Q82390467
star in the constellation Mensa
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Q82390467
Summary
Q82390467 is a star[1].
Key Facts
- Q82390467's instance of is recorded as star[2].
- Q82390467's constellation is recorded as Mensa[3].
- Q82390467's catalog code is recorded as MACHO 76.10812.9[4].
- Q82390467's catalog code is recorded as 2MASS J05465970-7005266[5].
- Q82390467's catalog code is recorded as Gaia DR2 4657379423891038848[6].
- Q82390467's type of variable star is recorded as long-period variable star[7].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.331'}[8].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.756'}[9].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.614'}[10].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.61'}[11].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.56'}[12].
- Q82390467's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.0359'}[13].
- Q82390467's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7244'}[14].
- Q82390467's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.44'}[15].
- Q82390467's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1380.4528'}[16].
- Q82390467's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.74884944781100'}[17].
- Q82390467's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-70.09071102160870'}[18].
- Q82390467's epoch is recorded as J2000.0[19].
- Q82390467's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+11.266'}[20].
- Q82390467's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.022'}[21].
Body
Definition and Type
Q82390467's instance of is recorded as star[2].