Q90189143

Summary

Q90189143 is a star^[1].

Key Facts

• Q90189143's instance of is recorded as star^[2].
• Q90189143's constellation is recorded as Gemini^[3].
• Q90189143's spectral class is recorded as K0^[4].
• Q90189143's catalog code is recorded as 2MASS J07045809+1421004^[5].
• Q90189143's catalog code is recorded as AG+14 747^[6].
• Q90189143's catalog code is recorded as BD+14 1554^[7].
• Q90189143's catalog code is recorded as GSC 00761-01303^[8].
• Q90189143's catalog code is recorded as HD 53260^[9].
• Q90189143's catalog code is recorded as PPM 123489^[10].
• Q90189143's catalog code is recorded as SAO 96460^[11].
• Q90189143's catalog code is recorded as TYC 761-1303-1^[12].
• Q90189143's catalog code is recorded as YZ 14 2681^[13].
• Q90189143's catalog code is recorded as Gaia DR2 3353664125765417344^[14].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.092'}^[15].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.599'}^[16].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.451'}^[17].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.06'}^[18].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.24'}^[19].
• Q90189143's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7083'}^[20].
• Q90189143's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2927'}^[21].
• Q90189143's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+60.25'}^[22].
• Q90189143's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+436.1670'}^[23].
• Q90189143's SIMBAD ID is recorded as HD 53260^[24].
• Q90189143's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+106.24209126581010'}^[25].
• Q90189143's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+14.35008526553460'}^[26].