Q90190978
star in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
Q90190978
Summary
Q90190978 is a star[1].
Key Facts
- Q90190978's instance of is recorded as star[2].
- Q90190978's constellation is recorded as Perseus[3].
- Q90190978's spectral class is recorded as K2[4].
- Q90190978's catalog code is recorded as 2MASS J02140547+5552096[5].
- Q90190978's catalog code is recorded as AG+55 224[6].
- Q90190978's catalog code is recorded as BD+55 546[7].
- Q90190978's catalog code is recorded as GSC 03690-02036[8].
- Q90190978's catalog code is recorded as HD 236956[9].
- Q90190978's catalog code is recorded as PPM 27277[10].
- Q90190978's catalog code is recorded as SAO 23056[11].
- Q90190978's catalog code is recorded as TYC 3690-2036-1[12].
- Q90190978's catalog code is recorded as YZ 55 1980[13].
- Q90190978's catalog code is recorded as Gaia DR1 456784752778464512[14].
- Q90190978's catalog code is recorded as Gaia DR2 456784757080484736[15].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.617'}[16].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.032'}[17].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.929'}[18].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.83'}[19].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.03'}[20].
- Q90190978's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4265'}[21].
- Q90190978's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.9851'}[22].
- Q90190978's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-43.54'}[23].
- Q90190978's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+503.7530'}[24].
- Q90190978's SIMBAD ID is recorded as HD 236956[25].
- Q90190978's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+33.52281383578350'}[26].