Q91798089
eclipsing binary star
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Q91798089
Summary
Q91798089 is an eclipsing binary star[1].
Key Facts
- Q91798089's instance of is recorded as eclipsing binary star[2].
- Q91798089's instance of is recorded as near-infrared source[3].
- Q91798089's constellation is recorded as Draco[4].
- Q91798089's spectral class is recorded as G0[5].
- Q91798089's catalog code is recorded as AG+66 624[6].
- Q91798089's catalog code is recorded as BD+67 803[7].
- Q91798089's catalog code is recorded as GSC 04177-00901[8].
- Q91798089's catalog code is recorded as PPM 18753[9].
- Q91798089's catalog code is recorded as 2MASS J13495623+6628276[10].
- Q91798089's catalog code is recorded as Gaia DR1 1672152092569285120[11].
- Q91798089's catalog code is recorded as Gaia DR2 1672152096865024512[12].
- Q91798089's catalog code is recorded as V462 Dra[13].
- Q91798089's catalog code is recorded as Gaia DR3 1672152096865024512[14].
- Q91798089's catalog code is recorded as TIC 154067797[15].
- Q91798089's catalog code is recorded as TYC 4177-901-1[16].
- Q91798089's type of variable star is recorded as W Ursae Majoris variable[17].
- Q91798089's type of variable star is recorded as eclipsing binary star[18].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.68'}[19].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.459'}[20].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.153'}[21].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.088'}[22].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.22'}[23].
- Q91798089's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.528978'}[24].
- Q91798089's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.2959'}[25].
- Q91798089's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+31.76'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2] and near-infrared source[3].