FREE BOOKS

Author's List




PREV.   NEXT  
|<   160   161   162   163   164   165   166   167   168   169   170   171   172   173   174   175   176   177   178   179   180   181   182   183   184  
185   186   187   188   189   190   191   192   193   194   195   196   197   198   199   200   201   202   203   204   205   206   207   208   209   >>   >|  
he sidereal day_, which is the interval of time between successive passages of a fixed star over a given meridian; _the apparent solar day_, which is the interval between two passages of the sun's centre over a given meridian, or the interval between two successive noons on a sundial; and _the mean solar day_, which is the interval between the successive passages of a fictitious sun moving uniformly eastward in the celestial equator, and completing its annual course in exactly the same time as that in which the actual sun makes the circuit of the ecliptic. The mean solar days are all exactly the same length; they are equal to the length of the average apparent solar day; and they are each four minutes longer than a sidereal day. We divide our days into 24 hours; each hour into 60 minutes; each minute into 60 seconds. This subdivision of the day requires some mechanical means of continually registering time, and for this purpose we use clocks and watches. The sidereal day and the mean solar day necessitate some means of registering time, such as clocks; therefore the original day in use must have been the apparent solar day. It must then have been reckoned either from sunset to sunset, or from sunrise to sunrise. Later it might have been possible to reckon it from noon to noon, when some method of fixing the moment of noon had been invented; some method, that is to say, of fixing the true north and south, and of noting that the sun was due south, or the shadow due north. Our own reckoning from midnight to midnight is a late method. Midnight is not marked by the peculiar position of any visible heavenly body; it has, in general, to be registered by some mechanical time-measurer. In the Old Testament Scriptures the ecclesiastical reckoning was always from one setting of the sun to the next. In the first chapter of Genesis the expressions for the days run, "The evening and the morning," as if the evening took precedence of the morning. When the Passover was instituted as a memorial feast, the command ran-- "In the first month, on the fourteenth day of the month at even, ye shall eat unleavened bread, until the one and twentieth day of the month at even. Seven days shall there be no leaven." And again, for the sabbath of rest in the seventh month-- "In the ninth day of the month at even, from even unto even, shall ye celebrate your sabbath." The ecclesiastical "day" of the Jews, the
PREV.   NEXT  
|<   160   161   162   163   164   165   166   167   168   169   170   171   172   173   174   175   176   177   178   179   180   181   182   183   184  
185   186   187   188   189   190   191   192   193   194   195   196   197   198   199   200   201   202   203   204   205   206   207   208   209   >>   >|  



Top keywords:

interval

 

sidereal

 

successive

 
method
 
apparent
 

passages

 
minutes
 

morning

 

clocks

 

ecclesiastical


midnight
 

registering

 

sunset

 

evening

 

mechanical

 
sunrise
 

fixing

 

sabbath

 

length

 
meridian

reckoning

 
marked
 

Scriptures

 

peculiar

 

visible

 

measurer

 

registered

 
general
 

Testament

 

heavenly


position

 

leaven

 

twentieth

 

celebrate

 

seventh

 

unleavened

 

expressions

 

Genesis

 

chapter

 

precedence


command

 

Midnight

 

fourteenth

 

memorial

 

Passover

 

instituted

 
setting
 

average

 

ecliptic

 

circuit