Q85833972
rotating variable star in the constellation Lyra
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Q85833972
Summary
Q85833972 is a rotating variable star[1].
Key Facts
- Q85833972's instance of is recorded as rotating variable star[2].
- Q85833972's instance of is recorded as star[3].
- Q85833972's instance of is recorded as near-infrared source[4].
- Q85833972's instance of is recorded as eruptive variable star[5].
- Q85833972's constellation is recorded as Lyra[6].
- Q85833972's spectral class is recorded as F2[7].
- Q85833972's child astronomical body is recorded as Q28502942[8].
- Q85833972's child astronomical body is recorded as Q28502940[9].
- Q85833972's child astronomical body is recorded as Kepler-184 d[10].
- Q85833972's catalog code is recorded as Gaia DR2 2125831210335846016[11].
- Q85833972's catalog code is recorded as 2MASS J19274845+4304289[12].
- Q85833972's catalog code is recorded as KIC 7445445[13].
- Q85833972's catalog code is recorded as Kepler-184[14].
- Q85833972's catalog code is recorded as KOI-567[15].
- Q85833972's catalog code is recorded as UCAC4 666-076091[16].
- Q85833972's catalog code is recorded as Gaia DR3 2125831210335846016[17].
- Q85833972's catalog code is recorded as TIC 63119782[18].
- Q85833972's type of variable star is recorded as rotating variable star[19].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.100'}[20].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.752'}[21].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.690'}[22].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.299555'}[23].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.098'}[24].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.276'}[25].
- Q85833972's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.753'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].