Q87119145
white dwarf in the constellation Cetus
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Q87119145
Summary
Q87119145 is a white dwarf[1].
Key Facts
- Q87119145's instance of is recorded as white dwarf[2].
- Q87119145's constellation is recorded as Cetus[3].
- Q87119145's spectral class is recorded as DABH:[4].
- Q87119145's catalog code is recorded as SDSS J002633.19-002230.2[5].
- Q87119145's catalog code is recorded as WD 0023-006[6].
- Q87119145's catalog code is recorded as Gaia DR2 2543512549320571008[7].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.09'}[8].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.653'}[9].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.550'}[10].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.550'}[11].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.47'}[12].
- Q87119145's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.5636'}[13].
- Q87119145's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.3844'}[14].
- Q87119145's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+6.63829886840760'}[15].
- Q87119145's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-0.37506028601510'}[16].
- Q87119145's epoch is recorded as J2000.0[17].
- Q87119145's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+7486'}[18].
- Q87119145's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+145000000'}[19].
- Q87119145's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.792'}[20].
- Q87119145's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.182'}[21].
Body
Definition and Type
Q87119145's instance of is recorded as white dwarf[2].