Q77557289
star in the constellation Dorado
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Q77557289
Summary
Q77557289 is a star[1].
Key Facts
- Q77557289's instance of is recorded as star[2].
- Q77557289's constellation is recorded as Dorado[3].
- Q77557289's catalog code is recorded as MACHO 55.3615.9[4].
- Q77557289's catalog code is recorded as 2MASS J05021518-6552186[5].
- Q77557289's catalog code is recorded as Gaia DR2 4662263557637121024[6].
- Q77557289's type of variable star is recorded as long-period variable star[7].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.058'}[8].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.551'}[9].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.412'}[10].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.18'}[11].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.11'}[12].
- Q77557289's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6970'}[13].
- Q77557289's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5681'}[14].
- Q77557289's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+46.29'}[15].
- Q77557289's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1760.2535'}[16].
- Q77557289's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+75.56330993780200'}[17].
- Q77557289's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-65.87182870239750'}[18].
- Q77557289's epoch is recorded as J2000.0[19].
- Q77557289's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+9.841'}[20].
- Q77557289's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.500'}[21].
Body
Definition and Type
Q77557289's instance of is recorded as star[2].