Q89740181
rotating variable star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q89740181
Summary
Q89740181 is a rotating variable star[1].
Key Facts
- Q89740181's instance of is recorded as rotating variable star[2].
- Q89740181's instance of is recorded as star[3].
- Q89740181's instance of is recorded as near-infrared source[4].
- Q89740181's instance of is recorded as eruptive variable star[5].
- Q89740181's constellation is recorded as Lyra[6].
- Q89740181's spectral class is recorded as G5Ib[7].
- Q89740181's child astronomical body is recorded as Q22252981[8].
- Q89740181's child astronomical body is recorded as Q22257075[9].
- Q89740181's catalog code is recorded as SPOCS 3043[10].
- Q89740181's catalog code is recorded as Gaia DR2 2101243789577188736[11].
- Q89740181's catalog code is recorded as KIC 4914423[12].
- Q89740181's catalog code is recorded as 2MASS J19155629+4003522[13].
- Q89740181's catalog code is recorded as Gaia DR1 2101243789577188736[14].
- Q89740181's catalog code is recorded as KOI-108[15].
- Q89740181's catalog code is recorded as Kepler-103[16].
- Q89740181's catalog code is recorded as UCAC4 651-069176[17].
- Q89740181's catalog code is recorded as Gaia DR3 2101243789577188736[18].
- Q89740181's catalog code is recorded as TIC 121865656[19].
- Q89740181's catalog code is recorded as TYC 3125-2038-1[20].
- Q89740181's type of variable star is recorded as rotating variable star[21].
- Q89740181's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.193'}[22].
- Q89740181's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.941'}[23].
- Q89740181's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.873'}[24].
- Q89740181's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.239382'}[25].
- Q89740181's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.199'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].