Q82049841
star in the constellation Centaurus
Press Enter · cited answer in seconds
0 sources
Q82049841
Summary
Q82049841 is a star[1].
Key Facts
- Q82049841's instance of is recorded as star[2].
- Q82049841's constellation is recorded as Centaurus[3].
- Q82049841's spectral class is recorded as K0III[4].
- Q82049841's catalog code is recorded as CD-50 6919[5].
- Q82049841's catalog code is recorded as CPC 0 10298[6].
- Q82049841's catalog code is recorded as CPD-50 5114[7].
- Q82049841's catalog code is recorded as GSC 08242-02447[8].
- Q82049841's catalog code is recorded as HD 107507[9].
- Q82049841's catalog code is recorded as HIC 60284[10].
- Q82049841's catalog code is recorded as HIP 60284[11].
- Q82049841's catalog code is recorded as PPM 340911[12].
- Q82049841's catalog code is recorded as SAO 239874[13].
- Q82049841's catalog code is recorded as SRS 1471[14].
- Q82049841's catalog code is recorded as TYC 8242-2447-1[15].
- Q82049841's catalog code is recorded as 2MASS J12214268-5132038[16].
- Q82049841's catalog code is recorded as Gaia DR2 6125670343988037376[17].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.024'}[18].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.535'}[19].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.417'}[20].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.75'}[21].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.74'}[22].
- Q82049841's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.4573'}[23].
- Q82049841's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1451'}[24].
- Q82049841's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-11.33'}[25].
- Q82049841's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+317.9549'}[26].
Body
Definition and Type
Q82049841's instance of is recorded as star[2].