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Subject: Gregorian Calendar -- from Eric Weisstein's World of Astronomy
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  =09
   Astronomy Contributors   	  Mercado
   Calendars   	  Calendrical Systems


Gregorian Calendar=09


	    =09
Portions of this entry contributed by Alejandra Mercado

The calendar currently in worldwide use for secular purposes based on =20=

a cycle of 400 years comprising 146,097 days, giving a year of =20
average length 365.2425 days. The Gregorian calendar is a =20
modification of the Julian calendar in which leap years are omitted =20
in years divisible  by 100 but not divisible  by 400. By this rule, =20
the year 1900 was not a leap year (1900 is divisible by 100 and not =20
divisible by 400), but the year 2000 will be a leap year (2000 is =20
divisible  by 400). The total number of days in 400 years is =20
therefore given by



This also gives an exact number of   weeks per 400-year cycle.

The Gregorian calendar was constructed to give a close approximation =20
to the tropical year, which is the actual length of time it takes for =20=

the Earth to complete one orbit around the Sun.

The Julian calendar was switched over to the Gregorian starting in =20
1582, at which point the 10 day difference between the actual time of =20=

year and traditional time of year on which calendrical events =20
occurred became intolerable. The switchover was bitterly opposed by =20
much of the populace, who feared it was attempt by landlords to cheat =20=

then out of a week and a half's rent. However, when Pope Gregory XIII =20=

decreed that the day after October 4, 1582 would be October 15, 1582, =20=

the Catholic countries of France, Spain, Portugal, and Italy =20
complied. Various Catholic German countries (Germany was not yet =20
unified), Belgium, the Netherlands, and Switzerland followed suit =20
within a year or two, and Hungary followed in 1587.

Because of the Pope's decree, the reform of the Julian calendar came =20
to be known as the Gregorian calendar. However, the rest of Europe =20
did not follow suit for more than a century.

The Protestant German countries adopted the Gregorian reform in 1700. =20=

By this time, the calendar trailed the seasons by 11 days. England =20
(and the American colonies) finally followed suit in 1752, and =20
Wednesday, September 2, 1752 was immediately followed by Thursday, =20
September 14, 1752. This traumatic change resulted in widespread =20
riots and the populace demanding "Give us the eleven days back!"

English Calendar:

September 1752
Su	M	Tu	W	Th	F	Sa
&;	&;	1	2	14	15	16
17	18	19	20	21	22	23
24	25	26	27	28	29	30
Sweden followed England's lead in 1753. Russia, however, did not =20
follow suit until 1918, when January 31, 1918 was immediately =20
followed by February 14th. In fact, however, the USSR is not on the =20
Gregorian calendar, but on a more accurate one of their own devising. =20=

The USSR calendar is designed to more closely approximate the true =20
length of the tropical year, thus has one additional rule for when a =20
year is a leap year. It will remain in synchronization with the =20
Gregorian calendar for thousands more years, by which time one or =20
both will have probably fallen into disuse. Similarly, Iranian =20
calendar is also a more accurate version of the Gregorian calendar =20
(Ross).

Formulas for computing the Julian date from the Gregorian dates are =20
given in Danby (1988) and Sinnott (1991). Let   denote the integer =20
part  (sometimes known in mathematical circles as the floor =20
function   ), let Y be the Gregorian year, M the month number =20
(1=3DJanuary, 2=3DFebruary, etc.), D the day of the month, and UT the =20=

universal time. For all AD dates in the Gregorian calendar,

=09
=09
	 (1)
For Gregorian calendar dates 1901-2099, the formula can be simplified to

=09
	 (2)


Calendar, French Revolutionary Calendar, Iranian Calendar, Islamic =20
Calendar, Julian Date, Julian Calendar, Julian Date, Leap Day, Leap =20
Year, Tropical Year, Year





References


Danby, J. M. Fundamentals of Celestial Mechanics, 2nd ed., rev. enl. =20
Richmond, VA: Willmann-Bell, Eqn. 6.16.4, p. 207, 1988.

