Q93337667
Algol variable in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q93337667
Summary
Q93337667 is an eclipsing binary star[1].
Key Facts
- Q93337667's instance of is recorded as eclipsing binary star[2].
- Q93337667's instance of is recorded as star[3].
- Q93337667's instance of is recorded as near-infrared source[4].
- Q93337667's constellation is recorded as Cassiopeia[5].
- Q93337667's spectral class is recorded as B8[6].
- Q93337667's catalog code is recorded as 2MASS J00551425+6123487[7].
- Q93337667's catalog code is recorded as AG+61 82[8].
- Q93337667's catalog code is recorded as BD+60 132[9].
- Q93337667's catalog code is recorded as GSC 04017-00520[10].
- Q93337667's catalog code is recorded as PPM 12574[11].
- Q93337667's catalog code is recorded as Gaia DR1 427422878871325824[12].
- Q93337667's catalog code is recorded as Gaia DR2 427422883173470336[13].
- Q93337667's catalog code is recorded as V1060 Cas[14].
- Q93337667's catalog code is recorded as TYC 4017-520-1[15].
- Q93337667's catalog code is recorded as TIC 51955546[16].
- Q93337667's catalog code is recorded as Gaia DR3 427422883173470336[17].
- Q93337667's type of variable star is recorded as eclipsing binary star[18].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.77'}[19].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.280'}[20].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.257'}[21].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.212'}[22].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.96'}[23].
- Q93337667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.700093'}[24].
- Q93337667's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0636'}[25].
- Q93337667's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+940.203'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], and near-infrared source[4].