMS, using 63-bit date/time postponing the next Y2K campaign to July 31, 31086 02:48:05.47.^[7]

• The Dublin Julian Day (DJD) is the number of days that has elapsed since the epoch of the solar and lunar ephemerides used from 1900 through 1983, Newcomb's Tables of the Sun and Ernest W. Brown's Tables of the Motion of the Moon (1919). This epoch was noon UT on January 0, 1900, which is the same as noon UT on December 31, 1899. The DJD was defined by the International Astronomical Union at their 1955 meeting in Dublin, Ireland.^[8]

• The Lilian day number is a count of days of the Gregorian calendar and not defined relative to the Julian Date. It is an integer applied to a whole day; day 1 was October 15, 1582, which was the day the Gregorian calendar went into effect. The original paper defining it makes no mention of the time zone, and no mention of time-of-day.^[9] It was named for Aloysius Lilius, the principal author of the Gregorian calendar.

• The ANSI Date defines January 1, 1601 as day 1, and is used as the origin of COBOL integer dates. This epoch is the beginning of the previous 400-year cycle of leap years in the Gregorian calendar, which ended with the year 2000.

• Rata Die is a system (or more precisely a family of three systems) used in the book Calendrical Calculations. It uses the local timezone, and day 1 is January 1, 1, that is, the first day of the Christian or Common Era in the proleptic Gregorian calendar.

The Heliocentric Julian Day (HJD) is the same as the Julian day, but adjusted to the frame of reference of the Sun, and thus can differ from the Julian day by as much as 8.3 minutes, that being the time it takes the Sun's light to reach Earth. As two separate astronomical measurements can exist that were taken when the Earth, astronomical objects, and Sun are in a straight line but the Earth was actually on opposite sides of the Sun for the two measurements, that is at one roughly 500 light seconds nearer to the astronomical than the Sun for the first measure, then 500 light seconds further from the astronomical object than the Sun for the second measure, then the subsequent light time error between two Julian Day measures can amount to nearly as much as 1000 seconds different relative to the same Heliocentric Julian Day interval which can make a significant difference when measuring temporal phenomena for short period astronomical objects over long time intervals. The Julian day is sometimes referred to as the Geocentric Julian Day (GJD) in order to distinguish it from HJD.

History

The Julian day number is based on the Julian Period proposed by Joseph Scaliger in 1583, at the time of the Gregorian calendar reform, but it is the multiple of three calendar cycles used with the Julian calendar:

15 (indiction cycle) × 19 (Metonic cycle) × 28 (Solar cycle) = 7980 years

Its epoch falls at the last time when all three cycles were in their first year together — Scaliger chose this because it preceded all historical dates.

Note: although many references say that the Julian in "Julian day" refers to Scaliger's father, Julius Scaliger, in the introduction to Book V of his Opus de Emendatione Temporum ("Work on the Emendation of Time") he states, "Iulianum vocavimus: quia ad annum Iulianum dumtaxat accomodata est", which translates more or less as "We have called it Julian merely because it is accommodated to the Julian year." This Julian refers to Julius Caesar, who introduced the Julian calendar in 46 BC.

In his book Outlines of Astronomy, first published in 1849, the astronomer John Herschel wrote:

The first year of the current Julian period, or that of which the number in each of the three subordinate cycles is 1, was the year 4713 B.C., and the noon of the 1st of January of that year, for the meridian of Alexandria, is the chronological epoch, to which all historical eras are most readily and intelligibly referred, by computing the number of integer days intervening between that epoch and the noon (for Alexandria) of the day, which is reckoned to be the first of the particular era in question. The meridian of Alexandria is chosen as that to which Ptolemy refers the commencement of the era of Nabonassar, the basis of all his calculations.

