Q94528923
star in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
Q94528923
Summary
Q94528923 is a star[1].
Key Facts
- Q94528923's instance of is recorded as star[2].
- Q94528923's constellation is recorded as Perseus[3].
- Q94528923's spectral class is recorded as K1III[4].
- Q94528923's catalog code is recorded as 2MASS J03064164+5728158[5].
- Q94528923's catalog code is recorded as AG+57 392[6].
- Q94528923's catalog code is recorded as BD+56 773[7].
- Q94528923's catalog code is recorded as GSC 03710-00042[8].
- Q94528923's catalog code is recorded as HD 19077[9].
- Q94528923's catalog code is recorded as PPM 28222[10].
- Q94528923's catalog code is recorded as SKY# 4646[11].
- Q94528923's catalog code is recorded as TYC 3710-42-1[12].
- Q94528923's catalog code is recorded as YZ 57 2748[13].
- Q94528923's catalog code is recorded as Gaia DR1 460262061378089984[14].
- Q94528923's catalog code is recorded as Gaia DR2 460262065679456640[15].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.21'}[16].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.37'}[17].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.959'}[18].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.391'}[19].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.241'}[20].
- Q94528923's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.7935'}[21].
- Q94528923's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.4925'}[22].
- Q94528923's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.10'}[23].
- Q94528923's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+222.5932'}[24].
- Q94528923's SIMBAD ID is recorded as HD 19077[25].
- Q94528923's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+46.67350358263030'}[26].