Q90513712
high proper-motion star in the constellation Serpens
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Q90513712
Summary
Q90513712 is a high proper-motion star[1].
Key Facts
- Q90513712's instance of is recorded as high proper-motion star[2].
- Q90513712's constellation is recorded as Serpens[3].
- Q90513712's spectral class is recorded as K0III[4].
- Q90513712's catalog code is recorded as AG-01 1938[5].
- Q90513712's catalog code is recorded as BD-01 3085[6].
- Q90513712's catalog code is recorded as GSC 05017-00672[7].
- Q90513712's catalog code is recorded as HD 140347[8].
- Q90513712's catalog code is recorded as HIC 76991[9].
- Q90513712's catalog code is recorded as HIP 76991[10].
- Q90513712's catalog code is recorded as PPM 179630[11].
- Q90513712's catalog code is recorded as SAO 140715[12].
- Q90513712's catalog code is recorded as TYC 5017-672-1[13].
- Q90513712's catalog code is recorded as YZ 91 3980[14].
- Q90513712's catalog code is recorded as 2MASS J15431355-0143582[15].
- Q90513712's catalog code is recorded as Gaia DR1 4404049775872184448[16].
- Q90513712's catalog code is recorded as Gaia DR2 4404049780169584512[17].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.905'}[18].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.400'}[19].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.224'}[20].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.92'}[21].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.04'}[22].
- Q90513712's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5662'}[23].
- Q90513712's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.7030'}[24].
- Q90513712's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.41'}[25].
- Q90513712's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+149.1869'}[26].
Body
Definition and Type
Q90513712's instance of is recorded as high proper-motion star[2].