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maansverduistering - translation to Αγγλικά
maansverduistering
n. lunar eclipse
lunar eclipse
![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.")
WHEN THE MOON PASSES DIRECTLY BEHIND THE EARTH
Penumbral eclipse; Lunar Eclipse; Partial lunar eclipse; Total lunar eclipse; Lunar eclipses; Full lunar eclipse; Moon eclipse; Lunar elipse; Selenelion; Penumbral lunar eclipse; Eclipse of the Moon; Eclipse of the moon; Selenehelion; Horizontal eclipse; Blood Moon (eclipse); Selenelionic; 🝶; Blood Moon eclipse
maansverduistering
Βικιπαίδεια
Maansverduistering
Een maansverduistering doet zich voor wanneer de Zon, de aarde en de Maan op één lijn staan (met de aarde in het midden), oftewel als Zon en Maan in oppositie staan. Normaal weerkaatst de maan het licht van de zon naar de aarde, maar tijdens een maansverduistering staat de aarde in de weg en ontvangt de maan geen zonlicht: de maan bevindt zich in de schaduw van de aarde en wordt dus donker, ofwel verduisterd.
