Q77559835
star in the constellation Mensa
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Q77559835
Summary
Q77559835 is a star[1].
Key Facts
- Q77559835's instance of is recorded as star[2].
- Q77559835's constellation is recorded as Mensa[3].
- Q77559835's catalog code is recorded as MACHO 39.3290.8[4].
- Q77559835's catalog code is recorded as 2MASS J05003613-7123124[5].
- Q77559835's catalog code is recorded as Gaia DR2 4654618030481868416[6].
- Q77559835's type of variable star is recorded as long-period variable star[7].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.587'}[8].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.070'}[9].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.950'}[10].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.68'}[11].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.54'}[12].
- Q77559835's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.1451'}[13].
- Q77559835's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3609'}[14].
- Q77559835's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+77.42'}[15].
- Q77559835's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2770.8507'}[16].
- Q77559835's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+75.15049410147990'}[17].
- Q77559835's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.38678976882840'}[18].
- Q77559835's epoch is recorded as J2000.0[19].
- Q77559835's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.064'}[20].
- Q77559835's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.432'}[21].
Body
Definition and Type
Q77559835's instance of is recorded as star[2].