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But the shading in the outer part of the penumbra is extremely slight. The eclipse technically begins when the Moon’s edge first enters the penumbra, or pale outer fringe, of Earth’s shadow. The world map at right tells the story.Ī total lunar eclipse goes through five distinct stages. Europe and West Africa see the eclipse high in the sky during the dark morning hours of the 21st, and in the rest of Africa, the Middle East, and Central Asia, the eclipse will still be under way when the Moon sets and the Sun rises on the 21st. This means that on the West Coast and in Alaska and Hawaii, the eclipse will already be in progress when the Sun sets and the Moon rises on the evening of the 20th.
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In Europe and Africa, the eclipse occurs on the morning of the 21st.
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Observing prospects for Americans couldn't be better during February 20th's total lunar eclipse. Unlike a solar eclipse, each stage of a lunar eclipse is visible to everyone on the Moon-facing side of Earth at once we’re all looking together. The partial phases of the eclipse last for about an hour and a quarter before and after totality. Pacific Standard Time, as shown at lower right. Eastern Standard Time, or 7:00 to 7:52 p.m. In the time zones of Europe and West Africa, the eclipse happens during the early-morning hours of Thursday, the 21st.Įarth’s shadow will totally engulf the Moon from 10:00 to 10:52 p.m. In the Americas, the eclipse happens during convenient evening hours on Wednesday, the 20th, when people are up and about. Skywatchers in nearly the entire Western Hemisphere will get an excellent view. The full Moon is going to get totally eclipsed on the night of February 20–21, putting on a gorgeous show as it glides through Earth's shadow. For best results see our lunar eclipse photography guide. Use a long lens and a tripod for your camera if you have an SLR, or just point any digital camera into a telescope. The last sunlit rim of the Moon was about to slip into the Earth's red shadow when Dennis di Cicco of Sky & Telescope took this picture on Aug.
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