Ross, K. L. "Iranian Calendars." http://www.friesian.com/=20
calendar.htm#iran.

Sinnott, R. W. "Bits and Bytes." Sky & Telescope 82, 183, Aug. 1991.

Vardi, I. "The Gregorian Calendar." =A73.5.2 in Computational =20
Recreations in Mathematica. Reading, MA: Addison-Wesley, p. 45, 1991.







=A9 Eric W. Weisstein






	 =09







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worldwide use for secular purposes based on a cycle of 400 years =
comprising 146,097 days, giving a year of average length 365.2425 days.  =
The Gregorian calendar is a modification of the Julian calendar in which =
leap years are omitted in years divisible by 100 but not divisible by =
400.  By this rule, the year 1900 was not a leap year (1900 is divisible =
by 100 and not divisible by 400), but the year 2000 will be a leap year =
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<P>
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<P>



  <I>Portions of this entry contributed by <A name=3D"tex2html7" =
href=3D"topics/Mercado.html">Alejandra Mercado</A></I> </P><P>The <A =
href=3D"Calendar.html">calendar</A> currently in worldwide use for =
secular purposes based on a cycle of 400 years comprising 146,097
days, giving a year of average length 365.2425 days.  The Gregorian =
calendar is a modification of the <A href=3D"JulianCalendar.html">Julian
calendar</A> in which <A href=3D"LeapYear.html">leap years</A> are =
<I>omitted</I> in years <A =
href=3D"http://mathworld.wolfram.com/Divisible.html">divisible</A> <IMG =
src=3D"http://scienceworld.wolfram.com/images/crossrefs/math.gif" =
width=3D"12" height=3D"12"> by 100 but <I>not</I>
<A href=3D"http://mathworld.wolfram.com/Divisible.html">divisible</A> =
<IMG src=3D"http://scienceworld.wolfram.com/images/crossrefs/math.gif" =
width=3D"12" height=3D"12"> by 400.  By this rule, the year 1900 was =
<I>not</I> a leap year (1900 is divisible by 100 and <I>not</I> =
divisible by 400), but the year 2000 <I>will</I> be a <A =
href=3D"LeapYear.html">leap year</A> (2000 is <A =
href=3D"http://mathworld.wolfram.com/Divisible.html">divisible</A> <IMG =
src=3D"http://scienceworld.wolfram.com/images/crossrefs/math.gif" =
width=3D"12" height=3D"12"> by 400).  The
total number of days in 400 years is therefore given by
</P><DIV align=3D"CENTER">
=20

<IMG width=3D"210" height=3D"27" border=3D"0" src=3D"gimg45.gif">
</DIV>
<BR clear=3D"ALL">


<P>This also gives an exact number of=20

<IMG width=3D"143" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg46.gif"> <A href=3D"Week.html">weeks</A> per 400-year cycle. =20=


</P><P>The Gregorian calendar was constructed to give a close =
approximation to the <A href=3D"TropicalYear.html">tropical year</A>, =
which is the actual
length of time it takes for the Earth to complete one orbit around the =
Sun.

</P><P>The <A href=3D"JulianCalendar.html">Julian calendar</A> was =
switched over to the Gregorian starting in 1582, at which point the 10 =
day difference
between the actual time of year and traditional time of year on which =
calendrical events occurred became intolerable.
The switchover was bitterly opposed by much of the populace, who feared =
it was attempt by landlords to cheat then out of
a week and a half's rent.  However, when Pope Gregory XIII decreed that =
the day after October 4, 1582 would be October
15, 1582, the Catholic countries of France, Spain, Portugal, and Italy =
complied.  Various Catholic German countries
(Germany was not yet unified), Belgium, the Netherlands, and Switzerland =
followed suit within a year or two, and Hungary
followed in 1587.

