The Year
The length of the year is
strictly expressed by the space of time required for the
revolution of the earth round the sun�namely, 365 days, 5
hours, 48 minutes, 49 seconds, and 7 tenths of a second,
for to such a nicety has this time been ascertained.
But
for convenience in reckoning, it has been found necessary
to make the year terminate with a day instead of a
fraction of one, lumping the fractions together so as to
make up a day among themselves. About forty-five years
before Christ, Julius Caesar, having, by the help of
Sosigenes, an Alexandrian philosopher, come to a tolerably
clear under standing of the length of the year, decreed
that every fourth year should be held to consist of 366
days for the purpose of absorbing the odd hours.
The arrangement he
dictated was a rather clumsy one. A day in February, the
sixth before the calends of March (sextilis), was to be
repeated in that fourth year; and each fourth year was
thus to be bissextile. It was as if we were to reckon the
23rd of February twice over. Seeing that, in reality, a
day every fourth year is too much by 11 minutes, 10
seconds, and 3 tenths of a second, it inevitably followed
that the beginning of the year moved onward ahead of the
point at which it was in the days of Caesar; in other
words, the natural time fell behind the reckoning.
From the time of the
Council of Nice, in 325, when the vernal equinox fell
correctly on the 21st of March, Pope Gregory found in 1582
that there had been an over- reckoning to the extent of
ten days, and now the vernal equinox fell on the 11th of
March. To correct the past error, he decreed that the 5th
of October that year should be reckoned as the 15th, and
to keep the year right in future, the overplus being 18
hours, 37 minutes, and 10 seconds in a century, he ordered
that every centurial year that could not be divided by 4,
(1700, 1800, 1900, 2100, 2200, &c.) should not be
bissextile, as it otherwise would be; thus, in short,
dropping the extra day three times every four hundred
years.
The Gregorian style, as
it was called, readily obtained sway in Catholic, but not
in Protestant countries. It was not adopted in Britain
till the year 1752, by which time the discrepancy between
the Julian and Gregorian periods amounted to eleven days.
An act of parliament was passed, dictating that the 3
rd of
September that year should be reckoned the 14th, and that
three of every four of the centurial years should, as in
Pope Gregory's arrangement, not be bissextile or
leap-years. It has consequently a risen�1800 not having
been a leapyear�that the new and old styles now differ by
twelve days, the let of January old style being the 13th
of the month new style. In Russia alone, of all Christian
countries, is the old style still retained ; wherefore it
becomes necessary for one writing in that country to any
foreign correspondent, to set down his date as thus:
12th/24th March, or 25th September /7th
October.
'The old style is still
retained in the accounts of Her Majesty's Treasury. This
is why the Christmas dividends are not considered due till
Twelfth Day, nor the midsummer dividends till the 5th of
July; and in the same way it is not until the 5th of
April that Lady Day is supposed to arrive. There is
another piece of antiquity visible in the public accounts.
In old times, the year was held to begin on the 25th
of March, and this usage is also still observed in the
computations over which the Chancellor of the Exchequer
presides. The consequence is, that the first day of the
financial year is the 5th of April, being old
Lady Day, and with that day the reckonings of our annual
budgets begin and end.' �Times, February 16th,
1861.
Part IV:
On Time
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