Q86844227
rotating variable star in the constellation Lyra
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Q86844227
Summary
Q86844227 is a rotating variable star[1].
Key Facts
- Q86844227's instance of is recorded as rotating variable star[2].
- Q86844227's instance of is recorded as high proper-motion star[3].
- Q86844227's instance of is recorded as near-infrared source[4].
- Q86844227's instance of is recorded as eruptive variable star[5].
- Q86844227's constellation is recorded as Lyra[6].
- Q86844227's spectral class is recorded as K7[7].
- Q86844227's child astronomical body is recorded as Kepler-205 c[8].
- Q86844227's child astronomical body is recorded as Q28503601[9].
- Q86844227's catalog code is recorded as Gaia DR2 2104076204545773440[10].
- Q86844227's catalog code is recorded as 2MASS J19010890+4151402[11].
- Q86844227's catalog code is recorded as KIC 6425957[12].
- Q86844227's catalog code is recorded as Kepler-205[13].
- Q86844227's catalog code is recorded as KOI-663[14].
- Q86844227's catalog code is recorded as UCAC4 660-069239[15].
- Q86844227's catalog code is recorded as Gaia DR3 2104076204545773440[16].
- Q86844227's catalog code is recorded as TIC 399822422[17].
- Q86844227's type of variable star is recorded as rotating variable star[18].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.608'}[19].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.962'}[20].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.833'}[21].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.480999'}[22].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.958'}[23].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.432'}[24].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.585'}[25].
- Q86844227's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.959'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], high proper-motion star[3], near-infrared source[4], and eruptive variable star[5].