Q82222567
star in the constellation Lyra
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Q82222567
Summary
Q82222567 is a star[1].
Key Facts
- Q82222567's instance of is recorded as star[2].
- Q82222567's constellation is recorded as Lyra[3].
- Q82222567's spectral class is recorded as G8.5IIIb[4].
- Q82222567's catalog code is recorded as Gaia DR2 2119121578060955776[5].
- Q82222567's catalog code is recorded as KIC 9631360[6].
- Q82222567's catalog code is recorded as 2MASS J18483887+4620422[7].
- Q82222567's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4301'}[8].
- Q82222567's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.724'}[9].
- Q82222567's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.090'}[10].
- Q82222567's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.992'}[11].
- Q82222567's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2154'}[12].
- Q82222567's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-162.16'}[13].
- Q82222567's metallicity is recorded as {'unit': '1', 'amount': '-0.31'}[14].
- Q82222567's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4642.53'}[15].
- Q82222567's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+282.16199372237713'}[16].
- Q82222567's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+46.34507583392889'}[17].
- Q82222567's epoch is recorded as J2000.0[18].
- Q82222567's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4713'}[19].
- Q82222567's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.562'}[20].
- Q82222567's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.465'}[21].
Body
Definition and Type
Q82222567's instance of is recorded as star[2].