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lunar eclipse - translation to γερμανικά
![refracts]] [[sunlight]] into the shadow cone.](https://commons.wikimedia.org/wiki/Special:FilePath/Blood Moon Corrected Labels.png?width=200 "refracts]] [[sunlight]] into the shadow cone.")
![a lunar eclipse]].](https://commons.wikimedia.org/wiki/Special:FilePath/Eclipse Christophe Colomb.jpg?width=200 "a lunar eclipse]].")
![Earth's orbital plane]]) results in the revolution of the [[lunar nodes]] relative to the Earth. This causes an [[eclipse season]] approximately every six months, in which a [[solar eclipse]] can occur at the [[new moon]] phase and a lunar eclipse can occur at the [[full moon]] phase.](https://commons.wikimedia.org/wiki/Special:FilePath/Eclipse vs new or full moons, annotated.svg?width=200 "Earth's orbital plane]]) results in the revolution of the [[lunar nodes]] relative to the Earth. This causes an [[eclipse season]] approximately every six months, in which a [[solar eclipse]] can occur at the [[new moon]] phase and a lunar eclipse can occur at the [[full moon]] phase.")
![refracted]] by Earth's atmosphere, producing a reddish color.](https://commons.wikimedia.org/wiki/Special:FilePath/Full Eclipse of the Moon as seen in from Irvine, CA, USA (52075715442) (cropped).jpg?width=200 "refracted]] by Earth's atmosphere, producing a reddish color.")
![shadow]] cast by [[Earth]]. Within the [[umbra]], the central region, the planet totally shields direct [[sunlight]]. In contrast, within the [[penumbra]], the outer portion, the sunlight is only partially blocked. (Neither the [[Sun]], [[Moon]], and Earth sizes nor the distances between the bodies are to scale.)](https://commons.wikimedia.org/wiki/Special:FilePath/Geometry of a Lunar Eclipse.svg?width=200 "shadow]] cast by [[Earth]]. Within the [[umbra]], the central region, the planet totally shields direct [[sunlight]]. In contrast, within the [[penumbra]], the outer portion, the sunlight is only partially blocked. (Neither the [[Sun]], [[Moon]], and Earth sizes nor the distances between the bodies are to scale.)")
![refracted]] by Earth's atmosphere shines on the Moon, leaving a reddish color. This can be seen in different exposures of a partial lunar eclipse, for example here with exposures of 1/80, 2/5, and 2 seconds.](https://commons.wikimedia.org/wiki/Special:FilePath/Lunar eclipse oct 8 2014 Minneapolis 4 46am.png?width=200 "refracted]] by Earth's atmosphere shines on the Moon, leaving a reddish color. This can be seen in different exposures of a partial lunar eclipse, for example here with exposures of 1/80, 2/5, and 2 seconds.")
Ορισμός
Βικιπαίδεια
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the moon to be darkened. Such alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to the plane of the Earth's orbit.
This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy) with Earth between the other two, which can happen only on the night of a full moon when the Moon is near either lunar node. The type and length of a lunar eclipse depend on the Moon's proximity to the lunar node.
When the moon is totally eclipsed by the Earth, it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon surface, as only the light reflected from the lunar surface has been refracted by Earth's atmosphere. This light appears reddish due to the Rayleigh scattering of blue light, the same reason sunrise and sunsets are more orange than during the day.
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. A total lunar eclipse can last up to nearly 2 hours, while a total solar eclipse lasts only up to a few minutes at any given place, because the Moon's shadow is smaller. Also unlike solar eclipses, lunar eclipses are safe to view without any eye protection or special precautions.
The symbol for a lunar eclipse (or indeed any body in the shadow of another) is (U+1F776 🝶).
