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== Month System ==
 
[Category: Proposed Calendars]
 
 
'''<u>Month System:</u>'''
 
   
 
Each quarter has 3 months, with the following lengths: 30 days, 30 days, & 31 days,,in that order..
 
Each quarter has 3 months, with the following lengths: 30 days, 30 days, & 31 days,,in that order..
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# For a given same year-start day, the 30,30,31 months' starting-days have the least possible maximum departure from the starting-days of the old Roman months.
 
# For a given same year-start day, the 30,30,31 months' starting-days have the least possible maximum departure from the starting-days of the old Roman months.
 
# This ordering of month-lengths divides weekdays most evenly between the 3 months of a quarter.
 
# This ordering of month-lengths divides weekdays most evenly between the 3 months of a quarter.
'''<u>Leapyear System:</u>'''
 
   
 
== Leapyear System ==
'''Year-Length:'''
 
  +
 
=== Year-Length ===
   
 
Ordinary (non-leap) years are 364 days long.
 
Ordinary (non-leap) years are 364 days long.
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The 364-day length of the ordinary year is chosen because it's a multiple of 7. With an ordinary year's length that's a multiple of 7, and by using a leapweek instead of a leapday, every year begins on the same day. ...and each quarter's 3 months always begin on Monday, Wednesday, & Friday.
 
The 364-day length of the ordinary year is chosen because it's a multiple of 7. With an ordinary year's length that's a multiple of 7, and by using a leapweek instead of a leapday, every year begins on the same day. ...and each quarter's 3 months always begin on Monday, Wednesday, & Friday.
   
'''Principle of Minimum-Displacement Leapyear Rule:'''
+
=== Principle of Minimum-Displacement Leapyear Rule ===
   
Due to the integer number of days in a calendar year, every calendar experiences an ongoing change of the relation between date and season. (More specifically, the relation between date and solar ecliptic longitude). With all calendars, a leapyear periodically counters that variation. ...resulting in a periodic oscillation of the relation between date & season.
+
Due to the integer number of days in a calendar year, every calendar experiences an ongoing change of the relation between date and season. (More specifically, the relation between date and solar ecliptic longitude). With all calendars, a leapyear periodically counters that variation. ...resulting in a periodic oscillation of the relation between date & season.
   
 
Minimum-Displacement centers that oscillation about a desired date/season relation, and minimizes the range of departure (displacement) from that desired center.
 
Minimum-Displacement centers that oscillation about a desired date/season relation, and minimizes the range of departure (displacement) from that desired center.
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(With a leapweek calendar, half a week is the minimum possible value for the maximum displacement of the calendar's date/season relation from its desired center--hence the name "Minimum-Displacement".)
 
(With a leapweek calendar, half a week is the minimum possible value for the maximum displacement of the calendar's date/season relation from its desired center--hence the name "Minimum-Displacement".)
   
'''<u>Detailed Instruction for Minimum-Displacement Leapyear Rule:</u>'''
+
=== Detailed Instruction for Minimum-Displacement Leapyear Rule ===
   
<u>Variable</u>:
+
; Variable: D (represents displacement)
 
; Constants
 
 
: ''Dzero'' = -.6288 or 0 (initial value of D at calendar's epoch)
D (represents displacement)
 
 
: ''Y'' = 365.24219 (That's the number of days in a mean-tropical-year)
 
<u>Constants:</u>
 
 
Dzero = -.6288 or 0 (initial value of D at calendar's epoch)
 
 
Y = 365.24219 (That's the number of days in a mean-tropical-year)
 
   
 
(More later about these choices of values for the 2 constants)
 
(More later about these choices of values for the 2 constants)
   
<u>Leapyear Rule:</u>
+
==== Leapyear Rule ====
   
At the end of every year, the value of D is changed by an amount equal to Y minus the number of days in that year.
+
At the end of every year, the value of D is changed by an amount equal to ''Y'' minus the number of days in that year.
   
