Traduction et analyse de mots par intelligence artificielle ChatGPT
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fuzzy conjunction - traduction vers russe
![Paranal]], the [[Moon]] shines along with two bright companions: [[Venus]] and [[Jupiter]].](https://commons.wikimedia.org/wiki/Special:FilePath/ESO’s Very Large Telescope (VLT) observatory at Paranal.jpg?width=200 "Paranal]], the [[Moon]] shines along with two bright companions: [[Venus]] and [[Jupiter]].")
![Talitha Borealis]] in conjunction with the comet [[C/2020 F3 (NEOWISE)]] on 18 July 2020 21:30 UTC with an attitude von 17° above the north horizon of [[Berlin]] (image height = 4°). At the lower edge of the picture, a bit left from the centre there is the neighbour star [[Alkaphrah]] (Kappa Ursae Majoris respectively ''Talitha Australis''). The distance between Talitha Borealis and C/2020 F3 was seven [[arc minute]]s.](https://commons.wikimedia.org/wiki/Special:FilePath/C2020F3.P1023630.jpg?width=200 "Talitha Borealis]] in conjunction with the comet [[C/2020 F3 (NEOWISE)]] on 18 July 2020 21:30 UTC with an attitude von 17° above the north horizon of [[Berlin]] (image height = 4°). At the lower edge of the picture, a bit left from the centre there is the neighbour star [[Alkaphrah]] (Kappa Ursae Majoris respectively ''Talitha Australis''). The distance between Talitha Borealis and C/2020 F3 was seven [[arc minute]]s.")
![objective]] with a [[focal length]] of 75 millimetres](https://commons.wikimedia.org/wiki/Special:FilePath/Konjunktion Pallas-Sirius am 9 Oktober 2022 mit kurzer Brennweite beschriftet.png?width=200 "objective]] with a [[focal length]] of 75 millimetres")
![objective]] with a [[focal length]] of 300 millimetres](https://commons.wikimedia.org/wiki/Special:FilePath/Konjunktion Pallas-Sirius am 9 Oktober 2022 mit langer Brennweite beschriftet.png?width=200 "objective]] with a [[focal length]] of 300 millimetres")
математика
нечеткая конъюнкция
общая лексика
нечёткое множество
математика
размытое (нечеткое) множество
Смотрите также
математика
нечеткая категория
Définition
Wikipédia
In astronomy, a conjunction occurs when two astronomical objects or spacecraft have either the same right ascension or the same ecliptic longitude, usually as observed from Earth.
When two objects always appear close to the ecliptic—such as two planets, the Moon and a planet, or the Sun and a planet—this fact implies an apparent close approach between the objects as seen in the sky. A related word, appulse, is the minimum apparent separation in the sky of two astronomical objects.
Conjunctions involve either two objects in the Solar System or one object in the Solar System and a more distant object, such as a star. A conjunction is an apparent phenomenon caused by the observer's perspective: the two objects involved are not actually close to one another in space. Conjunctions between two bright objects close to the ecliptic, such as two bright planets, can be seen with the naked eye.
The astronomical symbol for conjunction is (Unicode U+260C ☌). The conjunction symbol is not used in modern astronomy. It continues to be used in astrology.