</P><P>Because of the Pope's decree, the reform of the Julian calendar =
came to be known as the Gregorian calendar. However, the
rest of Europe did not follow suit for more than a century.

</P><P>The Protestant German countries adopted the Gregorian reform in =
1700.  By this time, the calendar trailed the seasons by
11 days.  England (and the American colonies) finally followed suit in =
1752, and Wednesday, September 2, 1752 was
immediately followed by Thursday, September 14, 1752.  This traumatic =
change resulted in widespread riots and the
populace demanding "Give us the eleven days back!"

</P><P>English Calendar:
</P><DIV align=3D"CENTER"><TABLE cellpadding=3D"3" border=3D"1">
<TBODY><TR><TD align=3D"CENTER" colspan=3D"7">September =
1752</TD></TR><TR><TD align=3D"RIGHT">Su</TD><TD align=3D"RIGHT">M</TD><TD=
 align=3D"RIGHT">Tu</TD><TD align=3D"RIGHT">W</TD><TD =
align=3D"RIGHT">Th</TD><TD align=3D"RIGHT">F</TD><TD =
align=3D"RIGHT">Sa</TD></TR><TR><TD align=3D"RIGHT">&amp;;</TD><TD =
align=3D"RIGHT">&amp;;</TD><TD align=3D"RIGHT">1</TD><TD =
align=3D"RIGHT">2</TD><TD align=3D"RIGHT">14</TD><TD =
align=3D"RIGHT">15</TD><TD align=3D"RIGHT">16</TD></TR><TR><TD =
align=3D"RIGHT">17</TD><TD align=3D"RIGHT">18</TD><TD =
align=3D"RIGHT">19</TD><TD align=3D"RIGHT">20</TD><TD =
align=3D"RIGHT">21</TD><TD align=3D"RIGHT">22</TD><TD =
align=3D"RIGHT">23</TD></TR><TR><TD align=3D"RIGHT">24</TD><TD =
align=3D"RIGHT">25</TD><TD align=3D"RIGHT">26</TD><TD =
align=3D"RIGHT">27</TD><TD align=3D"RIGHT">28</TD><TD =
align=3D"RIGHT">29</TD><TD align=3D"RIGHT">30</TD></TR></TBODY></TABLE>
</DIV>

<P>Sweden followed England's lead in 1753.  Russia, however, did not =
follow suit until 1918, when January 31, 1918 was
immediately followed by February 14th.  In fact, however, the USSR is =
not on the Gregorian calendar, but on a more
accurate one of their own devising.  The USSR calendar is designed to =
more closely approximate the true length of the
<A href=3D"TropicalYear.html">tropical year</A>, thus has one additional =
rule for when a year is a <A href=3D"LeapYear.html">leap year</A>.  It =
will remain in
synchronization with the Gregorian calendar for thousands more years, by =
which time one or both will have probably
fallen into disuse.  Similarly, <A href=3D"IranianCalendar.html">Iranian =
calendar</A> is also a more accurate version of the <A =
href=3D"GregorianCalendar.html">Gregorian calendar</A>
(Ross).

</P><P>Formulas for computing the <A href=3D"JulianDate.html">Julian =
date</A> from the Gregorian dates are given in Danby (1988) and Sinnott =
(1991). Let


<IMG width=3D"51" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg47.gif"> denote the <A =
href=3D"http://mathworld.wolfram.com/IntegerPart.html">integer part</A> =
<IMG src=3D"http://scienceworld.wolfram.com/images/crossrefs/math.gif" =
width=3D"12" height=3D"12"> (sometimes known in mathematical circles as =
the <A href=3D"http://mathworld.wolfram.com/FloorFunction.html">floor =
function</A> <IMG =
src=3D"http://scienceworld.wolfram.com/images/crossrefs/math.gif" =
width=3D"12" height=3D"12">


