Q85469120
low-mass star in the constellation Libra
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Q85469120
Summary
Q85469120 is a low-mass star[1].
Key Facts
- Q85469120's instance of is recorded as low-mass star[2].
- Q85469120's constellation is recorded as Libra[3].
- Q85469120's spectral class is recorded as K[4].
- Q85469120's catalog code is recorded as [BHR2005] 868-13[5].
- Q85469120's catalog code is recorded as 2MASS J15084651-0032401[6].
- Q85469120's catalog code is recorded as Gaia DR2 4418547871772521728[7].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.2'}[8].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.3'}[9].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.8'}[10].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.07'}[11].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.63'}[12].
- Q85469120's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.8337'}[13].
- Q85469120's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+18.3791'}[14].
- Q85469120's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+86'}[15].
- Q85469120's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+54.4096'}[16].
- Q85469120's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+227.19378417625350'}[17].
- Q85469120's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-0.54448896138170'}[18].
- Q85469120's epoch is recorded as J2000.0[19].
- Q85469120's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-115.048'}[20].
- Q85469120's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-16.698'}[21].
Body
Definition and Type
Q85469120's instance of is recorded as low-mass star[2].