Q91504893
star in the constellation Centaurus
Press Enter · cited answer in seconds
0 sources
Q91504893
Summary
Q91504893 is a star[1].
Key Facts
- Q91504893's instance of is recorded as star[2].
- Q91504893's constellation is recorded as Centaurus[3].
- Q91504893's spectral class is recorded as K1III[4].
- Q91504893's catalog code is recorded as CD-30 10188[5].
- Q91504893's catalog code is recorded as CPC 17 6486[6].
- Q91504893's catalog code is recorded as CPD-30 3560[7].
- Q91504893's catalog code is recorded as GSC 07248-00743[8].
- Q91504893's catalog code is recorded as HD 111965[9].
- Q91504893's catalog code is recorded as HIC 62890[10].
- Q91504893's catalog code is recorded as HIP 62890[11].
- Q91504893's catalog code is recorded as PPM 290710[12].
- Q91504893's catalog code is recorded as SAO 203906[13].
- Q91504893's catalog code is recorded as SRS 11276[14].
- Q91504893's catalog code is recorded as TYC 7248-743-1[15].
- Q91504893's catalog code is recorded as 2MASS J12531977-3120559[16].
- Q91504893's catalog code is recorded as Gaia DR2 6183829664366486656[17].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.395'}[18].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.837'}[19].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.697'}[20].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.40'}[21].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.60'}[22].
- Q91504893's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.0640'}[23].
- Q91504893's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.4547'}[24].
- Q91504893's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.32'}[25].
- Q91504893's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+289.4607'}[26].
Body
Definition and Type
Q91504893's instance of is recorded as star[2].