Q90193952
high proper-motion star in the constellation Apus
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Q90193952
Summary
Q90193952 is a high proper-motion star[1].
Key Facts
- Q90193952's instance of is recorded as high proper-motion star[2].
- Q90193952's constellation is recorded as Apus[3].
- Q90193952's spectral class is recorded as K1/2(V)[4].
- Q90193952's catalog code is recorded as CPD-71 1909[5].
- Q90193952's catalog code is recorded as GSC 09268-02093[6].
- Q90193952's catalog code is recorded as HD 139536[7].
- Q90193952's catalog code is recorded as HIC 77049[8].
- Q90193952's catalog code is recorded as HIP 77049[9].
- Q90193952's catalog code is recorded as TYC 9268-2093-1[10].
- Q90193952's catalog code is recorded as uvby98 100139536[11].
- Q90193952's catalog code is recorded as 2MASS J15435909-7142175[12].
- Q90193952's catalog code is recorded as WISEA J154358.83-714218.3[13].
- Q90193952's catalog code is recorded as Gaia DR1 5794923532516499712[14].
- Q90193952's catalog code is recorded as GEN# +1.00139536[15].
- Q90193952's catalog code is recorded as Gaia DR2 5794923536819249408[16].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.514'}[17].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.078'}[18].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.000'}[19].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.14'}[20].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.02'}[21].
- Q90193952's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8190'}[22].
- Q90193952's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+16.0898'}[23].
- Q90193952's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-18.499'}[24].
- Q90193952's metallicity is recorded as {'unit': '1', 'amount': '-0.07'}[25].
- Q90193952's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+62.1512'}[26].