Q85469295
low-mass star in the constellation Virgo
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Q85469295
Summary
Q85469295 is a low-mass star[1].
Key Facts
- Q85469295's instance of is recorded as low-mass star[2].
- Q85469295's constellation is recorded as Virgo[3].
- Q85469295's spectral class is recorded as K[4].
- Q85469295's catalog code is recorded as [BHR2005] 868-6[5].
- Q85469295's catalog code is recorded as 2MASS J14560917+0207165[6].
- Q85469295's catalog code is recorded as Gaia DR2 1154211888876993664[7].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.8'}[8].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6'}[9].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4'}[10].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.50'}[11].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.84'}[12].
- Q85469295's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9448'}[13].
- Q85469295's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0613'}[14].
- Q85469295's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9'}[15].
- Q85469295's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+942.2406'}[16].
- Q85469295's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+224.03826616473460'}[17].
- Q85469295's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+2.12125636652650'}[18].
- Q85469295's epoch is recorded as J2000.0[19].
- Q85469295's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.162'}[20].
- Q85469295's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-19.017'}[21].
Body
Definition and Type
Q85469295's instance of is recorded as low-mass star[2].