Astronomers adopted Herschel's Julian Days in the late nineteenth century, but used the meridian of Greenwich instead of Alexandria, after the former was adopted as the Prime Meridian after the International Meridian Conference in Washington in 1884. This has now become the standard system of Julian days. Julian days are typically used by astronomers to date astronomical observations, thus eliminating the complications resulting from using standard calendar periods like eras, years, or months. They were first introduced into variable star work by Edward Charles Pickering, of the Harvard College Observatory, in 1890.^[10]

Julian days begin at noon because when Herschel recommended them, the astronomical day began at noon (it did so until 1925). The astronomical day had begun at noon ever since Ptolemy chose to begin the days in his astronomical periods at noon. He chose noon because the transit of the Sun across the observer's meridian occurs at the same apparent time every day of the year, unlike sunrise or sunset, which vary by several hours. Midnight was not even considered because it could not be accurately determined using water clocks. Nevertheless, he double-dated most nighttime observations with both Egyptian days beginning at sunrise and Babylonian days beginning at sunset. This would seem to imply that his choice of noon was not, as is sometimes stated, made in order to allow all observations from a given night to be recorded with the same date.

Calculation

The Julian day number can be calculated using the following formulas (integer division is used exclusively, that is, the remainder of all divisions are dropped):

The months (M) January to December are 1 to 12. For the year (Y) astronomical year numbering is used, thus 1 BC is 0, 2 BC is −1, and 4713 BC is −4712. D is the day of the month. JDN is the Julian Day Number, which pertains to the noon occurring in the cooresponding calendar date.

Converting Gregorian calendar date to Julian Day Number

The algorithm^[11] is valid for all Gregorian calendar dates after November 23, −4713.

JDN = (1461 × (Y + 4800 + (M − 14)/12))/4 +(367 × (M − 2 − 12 × ((M − 14)/12)))/12 − (3 × ((Y + 4900 + (M - 14)/12)/100))/4 + D − 32075

Converting Julian calendar date to Julian Day Number

The algorithm^[12] is valid for all values of Y ≥ −4712, that is, for all JD ≥ 0.

JDN = 367 × Y − (7 × (Y + 5001 + (M − 9)/7))/4 + (275 × M)/9 + D + 1729777

Finding Julian date given Julian Day Number and time of day

For the full Julian date, not counting leap seconds (divisions are real numbers):

So, for example, January 1, 2000 at midday corresponds to JD = 2451545.0

The day of the week can be determined from the Julian day number by calculating it modulo 7, where 0 means Monday.

Gregorian calendar from Julian day number

• Let J be the Julian day number from which we want to compute the date components.
• From J, compute a relative Julian day number j from a Gregorian epoch starting on March 1, −4800 (i.e. March 1, 4801 BC in the proleptic Gregorian Calendar), the beginning of the Gregorian quadricentennial 32,044 days before the epoch of the Julian Period.
• From j, compute the number g of Gregorian quadricentennial cycles elapsed (there are exactly 146,097 days per cycle) since the epoch; subtract the days for this number of cycles, it leaves dg days since the beginning of the current cycle.
• From dg, compute the number c (from 0 to 4) of Gregorian centennial cycles (there are exactly 36,524 days per Gregorian centennial cycle) elapsed since the beginning of the current Gregorian quadricentennial cycle, number reduced to a maximum of 3 (this reduction occurs for the last day of a leap centennial year where c would be 4 if it were not reduced); subtract the number of days for this number of Gregorian centennial cycles, it leaves dc days since the beginning of a Gregorian century.
• From dc, compute the number b (from 0 to 24) of Julian quadrennial cycles (there are exactly 1,461 days in 4 years, except for the last cycle which may be incomplete by 1 day) since the beginning of the Gregorian century; subtract the number of days for this number of Julian cycles, it leaves db days in the Gregorian century.
• From db, compute the number a (from 0 to 4) of Roman annual cycles (there are exactly 365 days per Roman annual cycle) since the beginning of the Julian quadrennial cycle, number reduced to a maximum of 3 (this reduction occurs for the leap day, if any, where a would be 4 if it were not reduced); subtract the number of days for this number of annual cycles, it leaves da days in the Julian year (that begins on March 1).
• Convert the four components g, c, b, a into the number y of years since the epoch, by summing their values weighted by the number of years that each component represents (respectively 400 years, 100 years, 4 years, and 1 year).
• With da, compute the number m (from 0 to 11) of months since March (there are exactly 153 days per 5-month cycle; however, these 5-month cycles are offset by 2 months within the year, i.e. the cycles start in May, and so the year starts with an initial fixed number of days on March 1, the month can be computed from this cycle by a Euclidian division by 5); subtract the number of days for this number of months (using the formula above), it leaves d days past since the beginning of the month.
• The Gregorian date (Y, M, D) can then be deduced by simple shifts from (y, m, d).

