Q77541720
star in the constellation Mensa
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Q77541720
Summary
Q77541720 is a star[1].
Key Facts
- Q77541720's instance of is recorded as star[2].
- Q77541720's constellation is recorded as Mensa[3].
- Q77541720's catalog code is recorded as MACHO 43.510.9[4].
- Q77541720's catalog code is recorded as 2MASS J04440437-7110462[5].
- Q77541720's catalog code is recorded as Gaia DR2 4654776635036420096[6].
- Q77541720's type of variable star is recorded as long-period variable star[7].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.058'}[8].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.697'}[9].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.615'}[10].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.35'}[11].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.77'}[12].
- Q77541720's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3732'}[13].
- Q77541720's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.4880'}[14].
- Q77541720's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-6.25'}[15].
- Q77541720's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+286.6972'}[16].
- Q77541720's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+71.01831477612310'}[17].
- Q77541720's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.17950896257000'}[18].
- Q77541720's epoch is recorded as J2000.0[19].
- Q77541720's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+37.814'}[20].
- Q77541720's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+15.189'}[21].
Body
Definition and Type
Q77541720's instance of is recorded as star[2].