HD119277
star in the constellation Centaurus
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HD119277
Summary
HD119277 is a star[1].
Key Facts
- HD119277's instance of is recorded as star[2].
- HD119277's constellation is recorded as Centaurus[3].
- HD119277's spectral class is recorded as ApSi[4].
- HD119277's catalog code is recorded as HD 119277[5].
- HD119277's catalog code is recorded as GSC 07789-01104[6].
- HD119277's catalog code is recorded as 2MASS J13430072-3820084[7].
- HD119277's catalog code is recorded as SAO 204760[8].
- HD119277's catalog code is recorded as CD-37 8842[9].
- HD119277's catalog code is recorded as CPC 18 6592[10].
- HD119277's catalog code is recorded as CPD-37 5771[11].
- HD119277's catalog code is recorded as PPM 291723[12].
- HD119277's catalog code is recorded as TD1 16998[13].
- HD119277's catalog code is recorded as TYC 7789-1104-1[14].
- HD119277's catalog code is recorded as Gaia DR2 6115171824705184640[15].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.74'}[16].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.83'}[17].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7863'}[18].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.982'}[19].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.053'}[20].
- HD119277's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.053'}[21].
- HD119277's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3132'}[22].
- HD119277's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+761.4986'}[23].
- HD119277's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+205.75299561667580'}[24].
- HD119277's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-38.33568902231440'}[25].
- HD119277's epoch is recorded as J2000.0[26].
Body
Definition and Type
HD119277's instance of is recorded as star[2].