Q90660307
high proper-motion star in the constellation Ophiuchus
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Q90660307
Summary
Q90660307 is a high proper-motion star[1].
Key Facts
- Q90660307's instance of is recorded as high proper-motion star[2].
- Q90660307's constellation is recorded as Ophiuchus[3].
- Q90660307's spectral class is recorded as K0III/IV[4].
- Q90660307's catalog code is recorded as AG+02 2097[5].
- Q90660307's catalog code is recorded as BD+02 3335[6].
- Q90660307's catalog code is recorded as GC 23715[7].
- Q90660307's catalog code is recorded as GSC 00418-01077[8].
- Q90660307's catalog code is recorded as HD 158718[9].
- Q90660307's catalog code is recorded as PPM 164117[10].
- Q90660307's catalog code is recorded as SAO 122450[11].
- Q90660307's catalog code is recorded as TYC 418-1077-1[12].
- Q90660307's catalog code is recorded as Wolf 753[13].
- Q90660307's catalog code is recorded as YZ 2 5800[14].
- Q90660307's catalog code is recorded as 2MASS J17304256+0219211[15].
- Q90660307's catalog code is recorded as Gaia DR1 4376696984592255104[16].
- Q90660307's catalog code is recorded as Gaia DR2 4376696988889549056[17].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.470'}[18].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.126'}[19].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.000'}[20].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.02'}[21].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.98'}[22].
- Q90660307's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8420'}[23].
- Q90660307's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.0359'}[24].
- Q90660307's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+28.74'}[25].
- Q90660307's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+124.4416'}[26].
Body
Definition and Type
Q90660307's instance of is recorded as high proper-motion star[2].