Q87562511
star in the constellation Cygnus
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Q87562511
Summary
Q87562511 is a star[1].
Key Facts
- Q87562511's instance of is recorded as star[2].
- Q87562511's constellation is recorded as Cygnus[3].
- Q87562511's spectral class is recorded as K[4].
- Q87562511's catalog code is recorded as AG+43 1752[5].
- Q87562511's catalog code is recorded as BD+42 3540[6].
- Q87562511's catalog code is recorded as GSC 03149-01838[7].
- Q87562511's catalog code is recorded as HD 189300[8].
- Q87562511's catalog code is recorded as PPM 59094[9].
- Q87562511's catalog code is recorded as SAO 49021[10].
- Q87562511's catalog code is recorded as TYC 3149-1838-1[11].
- Q87562511's catalog code is recorded as 2MASS J19572838+4316468[12].
- Q87562511's catalog code is recorded as Gaia DR2 2075954614127861504[13].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.42'}[14].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.722'}[15].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.320'}[16].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.176'}[17].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.35'}[18].
- Q87562511's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1623'}[19].
- Q87562511's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.4087'}[20].
- Q87562511's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-61.79'}[21].
- Q87562511's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+156.0379'}[22].
- Q87562511's SIMBAD ID is recorded as HD 189300[23].
- Q87562511's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+299.36826041145010'}[24].
- Q87562511's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.27967305159340'}[25].
- Q87562511's epoch is recorded as J2000.0[26].