Q90858782

Summary

Q90858782 is a high proper-motion star^[1].

Key Facts

• Q90858782's instance of is recorded as high proper-motion star^[2].
• Q90858782's constellation is recorded as Capricornus^[3].
• Q90858782's spectral class is recorded as F7V^[4].
• Q90858782's catalog code is recorded as BD-21 6009^[5].
• Q90858782's catalog code is recorded as CPD-20 8152^[6].
• Q90858782's catalog code is recorded as GSC 06368-01157^[7].
• Q90858782's catalog code is recorded as HD 203770^[8].
• Q90858782's catalog code is recorded as PPM 272446^[9].
• Q90858782's catalog code is recorded as SAO 190307^[10].
• Q90858782's catalog code is recorded as TYC 6368-1157-1^[11].
• Q90858782's catalog code is recorded as YZ 110 9168^[12].
• Q90858782's catalog code is recorded as 2MASS J21244658-2023261^[13].
• Q90858782's catalog code is recorded as Gaia DR1 6829413581675881984^[14].
• Q90858782's catalog code is recorded as Gaia DR2 6829413585971488128^[15].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.11'}^[16].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.075'}^[17].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.819'}^[18].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.795'}^[19].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.55'}^[20].
• Q90858782's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8804'}^[21].
• Q90858782's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.7971'}^[22].
• Q90858782's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.44'}^[23].
• Q90858782's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+172.5000'}^[24].
• Q90858782's SIMBAD ID is recorded as HD 203770^[25].
• Q90858782's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+321.19414058904050'}^[26].