Q77557495
star in the constellation Dorado
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Q77557495
Summary
Q77557495 is a star[1].
Key Facts
- Q77557495's instance of is recorded as star[2].
- Q77557495's constellation is recorded as Dorado[3].
- Q77557495's catalog code is recorded as MACHO 45.1753.8[4].
- Q77557495's catalog code is recorded as 2MASS J04512929-6858252[5].
- Q77557495's catalog code is recorded as Gaia DR2 4655480803521834368[6].
- Q77557495's type of variable star is recorded as long-period variable star[7].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.415'}[8].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.947'}[9].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.829'}[10].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.68'}[11].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.51'}[12].
- Q77557495's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.9517'}[13].
- Q77557495's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4313'}[14].
- Q77557495's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+17.11'}[15].
- Q77557495's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+698.6655'}[16].
- Q77557495's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+72.87199499095540'}[17].
- Q77557495's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-68.97365614468220'}[18].
- Q77557495's epoch is recorded as J2000.0[19].
- Q77557495's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+13.360'}[20].
- Q77557495's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.215'}[21].
Body
Definition and Type
Q77557495's instance of is recorded as star[2].