Q87706616
rotating variable star in the constellation Lyra
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Q87706616
Summary
Q87706616 is a rotating variable star[1].
Key Facts
- Q87706616's instance of is recorded as rotating variable star[2].
- Q87706616's instance of is recorded as star[3].
- Q87706616's instance of is recorded as near-infrared source[4].
- Q87706616's instance of is recorded as eruptive variable star[5].
- Q87706616's constellation is recorded as Lyra[6].
- Q87706616's child astronomical body is recorded as Q28503950[7].
- Q87706616's child astronomical body is recorded as Q28503952[8].
- Q87706616's catalog code is recorded as Gaia DR2 2102509125599126144[9].
- Q87706616's catalog code is recorded as 2MASS J19113992+4226142[10].
- Q87706616's catalog code is recorded as KIC 6936909[11].
- Q87706616's catalog code is recorded as KOI-1363[12].
- Q87706616's catalog code is recorded as Kepler-291[13].
- Q87706616's catalog code is recorded as UCAC4 663-073375[14].
- Q87706616's catalog code is recorded as Gaia DR3 2102509125599126144[15].
- Q87706616's catalog code is recorded as TIC 158631683[16].
- Q87706616's catalog code is recorded as SPOCS 3645[17].
- Q87706616's type of variable star is recorded as rotating variable star[18].
- Q87706616's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.69'}[19].
- Q87706616's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.337'}[20].
- Q87706616's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.150'}[21].
- Q87706616's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.888929'}[22].
- Q87706616's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.076'}[23].
- Q87706616's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.1979871'}[24].
- Q87706616's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.03'}[25].
- Q87706616's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.2607737'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].