Q88606834
star in the constellation Gemini
Press Enter · cited answer in seconds
0 sources
Q88606834
Summary
Q88606834 is a star[1].
Key Facts
- Q88606834's instance of is recorded as star[2].
- Q88606834's constellation is recorded as Gemini[3].
- Q88606834's spectral class is recorded as B9[4].
- Q88606834's catalog code is recorded as AG+33 756[5].
- Q88606834's catalog code is recorded as BD+33 1512[6].
- Q88606834's catalog code is recorded as GSC 02456-00245[7].
- Q88606834's catalog code is recorded as HD 57380[8].
- Q88606834's catalog code is recorded as HIC 35748[9].
- Q88606834's catalog code is recorded as HIP 35748[10].
- Q88606834's catalog code is recorded as PPM 72724[11].
- Q88606834's catalog code is recorded as SAO 60020[12].
- Q88606834's catalog code is recorded as TD1 9832[13].
- Q88606834's catalog code is recorded as TYC 2456-245-1[14].
- Q88606834's catalog code is recorded as 2MASS J07222513+3313280[15].
- Q88606834's catalog code is recorded as Gaia DR1 893241665857258368[16].
- Q88606834's catalog code is recorded as Gaia DR2 893241670153865216[17].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.02'}[18].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.957'}[19].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.966'}[20].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.971'}[21].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.05'}[22].
- Q88606834's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.0485'}[23].
- Q88606834's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.0851'}[24].
- Q88606834's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-32.00'}[25].
- Q88606834's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+324.1386'}[26].
Body
Definition and Type
Q88606834's instance of is recorded as star[2].