HD52280
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HD52280
Summary
HD52280 is a peculiar star[1].
Key Facts
- HD52280's instance of is recorded as peculiar star[2].
- HD52280's instance of is recorded as infrared source[3].
- HD52280's constellation is recorded as Volans[4].
- HD52280's spectral class is recorded as ApSrEuCr[5].
- HD52280's catalog code is recorded as HD 52280[6].
- HD52280's catalog code is recorded as CPC 21 1279[7].
- HD52280's catalog code is recorded as GSC 08916-00469[8].
- HD52280's catalog code is recorded as 2MASS J06555309-6459495[9].
- HD52280's catalog code is recorded as PPM 355705[10].
- HD52280's catalog code is recorded as SAO 249682[11].
- HD52280's catalog code is recorded as TIC 167751145[12].
- HD52280's catalog code is recorded as TYC 8916-469-1[13].
- HD52280's catalog code is recorded as Gaia DR1 5285198772329863936[14].
- HD52280's catalog code is recorded as Gaia DR2 5285198776627254784[15].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.89'}[16].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.82'}[17].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7674'}[18].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.616'}[19].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.596'}[20].
- HD52280's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.585'}[21].
- HD52280's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.1313'}[22].
- HD52280's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+469.1972'}[23].
- HD52280's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+103.97124986433980'}[24].
- HD52280's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-64.99709932267800'}[25].
- HD52280's epoch is recorded as J2000.0[26].
Body
Definition and Type
Recorded instance of include peculiar star[2] and infrared source[3].