Q77539062
star in the constellation Mensa
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Q77539062
Summary
Q77539062 is a star[1].
Key Facts
- Q77539062's instance of is recorded as star[2].
- Q77539062's constellation is recorded as Mensa[3].
- Q77539062's catalog code is recorded as MACHO 39.3047.9[4].
- Q77539062's catalog code is recorded as 2MASS J04594625-7126334[5].
- Q77539062's catalog code is recorded as Gaia DR2 4654616896610502912[6].
- Q77539062's type of variable star is recorded as long-period variable star[7].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.622'}[8].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.103'}[9].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.006'}[10].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.20'}[11].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.55'}[12].
- Q77539062's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.0699'}[13].
- Q77539062's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4770'}[14].
- Q77539062's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.40'}[15].
- Q77539062's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2096.4361'}[16].
- Q77539062's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+74.94280889294440'}[17].
- Q77539062's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.44268207021780'}[18].
- Q77539062's epoch is recorded as J2000.0[19].
- Q77539062's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.410'}[20].
- Q77539062's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.944'}[21].
Body
Definition and Type
Q77539062's instance of is recorded as star[2].