Q88717739
Mira variable star in the constellation Ophiuchus
Press Enter · cited answer in seconds
0 sources
Q88717739
Summary
Q88717739 is a Mira variable[1].
Key Facts
- Q88717739's instance of is recorded as Mira variable[2].
- Q88717739's instance of is recorded as infrared source[3].
- Q88717739's instance of is recorded as long-period variable star[4].
- Q88717739's instance of is recorded as near-infrared source[5].
- Q88717739's constellation is recorded as Ophiuchus[6].
- Q88717739's spectral class is recorded as M1e[7].
- Q88717739's catalog code is recorded as HIC 83582[8].
- Q88717739's catalog code is recorded as HIP 83582[9].
- Q88717739's catalog code is recorded as IRAS 17021-1207[10].
- Q88717739's catalog code is recorded as PPM 232579[11].
- Q88717739's catalog code is recorded as ASAS J170457-1212.1[12].
- Q88717739's catalog code is recorded as 2MASS J17045698-1212054[13].
- Q88717739's catalog code is recorded as Gaia DR2 4142542621814786944[14].
- Q88717739's catalog code is recorded as UX Oph[15].
- Q88717739's catalog code is recorded as AAVSO 1659-12[16].
- Q88717739's catalog code is recorded as TYC 5651-656-1[17].
- Q88717739's catalog code is recorded as TIC 414559475[18].
- Q88717739's catalog code is recorded as Gaia DR3 4142542621814786944[19].
- Q88717739's type of variable star is recorded as long-period variable star[20].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.898'}[21].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.052'}[22].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.522'}[23].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.65'}[24].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.58'}[25].
- Q88717739's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.192618'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], infrared source[3], long-period variable star[4], and near-infrared source[5].