Q89264521
star in the constellation Centaurus
Press Enter · cited answer in seconds
0 sources
Q89264521
Summary
Q89264521 is a star[1].
Key Facts
- Q89264521's instance of is recorded as star[2].
- Q89264521's constellation is recorded as Centaurus[3].
- Q89264521's spectral class is recorded as G2/3V[4].
- Q89264521's catalog code is recorded as CD-32 9126[5].
- Q89264521's catalog code is recorded as CPC 17 6587[6].
- Q89264521's catalog code is recorded as CPD-32 3349[7].
- Q89264521's catalog code is recorded as GC 17728[8].
- Q89264521's catalog code is recorded as GSC 07254-01556[9].
- Q89264521's catalog code is recorded as HD 113531[10].
- Q89264521's catalog code is recorded as HIC 63808[11].
- Q89264521's catalog code is recorded as HIP 63808[12].
- Q89264521's catalog code is recorded as PPM 290939[13].
- Q89264521's catalog code is recorded as SAO 204100[14].
- Q89264521's catalog code is recorded as TYC 7254-1556-1[15].
- Q89264521's catalog code is recorded as 2MASS J13044411-3304219[16].
- Q89264521's catalog code is recorded as Gaia DR2 6180232612076212096[17].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.575'}[18].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.091'}[19].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.982'}[20].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.08'}[21].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.86'}[22].
- Q89264521's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8501'}[23].
- Q89264521's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.3665'}[24].
- Q89264521's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-2.80'}[25].
- Q89264521's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+422.5650'}[26].
Body
Definition and Type
Q89264521's instance of is recorded as star[2].