Q89389045
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Q89389045
Summary
Q89389045 is an eclipsing binary star[1].
Key Facts
- Q89389045's instance of is recorded as eclipsing binary star[2].
- Q89389045's instance of is recorded as eclipsing binary candidate[3].
- Q89389045's instance of is recorded as near-infrared source[4].
- Q89389045's constellation is recorded as Puppis[5].
- Q89389045's spectral class is recorded as B8[6].
- Q89389045's catalog code is recorded as CSV 1053[7].
- Q89389045's catalog code is recorded as GSC 05979-03207[8].
- Q89389045's catalog code is recorded as 2MASS J07284105-1635021[9].
- Q89389045's catalog code is recorded as Gaia DR1 3028178992831239296[10].
- Q89389045's catalog code is recorded as Gaia DR2 3028178992831239296[11].
- Q89389045's catalog code is recorded as GU Pup[12].
- Q89389045's catalog code is recorded as TYC 5979-3207-1[13].
- Q89389045's catalog code is recorded as ASAS J072841-1635.0[14].
- Q89389045's catalog code is recorded as TIC 50216192[15].
- Q89389045's catalog code is recorded as Gaia DR3 3028178992831239296[16].
- Q89389045's type of variable star is recorded as eclipsing binary star[17].
- Q89389045's type of variable star is recorded as W Ursae Majoris variable[18].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.688'}[19].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.627'}[20].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.554'}[21].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.70'}[22].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.75'}[23].
- Q89389045's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.56039'}[24].
- Q89389045's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4308'}[25].
- Q89389045's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2321.263'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], eclipsing binary candidate[3], and near-infrared source[4].