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Leap Year & Day

Date - February 29, 2008 - Generally Every 4 years

 
 

 


 


 

 

 

Additional Information and Links:

Leap Year / Leap Day  Lots of information and links

Leap Year from Eric Weisstein's World of Astronomy

Leap Year  History and about

Honor Society of Leap Year Day Babies

Why Leap Years?

 

 

About This Holiday

In the Gregorian calendar (used by most countries), Leap Day is the extra day in Leap Year that occurs every 4 years. The next leap day is February 29, 2008. Leap years are every year that is divisible by 4, except years that are divisible by 100, unless the year is also divisible by 400. Sound confusing? Then all you need to know is that leap year is every 4 years skipping the years 2100, 2200, 2300, 2500, etc.

Leap years are required so that the calendar stays in alignment with the earth's motion around the sun. This alignment,  calculated by the mean time between two successive vernal equinoxes, is 365.2422 days long, resulting in an error of .2422 days in a 365 day calendar year. After 100 years, the calendar would be more than 24 days ahead of the seasons. Leap years keep the calendar in line with the seasons.

 

 


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The vernal equinox is time when the sun is directly above the Earth's equator, appearantly moving from the southern to the northern hemisphere.

The mean time between two successive vernal equinoxes is called a tropical year, and it is about 365.2422 days long.

Using a calendar with 365 days would result in an error of 0.2422 days or almost 6 hours per year. After 100 years, this calendar would be more than 24 days ahead of the seasons (tropical year), which is not a desirable situation. It is desirable to align the calendar with the seasons, and make the difference as small as possible.

By adding leap years approximately every 4th year, this difference between the calendar and the seasons can be reduced significantly, and the calendar will follow the seasons much more closely than without leap years.

(One day is here used in the sense of "mean solar day", which is the mean time between two transits of the sun across the meridian of the observer.)