HD48478
peculiar star in the constellation Canis Major
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HD48478
Summary
HD48478 is a peculiar star[1].
Key Facts
- HD48478's instance of is recorded as peculiar star[2].
- HD48478's constellation is recorded as Canis Major[3].
- HD48478's spectral class is recorded as ApSi[4].
- HD48478's catalog code is recorded as HD 48478[5].
- HD48478's catalog code is recorded as GSC 05386-02116[6].
- HD48478's catalog code is recorded as HIC 32183[7].
- HD48478's catalog code is recorded as HIP 32183[8].
- HD48478's catalog code is recorded as 2MASS J06430924-1146436[9].
- HD48478's catalog code is recorded as PPM 217576[10].
- HD48478's catalog code is recorded as SAO 151831[11].
- HD48478's catalog code is recorded as BD-11 1603[12].
- HD48478's catalog code is recorded as TYC 5386-2116-1[13].
- HD48478's catalog code is recorded as YZC 11 2118[14].
- HD48478's catalog code is recorded as Gaia DR1 2953491332619839872[15].
- HD48478's catalog code is recorded as Gaia DR2 2953491336921391744[16].
- HD48478's type of variable star is recorded as Alpha² Canum Venaticorum variable[17].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.34'}[18].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.18'}[19].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.2103'}[20].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.048'}[21].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.025'}[22].
- HD48478's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.011'}[23].
- HD48478's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4461'}[24].
- HD48478's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+691.5151'}[25].
- HD48478's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+100.78851060475100'}[26].
Body
Definition and Type
HD48478's instance of is recorded as peculiar star[2].