The mean siderial day is determined by a procedure similar to that of fixing the solar day; however, this procedure uses a star's passage across a reference point on the celestial sphere (that point now being the vernal equinox) instead of the sun's passage. The mean sidereal day is 23 hours, 56 minutes, 4.10 seconds long in solar time. That means that the solar day appears to be about 4 minutes longer than the sidereal day because Earth in its solar orbit has to move a little farther to get back to the point at which the sun crosses the same meridian.
English | Latin | Saxon |
Sunday | Dies Solis (Sun) | Sun's Day |
Monday | Dies Lunae (Moon) | Moon's Day |
Tuesday | Dies Martis (Mars) | Tiw's Day |
Wednesday | Dies Mercurii (Mercury) | Woden's Day |
Thursday | Dies Jovis (Jupiter) | Thor's Day |
Friday | Dies Veneris (Venus) | Frigg's Day |
Saturday | Dies Saturni (Saturn) | Saterne's Day |
The 12-Hour System of Counting Hours
Midnight = 12 A.M. or 12 M,
A.M. (ante meridiem) = before noon
Noon = 12 P.M. or 12 N, P.M. (post
meridiem) = after noon