Q88420756

Summary

Q88420756 is a star^[1].

Key Facts

• Q88420756's instance of is recorded as star^[2].
• Q88420756's constellation is recorded as Auriga^[3].
• Q88420756's spectral class is recorded as F8^[4].
• Q88420756's catalog code is recorded as 2MASS J05505091+4018116^[5].
• Q88420756's catalog code is recorded as AG+40 677^[6].
• Q88420756's catalog code is recorded as BD+40 1427^[7].
• Q88420756's catalog code is recorded as GSC 02916-02471^[8].
• Q88420756's catalog code is recorded as HIC 27617^[9].
• Q88420756's catalog code is recorded as HIP 27617^[10].
• Q88420756's catalog code is recorded as PPM 48492^[11].
• Q88420756's catalog code is recorded as SAO 40648^[12].
• Q88420756's catalog code is recorded as TYC 2916-2471-1^[13].
• Q88420756's catalog code is recorded as Gaia DR2 191629964594945408^[14].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.139'}^[15].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.491'}^[16].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.337'}^[17].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.45'}^[18].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.55'}^[19].
• Q88420756's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0324'}^[20].
• Q88420756's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0294'}^[21].
• Q88420756's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.20'}^[22].
• Q88420756's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+971.4397'}^[23].
• Q88420756's SIMBAD ID is recorded as BD+40 1427^[24].
• Q88420756's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+87.71210885609090'}^[25].
• Q88420756's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.30321677450490'}^[26].