The calculations below (which use integer division [div] and modulo [mod] with positive numbers only) are valid for the whole range of dates since −4800. For dates before 1582, the resulting date components are valid only in the Gregorian proleptic calendar. This is based on the Gregorian calendar but extended to cover dates before its introduction, including the pre-Christian era. For dates in that era (before year 1 AD), astronomical year numbering is used. This includes a year zero, which immediately precedes 1 AD. Astronomical year zero is 1 BC in the proleptic Gregorian calendar and, in general, proleptic Gregorian year (n BC) = astronomical year (Y = 1 − n). For astronomical year Y (Y < 1), the proleptic Gregorian year is (1 - Y) BC.

Let J = JD + 0.5: (note: this shifts the epoch back by one half day, to start it at 00:00UTC, instead of 12:00 UTC);

• let j = J + 32044; (note: this shifts the epoch back to astronomical year -4800 instead of the start of the Christian era in year 1 AD of the proleptic Gregorian calendar).
• let g = j div 146097; let dg = j mod 146097;
• let c = (dg div 36524 + 1) × 3 div 4; let dc = dg − c × 36524;
• let b = dc div 1461; let db = dc mod 1461;
• let a = (db div 365 + 1) × 3 div 4; let da = db − a × 365;
• let y = g × 400 + c × 100 + b × 4 + a; (note: this is the integer number of full years elapsed since March 1, 4801 BC at 00:00 UTC);
• let m = (da × 5 + 308) div 153 − 2; (note: this is the integer number of full months elapsed since the last March 1 at 00:00 UTC);
• let d = da − (m + 4) × 153 div 5 + 122; (note: this is the number of days elapsed since day 1 of the month at 00:00 UTC, including fractions of one day);
• let Y = y − 4800 + (m + 2) div 12; let M = (m + 2) mod 12 + 1; let D = d + 1;

return astronomical Gregorian date (Y, M, D).

Please be careful implementing this algorithm in C/C++, using one from http://www.astro.uu.nl/~strous/AA/en/reken/juliaansedag.html results in more straight-forward code.The operations div and mod used here are intended to have the same binary operator priority as the multipication and division, and defined as:

You can also use only integers in most of the formula above, by taking J = floor(JD + 0.5), to compute the three integers (Y, M, D).

The time of the day is then computed from the fractional day T = frac(JD + 0.5). The additive 0.5 constant can also be adjusted to take the local timezone into account, when computing a astronomical Gregorian date localized in another timezone than UTC. To convert the fractional day into actual hours, minutes, seconds, the astronomical Gregorian calendar uses a constant length of 24 hours per day (i.e. 86400 seconds exactly), ignoring leap seconds inserted or deleted at end of some specific days in the UTC Gregorian calendar. If you want to convert it to actual UTC time, you will need to compensate the UTC leap seconds by adding them to J before restarting the computation (however this adjustment requires a lookup table, because leap seconds are not predictable with a simple formula); you'll also need to finally determine which of the two possible UTC date and time is used at times where leap seconds are added (no final compensation will be needed if negative leap seconds are occurring on the rare possible days that could be shorter than 24 hours).

