Q88080747
star in the constellation Orion
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Q88080747
Summary
Q88080747 is a star[1].
Key Facts
- Q88080747's instance of is recorded as star[2].
- Q88080747's constellation is recorded as Orion[3].
- Q88080747's spectral class is recorded as F2[4].
- Q88080747's catalog code is recorded as 2MASS J06054227+1328049[5].
- Q88080747's catalog code is recorded as AG+13 528[6].
- Q88080747's catalog code is recorded as BD+13 1103[7].
- Q88080747's catalog code is recorded as GSC 00729-01622[8].
- Q88080747's catalog code is recorded as PPM 121889[9].
- Q88080747's catalog code is recorded as SAO 95221[10].
- Q88080747's catalog code is recorded as TYC 729-1622-1[11].
- Q88080747's catalog code is recorded as YZ 13 1998[12].
- Q88080747's catalog code is recorded as Gaia DR2 3345056049231540096[13].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.685'}[14].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.422'}[15].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.354'}[16].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.67'}[17].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.34'}[18].
- Q88080747's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.5632'}[19].
- Q88080747's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.1881'}[20].
- Q88080747's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+28.47'}[21].
- Q88080747's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+192.7488'}[22].
- Q88080747's SIMBAD ID is recorded as BD+13 1103[23].
- Q88080747's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+91.42613115964170'}[24].
- Q88080747's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+13.46805057941770'}[25].
- Q88080747's epoch is recorded as J2000.0[26].