Q78796975

Summary

Q78796975 is a star^[1].

Key Facts

• Q78796975's instance of is recorded as star^[2].
• Q78796975's constellation is recorded as Orion^[3].
• Q78796975's spectral class is recorded as K5^[4].
• Q78796975's catalog code is recorded as 2MASS J06121484-0018222^[5].
• Q78796975's catalog code is recorded as AG-00 751^[6].
• Q78796975's catalog code is recorded as BD-00 1211^[7].
• Q78796975's catalog code is recorded as GSC 04783-00791^[8].
• Q78796975's catalog code is recorded as HD 291296^[9].
• Q78796975's catalog code is recorded as PPM 176157^[10].
• Q78796975's catalog code is recorded as SAO 132950^[11].
• Q78796975's catalog code is recorded as TYC 4783-791-1^[12].
• Q78796975's catalog code is recorded as YZ 90 1580^[13].
• Q78796975's catalog code is recorded as Gaia DR2 3121534543713388800^[14].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.10'}^[15].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.49'}^[16].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.689'}^[17].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.979'}^[18].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.820'}^[19].
• Q78796975's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6357'}^[20].
• Q78796975's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0903'}^[21].
• Q78796975's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+31.61'}^[22].
• Q78796975's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+478.4002'}^[23].
• Q78796975's SIMBAD ID is recorded as HD 291296^[24].
• Q78796975's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+93.06188122758870'}^[25].
• Q78796975's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-0.30618302894320'}^[26].