Gregorian calendar from UnixTime

Let 'U' be the UnixTime you want to convert, just follow these easy steps:

ss = U mod 60

a = (U − ss) div 60

mm = a mod 60

b = (a − mm) div 60

hh = b mod 24

u = U − ss − mm * 60 − hh * 3600

where ss are seconds, mm minutes, hh hours. Day, month and year can be calculated as in the section Gregorian calendar from Julian day number, applying calculations to:

J = u div 86400 + 2440588

and D being:

D = d + 1

See also

• Julian year (astronomy)
• Julian year (calendar)
• Decimal time
• Epoch (reference date)
• Epoch (astronomy)
• Era
• Time
• Time scales
• Ordinal date
• Dual dating
• 5th millennium BC

Footnotes

1. ^ This equals November 24, 4714 BC in the proleptic Gregorian calendar.
2. ^ The Astronomical Almanac Online 2008, Glossary s. v. Julian date
3. ^ Information Bulletin No. 81. (January 1998), p. 23.
4. ^ The Astronomical Almanac Online 2008, Glossary s. v. Julian day number
5. ^ Nachum Dershowitz and Edward M. Reingold 2008. See its applet Calendrica.
6. ^ Noerdlinger, 1995.
7. ^ Worsham 1988
8. ^ Ransom c. 1988
9. ^ Ohms 1986
10. ^ Furness 1988, p. 206.
11. ^ L. E. Doggett, Ch. 12, "Calendars", p. 604, in Seidelmann 1992
12. ^ L. E. Doggett, Ch. 12, "Calendars", p. 606, in Seidelmann 1992

References

• Astronomical Almanac Online. (2008). U.S. Nautical Almanac Office and Her Majesty's Nautical Almanac Office.
• Furness, C. E. (1915). An introduction to the study of variable stars. Boston: Houghton-Mifflin. Vassar Semi-Centennial Series.
• Information Bulletin No. 81. (January 1998). International Astronomical Union.
• Moyer, Gordon. (April 1981). "The Origin of the Julian Day System," Sky and Telescope 61 311−313.
• Noerdlinger, P. (April 1995 revised May 1996). Metadata Issues in the EOSDIS Science Data Processing Tools for Time Transformations and Geolocation. NASA Goddard Space Flight Center.
• Ohms, B. G. (1986). [http://researchweb.watson.ibm.com/journal/sj/252/ibmsj2502J.pdf Computer processing of dates outside the twentieth century]. IBM Systems Journal, 25, 244–251.
• Ransom, D. H. Jr. (c. 1988) ASTROCLK Astronomical Clock and Celestial Tracking Program (documentation). Published by author. Pages 69–143 archived at http://textfiles.meulie.net. Retrieved September 10, 2009.
• Reingold, E. M. & Dershowitz, N. (2008). Calendrical Calculations 3rd ed. Cambridge University Press.
• Seidelmann, P. Kenneth (ed.) (1992). Explanatory Supplement to the Astronomical Almanac. University Science Books, ISBN 0-935702-68-7
• Strous, L. (2007). Astronomy Answers: Julian Day Number. Astronomical Institute / Utrecht University.
• Worsham, K. (1988). Why is Wednesday, November 17, 1858 the base time for VAX/VMS? Copied from DSIN and archived at http://vms.tuwein.ac.at. Retrieved September 10,2009.

External links

• U.S. Naval Observatory Julian Date Converter
• Julian Day and Civil Date calculator
• U.S. Naval Observatory Time Service article on Modified Julian Date
• U.S. Naval Observatory current MJD service
• MJD explanation (18 bits for dates)
• Outlines of Astronomy by John Herschel
• International Astronomical Union Resolution 1B: On the Use of Julian Dates
• Open-source date conversion software
• Calendrica
• Another Julian Day calculator with conversions to many other calendars valid from 1 January 100 proleptic Gregorian calendar
• Pc-Calculator, Julian Date Calculator

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