If that, at the end of a particular year, would otherwise result in a D value greater than 3.5, then a leapweek is added to the end of that year. (...resulting in a D value between 0 and -3.5)
+
If that, at the end of a particular year, would otherwise result in a ''D'' value greater than 3.5, then a leapweek is added to the end of that year. (resulting in a ''D'' value between 0 and -3.5)
   
Thus, the magnitude of D is never greater than 3.5
+
Thus, the magnitude of ''D'' is never greater than 3.5
   
 
D is always between -3.5 and +3.5
 
D is always between -3.5 and +3.5
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<u>Explanation of the Choices of Values for the 2 Constants:</u>
 
<u>Explanation of the Choices of Values for the 2 Constants:</u>
   
Two values are offered for the value of Dzero:
+
Two values are offered for the value of ''Dzero'':
   
Dzero = 0 would center the date-season variation about the date-season relation existing on Gregorian January 1st, 2017, the day before this calendar's epoch..
+
''Dzero'' = 0 would center the date-season variation about the date-season relation existing on Gregorian January 1st, 2017, the day before this calendar's epoch..
   
Dzero = -.6288 would center the date-season variation about the midpoint of the Gregorian Calendar's date-season variation between the Gregorian dates of January 1, 1950 and January 1, 2017.
+
''Dzero'' = -0.6288 would center the date-season variation about the midpoint of the Gregorian Calendar's date-season variation between the Gregorian dates of January 1, 1950 and January 1, 2017.
   
The latter value, Dzero = - .6288 would center the calendar in the middle of the region where the Gregorian Calendar has been during the human lifetime preceding the calendar's epoch. .
+
The latter value, ''Dzero'' = - 0.6288 would center the calendar in the middle of the region where the Gregorian Calendar has been during the human lifetime preceding the calendar's epoch. .
   
'''<u>Epoch:</u>'''
+
== Epoch ==
   
<nowiki> </nowiki>This calendar's epoch (starting-date) is its January 1, 2017, which occurs on Gregorian January 2nd, 2017.
+
This calendar's epoch (starting-date) is its January 1, 2017, which occurs on Gregorian January 2nd, 2017.
   
'''<u>Advantages of Minimum-Displacement in Comparison to Other Calendars:</u>'''
+
== Advantages of Minimum-Displacement in Comparison to Other Calendars ==
   
<u>Advantages in comparison to Hanke-Henry:</u>
+
=== Advantages in comparison to Hanke-Henry ===
   
 
Hanke-Henry uses the Nearest-Monday year-start rule, instead of having its own leapyear rule. Each year starts on the Monday that is closes to the Gregorian January 1st for that year. There's nothing wrong with Nearest-Monday. It's very briefly-stated, and doesn't require the definition of a really new leapyear rule. And its maximum displacement during a 400 year Gregorian cycle is barely more than Minimum-Displacement's overall displacement-range.
 
Hanke-Henry uses the Nearest-Monday year-start rule, instead of having its own leapyear rule. Each year starts on the Monday that is closes to the Gregorian January 1st for that year. There's nothing wrong with Nearest-Monday. It's very briefly-stated, and doesn't require the definition of a really new leapyear rule. And its maximum displacement during a 400 year Gregorian cycle is barely more than Minimum-Displacement's overall displacement-range.
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Because Hanke-Henry's Nearest-Monday year-start rule is based on the Gregorian Calendar, it inherits some properties of the Gregorian:
 
Because Hanke-Henry's Nearest-Monday year-start rule is based on the Gregorian Calendar, it inherits some properties of the Gregorian:
  +
 
# The Gregorian leapyear rule was designed to minimize the variation of the (northern) Vernal Equinox with respect to the calendar's dates. But that emphasis on & favoring of the March Equinox is north-chauvinistic, because the March Equinox isn't everyone's Vernal Equinox. (In the Southern Hemisphere, it's their Autumnal Equinox). Hanke-Henry, by its use of Nearest-Monday, inherits that attribute. In contrast, Minimum-Displacement, by its use of the mean-tropical-year, minimizes variation in the date-season relation over the entire year.
 
