HD222701
peculiar star in the constellation Sculptor
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HD222701
Summary
HD222701 is a peculiar star[1].
Key Facts
- HD222701's instance of is recorded as peculiar star[2].
- HD222701's constellation is recorded as Sculptor[3].
- HD222701's spectral class is recorded as A5mA5-F0[4].
- HD222701's catalog code is recorded as HD 222701[5].
- HD222701's catalog code is recorded as CPC 18 12010[6].
- HD222701's catalog code is recorded as GSC 07521-01234[7].
- HD222701's catalog code is recorded as HIC 116998[8].
- HD222701's catalog code is recorded as HIP 116998[9].
- HD222701's catalog code is recorded as 2MASS J23430718-3647058[10].
- HD222701's catalog code is recorded as PPM 304099[11].
- HD222701's catalog code is recorded as SAO 214729[12].
- HD222701's catalog code is recorded as TD1 30037[13].
- HD222701's catalog code is recorded as uvby98 100222701[14].
- HD222701's catalog code is recorded as TYC 7521-1234-1[15].
- HD222701's catalog code is recorded as Gaia DR1 2311498897026990976[16].
- HD222701's catalog code is recorded as Gaia DR2 2311498901323220736[17].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.738'}[18].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.45'}[19].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.3868'}[20].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.938'}[21].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.847'}[22].
- HD222701's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.804'}[23].
- HD222701's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.2028'}[24].
- HD222701's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+161.2175'}[25].
- HD222701's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+355.77987612856290'}[26].
Body
Definition and Type
HD222701's instance of is recorded as peculiar star[2].