Q88019801
star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
Q88019801
Summary
Q88019801 is a star[1].
Key Facts
- Q88019801's instance of is recorded as star[2].
- Q88019801's constellation is recorded as Orion[3].
- Q88019801's spectral class is recorded as G6V[4].
- Q88019801's catalog code is recorded as 2MASS J05373655-1023513[5].
- Q88019801's catalog code is recorded as BD-10 1240[6].
- Q88019801's catalog code is recorded as GSC 05350-00435[7].
- Q88019801's catalog code is recorded as HD 37359[8].
- Q88019801's catalog code is recorded as PPM 216043[9].
- Q88019801's catalog code is recorded as SAO 150627[10].
- Q88019801's catalog code is recorded as SKY# 9122[11].
- Q88019801's catalog code is recorded as TYC 5350-435-1[12].
- Q88019801's catalog code is recorded as YZC 11 1535[13].
- Q88019801's catalog code is recorded as Gaia DR1 3010543788394290816[14].
- Q88019801's catalog code is recorded as Gaia DR2 3010543792691486592[15].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.552'}[16].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.114'}[17].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.997'}[18].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.22'}[19].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.17'}[20].
- Q88019801's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.9733'}[21].
- Q88019801's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.0196'}[22].
- Q88019801's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.82'}[23].
- Q88019801's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+331.1697'}[24].
- Q88019801's SIMBAD ID is recorded as HD 37359[25].
- Q88019801's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.40231006342690'}[26].