HD158205
star in the constellation Ara
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HD158205
Summary
HD158205 is a star[1].
Key Facts
- HD158205's instance of is recorded as star[2].
- HD158205's constellation is recorded as Ara[3].
- HD158205's spectral class is recorded as ApSr(EuCr)[4].
- HD158205's catalog code is recorded as HD 158205[5].
- HD158205's catalog code is recorded as HIP 85743[6].
- HD158205's catalog code is recorded as GSC 08736-03009[7].
- HD158205's catalog code is recorded as 2MASS J17311869-5644567[8].
- HD158205's catalog code is recorded as SAO 244807[9].
- HD158205's catalog code is recorded as CD-56 6892[10].
- HD158205's catalog code is recorded as CPC 20 5598[11].
- HD158205's catalog code is recorded as CPD-56 8303[12].
- HD158205's catalog code is recorded as HIC 85743[13].
- HD158205's catalog code is recorded as PPM 346073[14].
- HD158205's catalog code is recorded as TYC 8736-3009-1[15].
- HD158205's catalog code is recorded as Gaia DR2 5919358325754283904[16].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.45'}[17].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.31'}[18].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.2676'}[19].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.938'}[20].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.937'}[21].
- HD158205's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.920'}[22].
- HD158205's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.6236'}[23].
- HD158205's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+381.1557'}[24].
- HD158205's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+262.82788189690730'}[25].
- HD158205's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-56.74907722944890'}[26].
Body
Definition and Type
HD158205's instance of is recorded as star[2].