Q88830821
star in the constellation Hydra
Press Enter · cited answer in seconds
0 sources
Q88830821
Summary
Q88830821 is a star[1].
Key Facts
- Q88830821's instance of is recorded as star[2].
- Q88830821's constellation is recorded as Hydra[3].
- Q88830821's spectral class is recorded as K3(III)[4].
- Q88830821 is part of Messier 48[5].
- Q88830821's catalog code is recorded as Cl* NGC 2548 WTB 182[6].
- Q88830821's catalog code is recorded as BD-05 2470[7].
- Q88830821's catalog code is recorded as GSC 04860-00535[8].
- Q88830821's catalog code is recorded as HD 69291[9].
- Q88830821's catalog code is recorded as IRAS 08137-0536[10].
- Q88830821's catalog code is recorded as NGC 2548 2222[11].
- Q88830821's catalog code is recorded as PPM 191147[12].
- Q88830821's catalog code is recorded as SAO 135703[13].
- Q88830821's catalog code is recorded as TYC 4860-535-1[14].
- Q88830821's catalog code is recorded as YZ 95 3137[15].
- Q88830821's catalog code is recorded as 2MASS J08161358-0545250[16].
- Q88830821's catalog code is recorded as Gaia DR1 3064381890644519552[17].
- Q88830821's catalog code is recorded as Gaia DR2 3064381890644519552[18].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.99'}[19].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.960'}[20].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.129'}[21].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.852'}[22].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.77'}[23].
- Q88830821's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3353'}[24].
- Q88830821's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5487'}[25].
- Q88830821's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.80'}[26].
Body
Definition and Type
Q88830821's instance of is recorded as star[2].
Use and Application
Q88830821 is part of Messier 48[5].