Q78797211
star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
Q78797211
Summary
Q78797211 is a star[1].
Key Facts
- Q78797211's instance of is recorded as star[2].
- Q78797211's constellation is recorded as Orion[3].
- Q78797211's spectral class is recorded as G5[4].
- Q78797211's catalog code is recorded as 2MASS J06171731+0543066[5].
- Q78797211's catalog code is recorded as AG+05 745[6].
- Q78797211's catalog code is recorded as BD+05 1167[7].
- Q78797211's catalog code is recorded as GSC 00144-01665[8].
- Q78797211's catalog code is recorded as HD 43585[9].
- Q78797211's catalog code is recorded as PPM 150227[10].
- Q78797211's catalog code is recorded as SAO 113682[11].
- Q78797211's catalog code is recorded as TYC 144-1665-1[12].
- Q78797211's catalog code is recorded as YZ 5 2769[13].
- Q78797211's catalog code is recorded as Gaia DR1 3318006890658531584[14].
- Q78797211's catalog code is recorded as Gaia DR2 3318006894957054592[15].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.053'}[16].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.557'}[17].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.441'}[18].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.70'}[19].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.68'}[20].
- Q78797211's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.4632'}[21].
- Q78797211's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.1529'}[22].
- Q78797211's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.02'}[23].
- Q78797211's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+240.7956'}[24].
- Q78797211's SIMBAD ID is recorded as HD 43585[25].
- Q78797211's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+94.32207505774900'}[26].