Q77559324
star in the constellation Dorado
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Q77559324
Summary
Q77559324 is a star[1].
Key Facts
- Q77559324's instance of is recorded as star[2].
- Q77559324's constellation is recorded as Dorado[3].
- Q77559324's catalog code is recorded as MACHO 33.10592.10[4].
- Q77559324's catalog code is recorded as 2MASS J05451118-6833520[5].
- Q77559324's catalog code is recorded as Gaia DR2 4657759442602840448[6].
- Q77559324's type of variable star is recorded as long-period variable star[7].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.098'}[8].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.556'}[9].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.465'}[10].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.76'}[11].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.25'}[12].
- Q77559324's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6172'}[13].
- Q77559324's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1174'}[14].
- Q77559324's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.42'}[15].
- Q77559324's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+894.9347'}[16].
- Q77559324's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.29665866536770'}[17].
- Q77559324's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-68.56442724084110'}[18].
- Q77559324's epoch is recorded as J2000.0[19].
- Q77559324's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+13.831'}[20].
- Q77559324's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.875'}[21].
Body
Definition and Type
Q77559324's instance of is recorded as star[2].