Q87706372
rotating variable star in the constellation Cygnus
Press Enter · cited answer in seconds
0 sources
Q87706372
Summary
Q87706372 is a rotating variable star[1].
Key Facts
- Q87706372's instance of is recorded as rotating variable star[2].
- Q87706372's instance of is recorded as star[3].
- Q87706372's instance of is recorded as near-infrared source[4].
- Q87706372's instance of is recorded as eruptive variable star[5].
- Q87706372's constellation is recorded as Cygnus[6].
- Q87706372's spectral class is recorded as G7V[7].
- Q87706372's child astronomical body is recorded as Q85476529[8].
- Q87706372's child astronomical body is recorded as Q93759690[9].
- Q87706372's catalog code is recorded as Gaia DR2 2073779161653824640[10].
- Q87706372's catalog code is recorded as KIC 5474613[11].
- Q87706372's catalog code is recorded as 2MASS J19532972+4037063[12].
- Q87706372's catalog code is recorded as KOI-1599[13].
- Q87706372's catalog code is recorded as Kepler-1659[14].
- Q87706372's catalog code is recorded as UCAC4 654-079868[15].
- Q87706372's catalog code is recorded as Gaia DR3 2073779161653824640[16].
- Q87706372's catalog code is recorded as TIC 170647523[17].
- Q87706372's type of variable star is recorded as rotating variable star[18].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.24'}[19].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.842378'}[20].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.63'}[21].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.266'}[22].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.991'}[23].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.866'}[24].
- Q87706372's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.869'}[25].
- Q87706372's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.2076957'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].