Q86843909
rotating variable star in the constellation Lyra
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Q86843909
Summary
Q86843909 is a rotating variable star[1].
Key Facts
- Q86843909's instance of is recorded as rotating variable star[2].
- Q86843909's instance of is recorded as star[3].
- Q86843909's instance of is recorded as near-infrared source[4].
- Q86843909's instance of is recorded as eruptive variable star[5].
- Q86843909's constellation is recorded as Lyra[6].
- Q86843909's child astronomical body is recorded as Q28503826[7].
- Q86843909's child astronomical body is recorded as Q28503827[8].
- Q86843909's child astronomical body is recorded as Q28503828[9].
- Q86843909's catalog code is recorded as Gaia DR2 2102911576914748032[10].
- Q86843909's catalog code is recorded as KIC 7434875[11].
- Q86843909's catalog code is recorded as 2MASS J19143420+4302214[12].
- Q86843909's catalog code is recorded as Kepler-247[13].
- Q86843909's catalog code is recorded as KOI-884[14].
- Q86843909's catalog code is recorded as UCAC4 666-073760[15].
- Q86843909's catalog code is recorded as Gaia DR3 2102911581215700096[16].
- Q86843909's catalog code is recorded as TIC 158792051[17].
- Q86843909's catalog code is recorded as SPOCS 3691[18].
- Q86843909's type of variable star is recorded as rotating variable star[19].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.597'}[20].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.178'}[21].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.051'}[22].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.031876'}[23].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.833'}[24].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.117'}[25].
- Q86843909's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.752'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].