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This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, April 2, 1950, [1] with an umbral magnitude of 1.0329. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, September 26, 1950, [1] with an umbral magnitude of 1.0783. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow.
The shadow will be traveling at an average of about 2,300 miles per hour across NY state and will only take about 10 minutes, from one side of state to the other.
Michigan's last solar eclipse was June 30, 1954. It's been a while since a total solar eclipse, which happens when the moon passes between the sun and Earth , has been visible in Michigan.
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For total and annular eclipses, the duration of the eclipse is given, as well as the location of the greatest eclipse (the point of maximum eclipse) and the path width of the total or annular eclipse. The geographical areas from which the eclipse can be seen are listed along with a chart illustrating each eclipse's respective path. [3]