<IMG width=3D"27" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg48.gif">), let <I>Y</I> be the Gregorian year, <I>M</I> the =
month number (1=3DJanuary, 2=3DFebruary, etc.), <I>D</I> the day of the
month, and <I>UT</I> the <A href=3D"UniversalTime.html">universal =
time</A>.  For all <A href=3D"AD.html">AD</A> dates in the Gregorian =
calendar,

</P><P><TABLE width=3D"100%">
<TBODY><TR><TD align=3D"left">

<IMG width=3D"329" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg52.gif"> </TD><TD></TD></TR><TR><TD align=3D"left">


<IMG width=3D"307" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg53.gif"> </TD><TD></TD></TR><TR><TD align=3D"left">


<IMG width=3D"305" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg54.gif"> </TD><TD width=3D"10" align=3D"right">
(1)</TD></TR></TBODY></TABLE>
For Gregorian calendar dates 1901-2099, the formula can be simplified to

</P><P><TABLE width=3D"100%">
<TBODY><TR><TD align=3D"left">

<IMG width=3D"329" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg52.gif"> </TD><TD></TD></TR><TR><TD align=3D"right">


<IMG width=3D"305" height=3D"31" align=3D"MIDDLE" border=3D"0" =
src=3D"gimg55.gif"> </TD><TD width=3D"10" align=3D"right">
(2)</TD></TR></TBODY></TABLE>

</P><P>
</P><P><IMG width=3D"47" height=3D"13" align=3D"LEFT" =
src=3D"/images/seealso.gif"><A href=3D"Calendar.html">Calendar</A>, <A =
href=3D"FrenchRevolutionaryCalendar.html">French Revolutionary =
Calendar</A>, <A href=3D"IranianCalendar.html">Iranian Calendar</A>, <A =
href=3D"IslamicCalendar.html">Islamic Calendar</A>, <A =
href=3D"JulianDate.html">Julian Date</A>, <A =
href=3D"JulianCalendar.html">Julian Calendar</A>, <A =
href=3D"JulianDate.html">Julian Date</A>, <A href=3D"LeapDay.html">Leap =
Day</A>, <A href=3D"LeapYear.html">Leap Year</A>, <A =
href=3D"TropicalYear.html">Tropical Year</A>,
<A href=3D"Year.html">Year</A>

</P><P>
</P><P><BR clear=3D"all">
<IMG height=3D"2" align=3D"BOTTOM" border=3D"0" =
src=3D"/images/fade-teal.gif"> </P><P><A =
name=3D"refs"><B>References</B></A>
<FONT size=3D"-1"></FONT></P><FONT size=3D"-1"><P>

</P><P>Danby, J.=A0M.  <A =
href=3D"http://www.amazon.com/exec/obidos/ASIN/0943396204/weisstein-20"><I=
>Fundamentals of Celestial Mechanics, 2nd ed., rev. enl.</I></A>  =
Richmond, VA:
  Willmann-Bell, Eqn. 6.16.4, p.=A0207, 1988. </P><P>Ross, K.=A0L. =
"Iranian Calendars."  <TT><A name=3D"tex2html8" =
href=3D"http://www.friesian.com/calendar.htm#iran">http://www.friesian.com=
/calendar.htm#iran</A></TT>. </P><P>Sinnott, R.=A0W. "Bits and Bytes." =
<I>Sky &amp; Telescope</I> <B>82</B>, 183, Aug. 1991.
</P><P>Vardi, I. "The Gregorian Calendar." =A73.5.2 in <A =
href=3D"http://www.amazon.com/exec/obidos/ASIN/0685479412/weisstein-20"><I=
>Computational Recreations in Mathematica.</I></A>
  Reading, MA: Addison-Wesley, p.=A045, 1991. </P><P>
</P></FONT><P><FONT size=3D"-1"></FONT>

</P><P>
</P><P>
</P><P><BR>

</P><P>
<FONT size=3D"-1"><I>=A9 Eric W. Weisstein</I>

</FONT></P><FONT size=3D"-1"></FONT><P><FONT size=3D"-1"><BR>

</FONT>

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