Q85130422
high proper-motion star in the constellation Taurus
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Q85130422
Summary
Q85130422 is a high proper-motion star[1].
Key Facts
- Q85130422's instance of is recorded as high proper-motion star[2].
- Q85130422's constellation is recorded as Taurus[3].
- Q85130422's spectral class is recorded as K4[4].
- Q85130422's catalog code is recorded as StKM 1-472[5].
- Q85130422's catalog code is recorded as 2MASS J04125342+0219039[6].
- Q85130422's catalog code is recorded as WISEA J041253.49+021905.0[7].
- Q85130422's catalog code is recorded as Gaia DR2 3259057231868526848[8].
- Q85130422's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.7'}[9].
- Q85130422's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.681'}[10].
- Q85130422's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.053'}[11].
- Q85130422's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.932'}[12].
- Q85130422's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.3561'}[13].
- Q85130422's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.8188'}[14].
- Q85130422's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+90.49'}[15].
- Q85130422's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+72.3652'}[16].
- Q85130422's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+63.22262985838120'}[17].
- Q85130422's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+2.31780882069020'}[18].
- Q85130422's epoch is recorded as J2000.0[19].
- Q85130422's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+97.315'}[20].
- Q85130422's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+95.942'}[21].
Body
Definition and Type
Q85130422's instance of is recorded as high proper-motion star[2].