Q83717848
star in the constellation Mensa
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Q83717848
Summary
Q83717848 is a star[1].
Key Facts
- Q83717848's instance of is recorded as star[2].
- Q83717848's constellation is recorded as Mensa[3].
- Q83717848's catalog code is recorded as MACHO 13.7046.7[4].
- Q83717848's catalog code is recorded as 2MASS J05234903-7103333[5].
- Q83717848's catalog code is recorded as Gaia DR2 4651870488363013120[6].
- Q83717848's type of variable star is recorded as long-period variable star[7].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.102'}[8].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.805'}[9].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.765'}[10].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.64'}[11].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.93'}[12].
- Q83717848's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.1651'}[13].
- Q83717848's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.8131'}[14].
- Q83717848's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.15'}[15].
- Q83717848's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+551.5416'}[16].
- Q83717848's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+80.95428527180120'}[17].
- Q83717848's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.05930302313190'}[18].
- Q83717848's epoch is recorded as J2000.0[19].
- Q83717848's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+19.109'}[20].
- Q83717848's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+9.443'}[21].
Body
Definition and Type
Q83717848's instance of is recorded as star[2].