| Information | |
|---|---|
| has gloss | eng: FU Orionis is a variable star in the constellation of Orion, that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has since been around magnitude 9. For a long time it was considered unique, but in 1970 a similar star, V1057 Cygni, was discovered, and a number of additional examples have been discovered since then. These stars constitute the FU Orionis class of variable stars, GCVS type FU, often nicknamed FUors. These stars are pre-main sequence stars which display an extreme change in magnitude and spectral type. |
| lexicalization | eng: FU Orionis |
| instance of | e/FU Orionis star |
| Meaning | |
|---|---|
| Italian | |
| has gloss | ita: FU Orionis è una stella variabile situata nella costellazione di Orione; si trova ad una distanza di circa 1600 anni luce dal sistema solare, nella Regione di Lambda Orionis. |
| lexicalization | ita: FU Orionis |
| Russian | |
| has gloss | rus: FU Ориона (FU Ori) – неправильная переменная звезда в созвездии Ориона, прототип фуоров, жёлтый сверхгигант спектрального класса G. |
| lexicalization | rus: FU Ориона |
| Media | |
|---|---|
| media:img | FU Orionis.jpg |
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