Q89662293
star in the constellation Cepheus
Press Enter · cited answer in seconds
0 sources
Q89662293
Summary
Q89662293 is a star[1].
Key Facts
- Q89662293's instance of is recorded as star[2].
- Q89662293's constellation is recorded as Cepheus[3].
- Q89662293's spectral class is recorded as K5[4].
- Q89662293's catalog code is recorded as 2MASS J00185688+6825186[5].
- Q89662293's catalog code is recorded as AG+68 20[6].
- Q89662293's catalog code is recorded as BD+67 20[7].
- Q89662293's catalog code is recorded as GSC 04294-00786[8].
- Q89662293's catalog code is recorded as IRAS 00161+6808[9].
- Q89662293's catalog code is recorded as PPM 12092[10].
- Q89662293's catalog code is recorded as SAO 11100[11].
- Q89662293's catalog code is recorded as SKY# 556[12].
- Q89662293's catalog code is recorded as TYC 4294-786-1[13].
- Q89662293's catalog code is recorded as Gaia DR1 530324763367148800[14].
- Q89662293's catalog code is recorded as Gaia DR2 530324767665242752[15].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.04'}[16].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.72'}[17].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.957'}[18].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.186'}[19].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.865'}[20].
- Q89662293's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.3303'}[21].
- Q89662293's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.3234'}[22].
- Q89662293's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.16'}[23].
- Q89662293's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+430.4037'}[24].
- Q89662293's SIMBAD ID is recorded as BD+67 20[25].
- Q89662293's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.73699117045020'}[26].