Spring Equinox

StarDate: March 19, 2010

You are missing some Flash content that should appear here! Perhaps your browser cannot display it, or maybe it did not initialize correctly.

audio/mpeg icon

A winter that's brought record cold is about to meet its end. Spring arrives in the northern hemisphere around midday tomorrow.

That moment is known as the vernal equinox. And over the centuries, it's played an important role in the development of the calendar.

In fact, people discovered the length of the year -- and the concept of the year itself -- by following the rhythms of the seasons. Spring brought renewed life to the world after the dark winter, so it became the most important seasonal marker. Indeed, the period between vernal equinoxes defined the length of the year. This period is known as the tropical year, and it lasts 365 days, 5 hours, 48 minutes, and 45 seconds.

That extra dab of time beyond 365 days has given calendar makers fits. It's required them to add extra days, and even to revamp the entire calendar.

In ancient Rome, for example, the astronomer Sisogenes recommended adding an extra day every fourth year. Julius Caesar accepted the idea and instituted a new calendar in 46 B.C.

That worked for a while. But by the 16th century, the calendar had slipped out of sync with the equinox by about 11 days. That was a particular problem for Christians, who used the equinox to calculate the date of Easter. So Pope Gregory XIII made one more change: he dropped three leap years from every four centuries.

We still use the Gregorian calendar today -- a calendar calibrated by the vernal equinox.

Script by Damond Benningfield, Copyright 2010

For more skywatching tips, astronomy news, and much more, read StarDate magazine.

The one constant in the Universe: StarDate magazine


©2015 The University of Texas McDonald Observatory