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Geometry of a total solar eclipse (not to scale) The diagrams to the right show the alignment of the Sun, Moon, and Earth during a solar eclipse. The dark gray region between the Moon and Earth is the umbra, where the Sun is completely obscured by the Moon. The small area where the umbra touches Earth's surface is where a total eclipse can be seen.
A painting by Lucien Rudaux showing how a solar eclipse might appear when viewed from the lunar surface. [1] A simulation of the start and end of the August 28, 2007 lunar eclipse, viewed from the center of the Moon. [2] Solar eclipses on the Moon are caused when the planet Earth passes in front of the Sun and blocks its light.
English: A diagram illustrating the difference between a full moon and a lunar eclipse, and the difference between a new moon and a solar eclipse. This is caused by the 5° incline of the moon's orbital plane around earth, meaning that an eclipse can only happen when the moon is nearly in line with the nodal line.
A lunar eclipse appears when the Earth stands between the moon and the sun. This blocks the sunlight from the moon, making it appear in hues of orange, brown, red — or even, black out entirely.
The term eclipse is most often used to describe either a solar eclipse, when the Moon's shadow crosses the Earth's surface, or a lunar eclipse, when the Moon moves into the Earth's shadow. However, it can also refer to such events beyond the Earth–Moon system: for example, a planet moving into the shadow cast by one of its moons, a moon ...
The rarity of today's event has many curious about the nature of eclipses and the difference between the two kinds.
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A painting by Lucien Rudaux showing how a solar eclipse might appear when viewed from the lunar surface. The Moon's surface appears red because the only sunlight available is refracted through Earth's atmosphere on the edges of Earth, as shown in the sky in this painting. A lunar eclipse is on the Moon a solar eclipse. The occurrence makes ...
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