Q95689603
high proper-motion star in the constellation Cygnus
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Q95689603
Summary
Q95689603 is a high proper-motion star[1].
Key Facts
- Q95689603's instance of is recorded as high proper-motion star[2].
- Q95689603's constellation is recorded as Cygnus[3].
- Q95689603's spectral class is recorded as G0[4].
- Q95689603's catalog code is recorded as ADS 14156 AB[5].
- Q95689603's catalog code is recorded as AG+48 1662[6].
- Q95689603's catalog code is recorded as BD+48 3185[7].
- Q95689603's catalog code is recorded as CCDM J20405+4855AB[8].
- Q95689603's catalog code is recorded as GSC 03582-01863[9].
- Q95689603's catalog code is recorded as IDS 20373+4834 AB[10].
- Q95689603's catalog code is recorded as PPM 60305[11].
- Q95689603's catalog code is recorded as SAO 49924[12].
- Q95689603's catalog code is recorded as TYC 3582-1863-1[13].
- Q95689603's catalog code is recorded as WDS J20405+4855AB[14].
- Q95689603's catalog code is recorded as Gaia DR1 2167838116494731648[15].
- Q95689603's catalog code is recorded as Gaia DR2 2167838120797539200[16].
- Q95689603's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.31'}[17].
- Q95689603's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.87'}[18].
- Q95689603's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1570'}[19].
- Q95689603's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.5855'}[20].
- Q95689603's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.9'}[21].
- Q95689603's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+86.3148'}[22].
- Q95689603's SIMBAD ID is recorded as BD+48 3185[23].
- Q95689603's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+310.12634893130340'}[24].
- Q95689603's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.91979753759110'}[25].
- Q95689603's epoch is recorded as J2000.0[26].