Q89976248
high proper-motion star in the constellation Centaurus
Press Enter · cited answer in seconds
0 sources
Q89976248
Summary
Q89976248 is a high proper-motion star[1].
Key Facts
- Q89976248's instance of is recorded as high proper-motion star[2].
- Q89976248's constellation is recorded as Centaurus[3].
- Q89976248's spectral class is recorded as G1V[4].
- Q89976248's catalog code is recorded as CD-49 6260[5].
- Q89976248's catalog code is recorded as CPC 0 9595[6].
- Q89976248's catalog code is recorded as CPD-49 4321[7].
- Q89976248's catalog code is recorded as GSC 08222-00592[8].
- Q89976248's catalog code is recorded as HD 100331[9].
- Q89976248's catalog code is recorded as HIC 56285[10].
- Q89976248's catalog code is recorded as HIP 56285[11].
- Q89976248's catalog code is recorded as PPM 316499[12].
- Q89976248's catalog code is recorded as SAO 222852[13].
- Q89976248's catalog code is recorded as TYC 8222-592-1[14].
- Q89976248's catalog code is recorded as 2MASS J11321886-4956507[15].
- Q89976248's catalog code is recorded as Gaia DR1 5372974847159943168[16].
- Q89976248's catalog code is recorded as Gaia DR2 5372974851463727872[17].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.217'}[18].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.974'}[19].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.862'}[20].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.32'}[21].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.00'}[22].
- Q89976248's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2111'}[23].
- Q89976248's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.0605'}[24].
- Q89976248's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+36.81'}[25].
- Q89976248's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+141.6330'}[26].