Q80937488
high proper-motion star in the constellation Draco
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Q80937488
Summary
Q80937488 is a high proper-motion star[1].
Key Facts
- Q80937488's instance of is recorded as high proper-motion star[2].
- Q80937488's constellation is recorded as Draco[3].
- Q80937488's spectral class is recorded as K7[4].
- Q80937488's catalog code is recorded as SDSS J172106.71+584942.3[5].
- Q80937488's catalog code is recorded as [PCE2006] 862[6].
- Q80937488's catalog code is recorded as Gaia DR2 1434008147554963072[7].
- Q80937488's redshift is recorded as {'unit': '1', 'amount': '-0.00063'}[8].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+22.611'}[9].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.767'}[10].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.429'}[11].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.802'}[12].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.384'}[13].
- Q80937488's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.3885'}[14].
- Q80937488's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7314'}[15].
- Q80937488's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-189'}[16].
- Q80937488's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+260.27799019711970'}[17].
- Q80937488's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+58.82840416794100'}[18].
- Q80937488's epoch is recorded as J2000.0[19].
- Q80937488's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+39.735'}[20].
- Q80937488's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-36.169'}[21].
Body
Definition and Type
Q80937488's instance of is recorded as high proper-motion star[2].