# The Gregorian leapyear rule was designed to minimize the variation of the (northern) Vernal Equinox with respect to the calendar's dates. But that emphasis on & favoring of the March Equinox is north-chauvinistic, because the March Equinox isn't everyone's Vernal Equinox. (In the Southern Hemisphere, it's their Autumnal Equinox). Hanke-Henry, by its use of Nearest-Monday, inherits that attribute. In contrast, Minimum-Displacement, by its use of the mean-tropical-year, minimizes variation in the date-season relation over the entire year.
# The Gregorian Calendar, in addition to the unavoidable periodic displacement, a unidirectional displacement ''drift''. ...with the result that there's no stationary center of oscillation. The center of oscillation experiences an ongoing unidirectional drift. Hanke-Henry, by its use of Nearest-Monday, inherits that drift. Minimum-Displacement has no drift. It has a stationary center of oscillation, chosen by the choice of Dzero value, as described above.
+
# The Gregorian Calendar, in addition to the unavoidable periodic displacement, a unidirectional displacement ''drift''. ...with the result that there's no stationary center of oscillation. The center of oscillation experiences an ongoing unidirectional drift. Hanke-Henry, by its use of Nearest-Monday, inherits that drift. Minimum-Displacement has no drift. It has a stationary center of oscillation, chosen by the choice of Dzero value, as described above.
  +
<u>Advantages in comparison to Symmetry 454 & Symmetry010:</u>
+
=== Advantages in comparison to Symmetry 454 & Symmetry010 ===
  +
 
# The Minimum-Displacement leapyear rule is the direct, natural obvious, and obviouisly-motivated way to minimize a calendar's displacement with respect to a desired center of oscillation.
 
# The Minimum-Displacement leapyear rule is the direct, natural obvious, and obviouisly-motivated way to minimize a calendar's displacement with respect to a desired center of oscillation.
 
# Symmetry454's months of 28, 35, & 28 days are drastically unequal, whereas 30,20,31 Minimum-Displacement achieves the most uniform month-lengths possible with 12 months.
 
# Symmetry454's months of 28, 35, & 28 days are drastically unequal, whereas 30,20,31 Minimum-Displacement achieves the most uniform month-lengths possible with 12 months.
# In comparison to Symmetry010's 30,31,30 quarters, 30,30,31 Minimum-Displacement (as described in the "Month-System" section above) minimizes the departure of the months' start-days from those of the current Roman months. ...and divides the quarter's weekdays as equally as possible between the quarter's 3 months.
+
# In comparison to Symmetry010's 30,31,30 quarters, 30,30,31 Minimum-Displacement (as described in the "Month-System" section above) minimizes the departure of the months' start-days from those of the current Roman months. ...and divides the quarter's weekdays as equally as possible between the quarter's 3 months.
   
 
[[Category: Proposed Calendars]]
.
 

Revision as of 15:44, 3 January 2017

Month System

Each quarter has 3 months, with the following lengths: 30 days, 30 days, & 31 days,,in that order..

There have been a number of calendar proposals with this month system. Its advantages are:

  1. With all months 30 or 31 days long, the months are as uniform as is possible with 12 months.
  2. For a given same year-start day, the 30,30,31 months' starting-days have the least possible maximum departure from the starting-days of the old Roman months.
  3. This ordering of month-lengths divides weekdays most evenly between the 3 months of a quarter.

Leapyear System

Year-Length

Ordinary (non-leap) years are 364 days long.

Leapyears have a "leap-week" added to their end, making leapyears 371 days long.

The 364-day length of the ordinary year is chosen because it's a multiple of 7. With an ordinary year's length that's a multiple of 7, and by using a leapweek instead of a leapday, every year begins on the same day. ...and each quarter's 3 months always begin on Monday, Wednesday, & Friday.

Principle of Minimum-Displacement Leapyear Rule

Due to the integer number of days in a calendar year, every calendar experiences an ongoing change of the relation between date and season. (More specifically, the relation between date and solar ecliptic longitude). With all calendars, a leapyear periodically counters that variation. ...resulting in a periodic oscillation of the relation between date & season.

Minimum-Displacement centers that oscillation about a desired date/season relation, and minimizes the range of departure (displacement) from that desired center.

