Q92603356
rotating variable star in the constellation Lyra
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Q92603356
Summary
Q92603356 is a rotating variable star[1].
Key Facts
- Q92603356's instance of is recorded as rotating variable star[2].
- Q92603356's instance of is recorded as star[3].
- Q92603356's instance of is recorded as near-infrared source[4].
- Q92603356's constellation is recorded as Lyra[5].
- Q92603356's spectral class is recorded as K1[6].
- Q92603356's child astronomical body is recorded as Q28855752[7].
- Q92603356's catalog code is recorded as Gaia DR2 2104705193915993216[8].
- Q92603356's catalog code is recorded as KIC 6665695[9].
- Q92603356's catalog code is recorded as KOI-561[10].
- Q92603356's catalog code is recorded as 2MASS J18480110+4210355[11].
- Q92603356's catalog code is recorded as Kepler-601[12].
- Q92603356's catalog code is recorded as Gaia DR3 2104705193915993216[13].
- Q92603356's catalog code is recorded as TIC 351801933[14].
- Q92603356's catalog code is recorded as SPOCS 3620[15].
- Q92603356's type of variable star is recorded as rotating variable star[16].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.732'}[17].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.955'}[18].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.647'}[19].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.15'}[20].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.129'}[21].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.640'}[22].
- Q92603356's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.98957'}[23].
- Q92603356's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.85'}[24].
- Q92603356's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.79'}[25].
- Q92603356's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.384'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], and near-infrared source[4].