50 days to the Total Solar Eclipse!
On Monday, April 8, Hamilton will experience a total solar eclipse for the first time since January 24, 1925.
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What is a solar eclipse?
A solar eclipse happens when, at just the right moment, the Moon passes between the Sun and Earth. This only happens when it is a New Moon, the time when the Moon is directly between the Earth and the Sun. The path of the total eclipse is usually very narrow; for this eclipse, it is about 185 km wide; people outside this path will only see a partial eclipse.
Why don't we see an eclipse every month?
There are several factors that affect when we see an eclipse, and what type of eclipse we see. Simply put, the Moon's orbit around the Earth is not perectly aligned with the Earth's orbit around the Sun.
First, The Moon's path around Earth is slightly tilted compared to the Earth's orbit around the Sun (its "inclination"). The path the Moon takes means that sometimes it appears to be higher or lower than the Sun when viewed from Earth.
The Moon's orbit around the Earth is also slightly elliptical; sometimes it is a little closer to us, and sometimes it is farther from us. The Moon's closest point to the Earth (its "perigee") also changes slightly over time, completing an orbit of the Earth every 8.85 years (its "precession").
The combination of these factors means that the conditions for a solar eclipse usually occur only a couple of times a year.
The type of eclipse will depend on the combination of the factors above. If the moon appears slightly higher or lower than the Sun as it reaches the New Moon phase, we get a partial eclipse such as the one we had in Southern Ontario this past October. If the Moon is near the furthest point of its elliptical orbit (its "apogee"), we get an Annular or "Ring of Fire" eclipse. If the Moon is perfectly lined up between the Earth and Moon, and is close enough, we get a Total Solar Eclipse!
For more information on eclipses, see the following sites: