HD74494
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HD74494
Summary
HD74494 is a peculiar star[1].
Key Facts
- HD74494's instance of is recorded as peculiar star[2].
- HD74494's instance of is recorded as infrared source[3].
- HD74494's constellation is recorded as Pyxis[4].
- HD74494's spectral class is recorded as ApEuCrSr[5].
- HD74494's catalog code is recorded as HD 74494[6].
- HD74494's catalog code is recorded as GSC 06575-00047[7].
- HD74494's catalog code is recorded as HIC 42825[8].
- HD74494's catalog code is recorded as HIP 42825[9].
- HD74494's catalog code is recorded as 2MASS J08433493-2431393[10].
- HD74494's catalog code is recorded as PPM 255037[11].
- HD74494's catalog code is recorded as SAO 176362[12].
- HD74494's catalog code is recorded as YZ 114 6697[13].
- HD74494's catalog code is recorded as TYC 6575-47-1[14].
- HD74494's catalog code is recorded as Gaia DR1 5653380205213933184[15].
- HD74494's catalog code is recorded as Gaia DR2 5653380205213933184[16].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.93'}[17].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.88'}[18].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8783'}[19].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.801'}[20].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.839'}[21].
- HD74494's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.862'}[22].
- HD74494's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0680'}[23].
- HD74494's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+483.5590'}[24].
- HD74494's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+130.89555402960950'}[25].
- HD74494's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-24.52757613567100'}[26].
Body
Definition and Type
Recorded instance of include peculiar star[2] and infrared source[3].