Q92650122
star
Press Enter · cited answer in seconds
0 sources
Q92650122
Summary
Q92650122 is a star[1].
Key Facts
- Q92650122's instance of is recorded as star[2].
- Q92650122's constellation is recorded as Sagittarius[3].
- Q92650122's spectral class is recorded as K1/2(III)[4].
- Q92650122's catalog code is recorded as BD-20 5508[5].
- Q92650122's catalog code is recorded as CPD-20 7541[6].
- Q92650122's catalog code is recorded as GSC 06305-02155[7].
- Q92650122's catalog code is recorded as HD 181512[8].
- Q92650122's catalog code is recorded as HIC 95142[9].
- Q92650122's catalog code is recorded as HIP 95142[10].
- Q92650122's catalog code is recorded as PPM 235875[11].
- Q92650122's catalog code is recorded as SAO 162505[12].
- Q92650122's catalog code is recorded as TYC 6305-2155-1[13].
- Q92650122's catalog code is recorded as YZ 109 8247[14].
- Q92650122's catalog code is recorded as 2MASS J19212395-1953038[15].
- Q92650122's catalog code is recorded as Gaia DR1 4083365218082634496[16].
- Q92650122's catalog code is recorded as Gaia DR2 4083365222387806208[17].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.32'}[18].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.742'}[19].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.028'}[20].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.771'}[21].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.89'}[22].
- Q92650122's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8447'}[23].
- Q92650122's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9520'}[24].
- Q92650122's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+1.88'}[25].
- Q92650122's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1050.4202'}[26].
Body
Definition and Type
Q92650122's instance of is recorded as star[2].