Minimum-Displacement accomplishes that by having a leapyear, adding a week to the end of a particular year, if the completion of that year would otherwise displace the calendar from its desired center by more than half of a week. Thus, the displacement from desired center never exceeds half of a week.

(With a leapweek calendar, half a week is the minimum possible value for the maximum displacement of the calendar's date/season relation from its desired center--hence the name "Minimum-Displacement".)

Detailed Instruction for Minimum-Displacement Leapyear Rule

Variable
D (represents displacement)
Constants
Dzero = -.6288 or 0 (initial value of D at calendar's epoch)
Y = 365.24219 (That's the number of days in a mean-tropical-year)

(More later about these choices of values for the 2 constants)

Leapyear Rule

At the end of every year, the value of D is changed by an amount equal to Y minus the number of days in that year.

If that, at the end of a particular year, would otherwise result in a D value greater than 3.5, then a leapweek is added to the end of that year. (… resulting in a D value between 0 and -3.5)

Thus, the magnitude of D is never greater than 3.5

D is always between -3.5 and +3.5

Explanation of the Choices of Values for the 2 Constants:

Two values are offered for the value of Dzero:

Dzero = 0 would center the date-season variation about the date-season relation existing on Gregorian January 1st, 2017, the day before this calendar's epoch..

Dzero = -0.6288 would center the date-season variation about the midpoint of the Gregorian Calendar's date-season variation between the Gregorian dates of January 1, 1950 and January 1, 2017.

The latter value, Dzero = - 0.6288 would center the calendar in the middle of the region where the Gregorian Calendar has been during the human lifetime preceding the calendar's epoch. .

Epoch

This calendar's epoch (starting-date) is its January 1, 2017, which occurs on Gregorian January 2nd, 2017.

Advantages of Minimum-Displacement in Comparison to Other Calendars

Advantages in comparison to Hanke-Henry

Hanke-Henry uses the Nearest-Monday year-start rule, instead of having its own leapyear rule. Each year starts on the Monday that is closes to the Gregorian January 1st for that year. There's nothing wrong with Nearest-Monday. It's very briefly-stated, and doesn't require the definition of a really new leapyear rule. And its maximum displacement during a 400 year Gregorian cycle is barely more than Minimum-Displacement's overall displacement-range.

But it's defined in terms of the leapyear rule of another calendar (the Gregorian), as opposed to Minimum-Displacement's direct, ovious & natural minimization of displacement.

Because Hanke-Henry's Nearest-Monday year-start rule is based on the Gregorian Calendar, it inherits some properties of the Gregorian:

  1. The Gregorian leapyear rule was designed to minimize the variation of the (northern) Vernal Equinox with respect to the calendar's dates. But that emphasis on & favoring of the March Equinox is north-chauvinistic, because the March Equinox isn't everyone's Vernal Equinox. (In the Southern Hemisphere, it's their Autumnal Equinox). Hanke-Henry, by its use of Nearest-Monday, inherits that attribute. In contrast, Minimum-Displacement, by its use of the mean-tropical-year, minimizes variation in the date-season relation over the entire year.
  2. The Gregorian Calendar, in addition to the unavoidable periodic displacement, a unidirectional displacement drift. ...with the result that there's no stationary center of oscillation. The center of oscillation experiences an ongoing unidirectional drift. Hanke-Henry, by its use of Nearest-Monday, inherits that drift. Minimum-Displacement has no drift. It has a stationary center of oscillation, chosen by the choice of Dzero value, as described above.

Advantages in comparison to Symmetry 454 & Symmetry010

  1. The Minimum-Displacement leapyear rule is the direct, natural obvious, and obviouisly-motivated way to minimize a calendar's displacement with respect to a desired center of oscillation.
  2. Symmetry454's months of 28, 35, & 28 days are drastically unequal, whereas 30,20,31 Minimum-Displacement achieves the most uniform month-lengths possible with 12 months.
  3. In comparison to Symmetry010's 30,31,30 quarters, 30,30,31 Minimum-Displacement (as described in the "Month-System" section above) minimizes the departure of the months' start-days from those of the current Roman months. ...and divides the quarter's weekdays as equally as possible between the quarter's 3 months.