The calendar is such a routine, everyday thing, but how much do you actually know about the operation of it. Why is it like that?
A DAY: The Earth rotates at a reasonably steady speed about the imaginary line running between the North and South Poles called the Earth’s Axis. The time it takes to spin once is called a ‘rotation’ and this takes just under twenty-four hours. However, because the Earth is continuously travelling around the Sun, the precise time from noon one day to noon the next is 3 minutes 56 seconds longer and this makes a day almost precisely twenty-four hours in length.
The actual time from noon to noon differs depending where the Earth is on its celestial course around the Sun, but if you average the days in a year out, it comes to precisely twenty-four hours.
A YEAR: All nine planets in our solar system move around the Sun in almost perfectly circular routes called orbits. Each journey around the Sun is called a revolution and all the planets orbit around the Sun in the same direction. The direction the Earth takes can be verified by noting its position against the background stars.
Since you cannot see the Sun and the stars at the same time, it is obligatory to note the location of the Sun in the morning and the see which stars appear there in the night. You will see that the Sun appears to pass through the twelve constellations of the zodiac during a year.
Earth’s journey around the Sun, which seems like the Sun travelling through the zodiac takes about 365.25 days. This is different from year to year, so astronomers add or delete a second in some years to keep their time accurate with the Earth’s motion.
THE SEASONS: The seasons indicate the change in the pattern of daylight over the course of a year. Because the Earth is tilted off centre, different parts of it receive different amounts of sunlight on different stages of its path around the Sun, a path that we call a year. So, between approximately the 21st September and late March, the Earth’s Northern Hemisphere is tilted away from the Sun, which creates Autumn and Winter, giving less than twelve hours of daylight per day.
From April to the 20th September, the Northern Hemisphere receives more than twelve hours of daylight a day, producing Spring and Summer. The exact opposite occurs in the Southern Hemisphere.
The Equinoxes take place at the points in the year when there is exactly twelve hours of sunlight and darkness in the day. So, the vernal or Spring equinox is on or around the 21st March and the autumnal equinox is on or around the 21st September. Summer officially commences on the day with the greatest amount of daylight, the 21st June or summer solstice.
The winter solstice occurs on the shortest day, the 21st December. ‘Solstice’ is a combination of two words meaning ’sun standing still’ and the days are so called because they are the days when the apparent movement of the Sun reaches its extremes and reverses direction again.
Owen Jones, the author of this article, writes on many subjects, but is currently involved with researching Franklin planner pages. If you have an interest in calendars, organizers or promotional calendars, please go over to our web site now at Promotional Desk Calendars
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