| Information | |
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| has gloss | eng: U Scorpii is one of only 10 known recurring nova in our galaxy. Located near the northern edge of the constellation Scorpius it normally has a magnitude of 18, but reaches a magnitude of about 8 during outbursts. Outbursts have been observed in 1863, 1906, 1936, 1979, 1987, 1999, and 2010 . The most recent outburst, on 28 Jan 2010, was predicted to occur on 2009.3 +/- 1.0 year based on observations during quiescence following the 1999 outburst. |
| lexicalization | eng: U Scorpii |
| instance of | (noun) a star that varies noticeably in brightness variable star, variable |
| Meaning | |
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| Japanese | |
| has gloss | jpn: さそり座U星 (さそりざUせい、U Scorpii) は銀河系内で知られる10個 の反復新星 (RNe)の内の一つ。さそり座の北辺付近に位置し、静穏時は19等級程だが、増光時には8等級にせまる輝きを見せる。現在までに1863年、1906年、1936年、1979年、1987年、1999年、そして近年2010年に増光が観測された。 |
| lexicalization | jpn: さそり座U星 |
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