Q87950154
star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
Q87950154
Summary
Q87950154 is a star[1].
Key Facts
- Q87950154's instance of is recorded as star[2].
- Q87950154's constellation is recorded as Orion[3].
- Q87950154's spectral class is recorded as G5[4].
- Q87950154's catalog code is recorded as 2MASS J05115397+1026324[5].
- Q87950154's catalog code is recorded as AG+10 558[6].
- Q87950154's catalog code is recorded as BD+10 728[7].
- Q87950154's catalog code is recorded as GSC 00702-01316[8].
- Q87950154's catalog code is recorded as HD 33625[9].
- Q87950154's catalog code is recorded as PPM 120695[10].
- Q87950154's catalog code is recorded as SAO 94383[11].
- Q87950154's catalog code is recorded as TYC 702-1316-1[12].
- Q87950154's catalog code is recorded as YZ 10 1547[13].
- Q87950154's catalog code is recorded as Gaia DR1 3387008220328395904[14].
- Q87950154's catalog code is recorded as Gaia DR2 3387008224624889088[15].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.617'}[16].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.091'}[17].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.928'}[18].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.68'}[19].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.86'}[20].
- Q87950154's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3611'}[21].
- Q87950154's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.0273'}[22].
- Q87950154's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+62.15'}[23].
- Q87950154's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+330.3274'}[24].
- Q87950154's SIMBAD ID is recorded as HD 33625[25].
- Q87950154's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+77.97487097834170'}[26].