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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.
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.
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.
A partial lunar eclipse of the Harvest Moon, in tandem with a supermoon, lit up the skies Tuesday night in Fresno, a video shows. Supermoons appear larger that regular full moons because they ...
This eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950 ...
Sky gazers can expect slightly better conditions as they go northeast along the path of totality. In Burlington, Vt. , the forecast is for mostly sunny skies with a high of 62 degrees.
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]