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eclissi - tradução para Inglês
eclissi
n. eclipse, obscuration, obscuring of one celestial body by another
solar eclipse
![Einstein]]'s theory of [[general relativity]].](https://commons.wikimedia.org/wiki/Special:FilePath/1919 eclipse positive.jpg?width=200 "Einstein]]'s theory of [[general relativity]].")
![solar eclipse on August 1, 2008]] in [[Novosibirsk]], [[Russia]]. All times UTC (local time was UTC+7). The time span between shots is three minutes.](https://commons.wikimedia.org/wiki/Special:FilePath/2008-08-01 Solar eclipse progression with timestamps.jpg?width=200 "solar eclipse on August 1, 2008]] in [[Novosibirsk]], [[Russia]]. All times UTC (local time was UTC+7). The time span between shots is three minutes.")
![''Astronomers Studying an Eclipse'' painted by [[Antoine Caron]] in 1571](https://commons.wikimedia.org/wiki/Special:FilePath/Antoine Caron Astronomers Studying an Eclipse.jpg?width=200 "''Astronomers Studying an Eclipse'' painted by [[Antoine Caron]] in 1571")
![O.S.]] 2 August)](https://commons.wikimedia.org/wiki/Special:FilePath/Course of moon shadow 2.=12. 8. 1654 figured in advance by Erhard Weigel.jpg?width=200 "O.S.]] 2 August)")
![2006 total solar eclipse]].](https://commons.wikimedia.org/wiki/Special:FilePath/Eclipse fromISS 2006-03-29.jpg?width=200 "2006 total solar 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.")
![Records of the solar eclipses of 993 and 1004 as well as the lunar eclipses of 1001 and 1002 by [[Ibn Yunus]] of Cairo (c. 1005).](https://commons.wikimedia.org/wiki/Special:FilePath/Ibn Yunus eclipses 1004 CE manuscript records Arabic.jpg?width=200 "Records of the solar eclipses of 993 and 1004 as well as the lunar eclipses of 1001 and 1002 by [[Ibn Yunus]] of Cairo (c. 1005).")
![Partial and annular phases of the [[solar eclipse of May 20, 2012]]](https://commons.wikimedia.org/wiki/Special:FilePath/Solar Eclipse May 20,2012.jpg?width=200 "Partial and annular phases of the [[solar eclipse of May 20, 2012]]")
NATURAL PHENOMENON WHEREIN THE SUN IS OBSCURED BY THE MOON
Annular eclipse; Annular Eclipse; Solar eclipses; Sun eclipse; Partial Solar Eclipse; Solar eclipse (astronomy); Eclipse of the earth; Eclipse of the Earth; Solar Eclipse; Annular solar eclipse; Total solar eclipse; Hybrid eclipse; Partial solar eclipse; Hybrid solar eclipse; Umbraphiles; Eclipse of the sun; Solar eclipses on Earth; Total eclipse of the sun; Eclipse of the Sun; Total eclipse of the Sun; Solareclipse; Umbra, penumbra, and antumbra; Totality (eclipse)
eclissi solare
total eclipse
.jpg?width=200 "The shadow of an eclipse on Earth as seen from space")
WIKIMEDIA DISAMBIGUATION PAGE
Total Eclipse (album); Total eclipse (disambiguation); Total Eclipse (disambiguation); Total Eclipse (video game)
eclissi totale
Wikipédia
Eclissi
Leclissi, o eclisse, è un evento ottico-astronomico che avviene quando un qualsiasi corpo celeste, come un pianeta o un satellite, si interpone tra una sorgente di luce, ad esempio una stella o un corpo che brilla di luce riflessa, e uno dei due corpi celesti sopracitati. Il secondo corpo quindi, entra nel cono d'ombra o di penombra del primo.
