Q97318152
star
Press Enter · cited answer in seconds
0 sources
Q97318152
Summary
Q97318152 is a long-period variable star[1].
Key Facts
- Q97318152's instance of is recorded as long-period variable star[2].
- Q97318152's instance of is recorded as near-infrared source[3].
- Q97318152's constellation is recorded as Pegasus[4].
- Q97318152's spectral class is recorded as K0[5].
- Q97318152's catalog code is recorded as AG+12 2694[6].
- Q97318152's catalog code is recorded as BD+11 4890[7].
- Q97318152's catalog code is recorded as GSC 01156-01088[8].
- Q97318152's catalog code is recorded as HIC 112919[9].
- Q97318152's catalog code is recorded as HIP 112919[10].
- Q97318152's catalog code is recorded as PPM 141924[11].
- Q97318152's catalog code is recorded as 2MASS J22520295+1220115[12].
- Q97318152's catalog code is recorded as Gaia DR2 2719632360513022080[13].
- Q97318152's catalog code is recorded as QZ Peg[14].
- Q97318152's catalog code is recorded as TYC 1156-1088-1[15].
- Q97318152's catalog code is recorded as TIC 456829464[16].
- Q97318152's catalog code is recorded as Gaia DR3 2719632360513022080[17].
- Q97318152's type of variable star is recorded as slow irregular variables of late spectral types[18].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.477'}[19].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.549'}[20].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.368'}[21].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.97'}[22].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.69'}[23].
- Q97318152's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.182658'}[24].
- Q97318152's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5205'}[25].
- Q97318152's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.19'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2] and near-infrared source[3].