Q90342776

Summary

Q90342776 is a high proper-motion star^[1].

Key Facts

• Q90342776's instance of is recorded as high proper-motion star^[2].
• Q90342776's constellation is recorded as Sagittarius^[3].
• Q90342776's spectral class is recorded as G0V^[4].
• Q90342776's catalog code is recorded as CD-36 13858^[5].
• Q90342776's catalog code is recorded as CPC 18 10385^[6].
• Q90342776's catalog code is recorded as CPD-36 8994^[7].
• Q90342776's catalog code is recorded as GSC 07452-01556^[8].
• Q90342776's catalog code is recorded as HD 189873^[9].
• Q90342776's catalog code is recorded as PPM 299721^[10].
• Q90342776's catalog code is recorded as SAO 211771^[11].
• Q90342776's catalog code is recorded as TYC 7452-1556-1^[12].
• Q90342776's catalog code is recorded as 2MASS J20033846-3550549^[13].
• Q90342776's catalog code is recorded as Gaia DR1 6697412194240063104^[14].
• Q90342776's catalog code is recorded as Gaia DR2 6697412194240063104^[15].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.100'}^[16].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.799'}^[17].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.749'}^[18].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.27'}^[19].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.89'}^[20].
• Q90342776's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0868'}^[21].
• Q90342776's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.3037'}^[22].
• Q90342776's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+35.75'}^[23].
• Q90342776's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+75.1671'}^[24].
• Q90342776's SIMBAD ID is recorded as HD 189873^[25].
• Q90342776's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+300.91024670004220'}^[26].