Q93458017
high proper-motion star in the constellation Perseus
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Q93458017
Summary
Q93458017 is a high proper-motion star[1].
Key Facts
- Q93458017's instance of is recorded as high proper-motion star[2].
- Q93458017's constellation is recorded as Perseus[3].
- Q93458017's spectral class is recorded as F8[4].
- Q93458017's catalog code is recorded as 2MASS J04331375+4507012[5].
- Q93458017's catalog code is recorded as ADS 3288 AB[6].
- Q93458017's catalog code is recorded as AG+45 453[7].
- Q93458017's catalog code is recorded as BD+44 974[8].
- Q93458017's catalog code is recorded as CCDM J04332+4507AB[9].
- Q93458017's catalog code is recorded as GSC 03342-00033[10].
- Q93458017's catalog code is recorded as IDS 04260+4454 AB[11].
- Q93458017's catalog code is recorded as PPM 47165[12].
- Q93458017's catalog code is recorded as SAO 39599[13].
- Q93458017's catalog code is recorded as TYC 3342-33-1[14].
- Q93458017's catalog code is recorded as 1RXS J043314.2+450706[15].
- Q93458017's catalog code is recorded as WDS J04332+4507AB[16].
- Q93458017's catalog code is recorded as Gaia DR1 253575487631170560[17].
- Q93458017's catalog code is recorded as Gaia DR2 253575491934296960[18].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.41'}[19].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.92'}[20].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.340'}[21].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.009'}[22].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.968'}[23].
- Q93458017's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2781'}[24].
- Q93458017's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.6230'}[25].
- Q93458017's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.19'}[26].
Body
Definition and Type
Q93458017's instance of is recorded as high proper-motion star[2].