Q85959863
star in the constellation Draco
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Q85959863
Summary
Q85959863 is a star[1].
Key Facts
- Q85959863's instance of is recorded as star[2].
- Q85959863's constellation is recorded as Draco[3].
- Q85959863's spectral class is recorded as K0[4].
- Q85959863's catalog code is recorded as AG+84 399[5].
- Q85959863's catalog code is recorded as BD+84 428[6].
- Q85959863's catalog code is recorded as GSC 04652-01702[7].
- Q85959863's catalog code is recorded as PPM 3282[8].
- Q85959863's catalog code is recorded as SAO 3123[9].
- Q85959863's catalog code is recorded as TYC 4652-1702-1[10].
- Q85959863's catalog code is recorded as Gaia DR1 2302936965622236672[11].
- Q85959863's catalog code is recorded as Gaia DR2 2302936969918425856[12].
- Q85959863's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.35'}[13].
- Q85959863's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.66'}[14].
- Q85959863's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.0138'}[15].
- Q85959863's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9133'}[16].
- Q85959863's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+7.78'}[17].
- Q85959863's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1094.9305'}[18].
- Q85959863's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+280.57049934551210'}[19].
- Q85959863's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.91723262650430'}[20].
- Q85959863's epoch is recorded as J2000.0[21].
- Q85959863's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.566'}[22].
- Q85959863's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.706'}[23].
Body
Definition and Type
Q85959863's instance of is recorded as star[2].