Q93289020
star in the constellation Draco
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Q93289020
Summary
Q93289020 is a star[1].
Key Facts
- Q93289020's instance of is recorded as star[2].
- Q93289020's constellation is recorded as Draco[3].
- Q93289020's spectral class is recorded as G0[4].
- Q93289020's catalog code is recorded as AG+71 577[5].
- Q93289020's catalog code is recorded as BD+71 957[6].
- Q93289020's catalog code is recorded as GSC 04452-01494[7].
- Q93289020's catalog code is recorded as PPM 10214[8].
- Q93289020's catalog code is recorded as SAO 9446[9].
- Q93289020's catalog code is recorded as TYC 4452-1494-1[10].
- Q93289020's catalog code is recorded as Gaia DR1 2263558059752194560[11].
- Q93289020's catalog code is recorded as Gaia DR2 2263558064049010432[12].
- Q93289020's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.92'}[13].
- Q93289020's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.58'}[14].
- Q93289020's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8141'}[15].
- Q93289020's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.1123'}[16].
- Q93289020's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.79'}[17].
- Q93289020's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+140.6015'}[18].
- Q93289020's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.66345987130660'}[19].
- Q93289020's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+71.49115789616960'}[20].
- Q93289020's epoch is recorded as J2000.0[21].
- Q93289020's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-13.779'}[22].
- Q93289020's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+5.261'}[23].
Body
Definition and Type
Q93289020's instance of is recorded as star[2].