Q85131922
star in the constellation Aries
Press Enter · cited answer in seconds
0 sources
Q85131922
Summary
Q85131922 is a star[1].
Key Facts
- Q85131922's instance of is recorded as star[2].
- Q85131922's constellation is recorded as Aries[3].
- Q85131922's spectral class is recorded as M1[4].
- Q85131922's catalog code is recorded as 2MASS J03223611+2452287[5].
- Q85131922's catalog code is recorded as AG+24 285[6].
- Q85131922's catalog code is recorded as BD+24 476[7].
- Q85131922's catalog code is recorded as GSC 01801-00629[8].
- Q85131922's catalog code is recorded as IRAS 03196+2441[9].
- Q85131922's catalog code is recorded as PPM 92447[10].
- Q85131922's catalog code is recorded as SAO 75898[11].
- Q85131922's catalog code is recorded as TYC 1801-629-1[12].
- Q85131922's catalog code is recorded as YZ 24 998[13].
- Q85131922's catalog code is recorded as Gaia DR1 117101115094349184[14].
- Q85131922's catalog code is recorded as Gaia DR2 117101119390875904[15].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.26'}[16].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.94'}[17].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.945'}[18].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.972'}[19].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.796'}[20].
- Q85131922's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.3458'}[21].
- Q85131922's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0920'}[22].
- Q85131922's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+21.89'}[23].
- Q85131922's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+915.7509'}[24].
- Q85131922's SIMBAD ID is recorded as BD+24 476[25].
- Q85131922's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.65044253909610'}[26].