Q90493569
high proper-motion star in the constellation Canes Venatici
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Q90493569
Summary
Q90493569 is a high proper-motion star[1].
Key Facts
- Q90493569's instance of is recorded as high proper-motion star[2].
- Q90493569's constellation is recorded as Canes Venatici[3].
- Q90493569's spectral class is recorded as G8V[4].
- Q90493569's catalog code is recorded as Pul -3 890240[5].
- Q90493569's catalog code is recorded as AG+40 1243[6].
- Q90493569's catalog code is recorded as BD+40 2509[7].
- Q90493569's catalog code is recorded as GPM 183.171753+40.041185[8].
- Q90493569's catalog code is recorded as GSC 03017-00763[9].
- Q90493569's catalog code is recorded as NGP 40 86[10].
- Q90493569's catalog code is recorded as PPM 52863[11].
- Q90493569's catalog code is recorded as SAO 44079[12].
- Q90493569's catalog code is recorded as TYC 3017-763-1[13].
- Q90493569's catalog code is recorded as [HFE83] 858[14].
- Q90493569's catalog code is recorded as 2MASS J12124117+4002278[15].
- Q90493569's catalog code is recorded as Gaia DR1 1535942221298142848[16].
- Q90493569's catalog code is recorded as Gaia DR2 1535942221298142848[17].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5'}[18].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.377'}[19].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.902'}[20].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.97'}[21].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.85'}[22].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.00'}[23].
- Q90493569's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7379'}[24].
- Q90493569's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+15.7784'}[25].
- Q90493569's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-18.41'}[26].
Body
Definition and Type
Q90493569's instance of is recorded as high proper-motion star[2].