Q94487938
rotating variable star in the constellation Lyra
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Q94487938
Summary
Q94487938 is a rotating variable star[1].
Key Facts
- Q94487938's instance of is recorded as rotating variable star[2].
- Q94487938's instance of is recorded as star[3].
- Q94487938's instance of is recorded as double star[4].
- Q94487938's instance of is recorded as near-infrared source[5].
- Q94487938's constellation is recorded as Lyra[6].
- Q94487938's spectral class is recorded as M1V[7].
- Q94487938's child astronomical body is recorded as Q76100069[8].
- Q94487938's catalog code is recorded as WDS J19251+4044AB[9].
- Q94487938's catalog code is recorded as Gaia DR2 2101508501301083520[10].
- Q94487938's catalog code is recorded as KIC 5531953[11].
- Q94487938's catalog code is recorded as 2MASS J19250840+4043481[12].
- Q94487938's catalog code is recorded as KOI-1681[13].
- Q94487938's catalog code is recorded as Kepler-1984[14].
- Q94487938's catalog code is recorded as Gaia DR3 2101508501301083520[15].
- Q94487938's catalog code is recorded as TIC 137089954[16].
- Q94487938's type of variable star is recorded as rotating variable star[17].
- Q94487938's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.465'}[18].
- Q94487938's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.847'}[19].
- Q94487938's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.580'}[20].
- Q94487938's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.02022'}[21].
- Q94487938's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.19'}[22].
- Q94487938's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.11'}[23].
- Q94487938's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.45'}[24].
- Q94487938's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+0.071871'}[25].
- Q94487938's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1.99285996'}[26].