Q89705828
star in the constellation Perseus
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Q89705828
Summary
Q89705828 is a star[1].
Key Facts
- Q89705828's instance of is recorded as star[2].
- Q89705828's constellation is recorded as Perseus[3].
- Q89705828's spectral class is recorded as K0[4].
- Q89705828's catalog code is recorded as AG+31 377[5].
- Q89705828's catalog code is recorded as BD+31 682[6].
- Q89705828's catalog code is recorded as GSC 02357-00549[7].
- Q89705828's catalog code is recorded as PPM 68986[8].
- Q89705828's catalog code is recorded as TYC 2357-549-1[9].
- Q89705828's catalog code is recorded as HD 281387[10].
- Q89705828's catalog code is recorded as Gaia DR1 168581245940073088[11].
- Q89705828's catalog code is recorded as Gaia DR2 168581245940073088[12].
- Q89705828's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.34'}[13].
- Q89705828's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.42'}[14].
- Q89705828's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9968'}[15].
- Q89705828's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6624'}[16].
- Q89705828's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.73'}[17].
- Q89705828's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+601.5399'}[18].
- Q89705828's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+60.00318605041440'}[19].
- Q89705828's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+31.77398584134960'}[20].
- Q89705828's epoch is recorded as J2000.0[21].
- Q89705828's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.857'}[22].
- Q89705828's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+12.464'}[23].
Body
Definition and Type
Q89705828's instance of is recorded as star[2].