Q88545058
high proper-motion star in the constellation Cepheus
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Q88545058
Summary
Q88545058 is a high proper-motion star[1].
Key Facts
- Q88545058's instance of is recorded as high proper-motion star[2].
- Q88545058's instance of is recorded as near-infrared source[3].
- Q88545058's constellation is recorded as Cepheus[4].
- Q88545058's spectral class is recorded as dM4.0[5].
- Q88545058's child astronomical body is recorded as G 264-012 c[6].
- Q88545058's child astronomical body is recorded as G 264-012 b[7].
- Q88545058's catalog code is recorded as Karmn J21466+668[8].
- Q88545058's catalog code is recorded as LSPM J2146+6648[9].
- Q88545058's catalog code is recorded as NLTT 52122[10].
- Q88545058's catalog code is recorded as ASCC 95826[11].
- Q88545058's catalog code is recorded as 2MASS J21464021+6648105[12].
- Q88545058's catalog code is recorded as UCAC4 785-036345[13].
- Q88545058's catalog code is recorded as PM J21466+6648S[14].
- Q88545058's catalog code is recorded as Gaia DR2 2222540228723911168[15].
- Q88545058's catalog code is recorded as Gaia DR3 2222540228723911168[16].
- Q88545058's catalog code is recorded as TIC 322391844[17].
- Q88545058's type of variable star is recorded as rotating variable star[18].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.66'}[19].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.740'}[20].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.793'}[21].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.486'}[22].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.963'}[23].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.837'}[24].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.258'}[25].
- Q88545058's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.986'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and near-infrared source[3].