Q89375206
Algol variable in the constellation Fornax
Press Enter · cited answer in seconds
0 sources
Q89375206
Summary
Q89375206 is an eclipsing binary star[1].
Key Facts
- Q89375206's instance of is recorded as eclipsing binary star[2].
- Q89375206's instance of is recorded as near-infrared source[3].
- Q89375206's constellation is recorded as Fornax[4].
- Q89375206's spectral class is recorded as A2/3V[5].
- Q89375206's catalog code is recorded as 2MASS J02510940-3804527[6].
- Q89375206's catalog code is recorded as CPC 18 921[7].
- Q89375206's catalog code is recorded as CSV 252[8].
- Q89375206's catalog code is recorded as GSC 07559-00856[9].
- Q89375206's catalog code is recorded as HD 17886[10].
- Q89375206's catalog code is recorded as NSV 969[11].
- Q89375206's catalog code is recorded as PPM 278425[12].
- Q89375206's catalog code is recorded as Gaia DR1 5045577014967354496[13].
- Q89375206's catalog code is recorded as Gaia DR2 5045577019264318720[14].
- Q89375206's catalog code is recorded as AT For[15].
- Q89375206's catalog code is recorded as TYC 7559-856-1[16].
- Q89375206's catalog code is recorded as TIC 215336287[17].
- Q89375206's catalog code is recorded as Gaia DR3 5045577019264318720[18].
- Q89375206's type of variable star is recorded as eclipsing binary star[19].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.679'}[20].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.407'}[21].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.283'}[22].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.32'}[23].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.49'}[24].
- Q89375206's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.264936'}[25].
- Q89375206's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.9594'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2] and near-infrared source[3].