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A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Wednesday, February 21, 1951, with an umbral magnitude of −1.0600. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 6.5 days after apogee, the Moon's apparent diameter was smaller.
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