Q77866030
star in the constellation Ara
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Q77866030
Summary
Q77866030 is a star[1].
Key Facts
- Q77866030's instance of is recorded as star[2].
- Q77866030's constellation is recorded as Ara[3].
- Q77866030 is part of Q757175[4].
- Q77866030's catalog code is recorded as [LML2012] 56902[5].
- Q77866030's catalog code is recorded as Gaia DR2 5921755329830903296[6].
- Q77866030's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.26'}[7].
- Q77866030's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.42'}[8].
- Q77866030's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0824'}[9].
- Q77866030's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3488'}[10].
- Q77866030's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+17.5'}[11].
- Q77866030's metallicity is recorded as {'unit': '1', 'amount': '-2.19'}[12].
- Q77866030's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+6'}[13].
- Q77866030's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+265.03004446356370'}[14].
- Q77866030's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-53.58331822124900'}[15].
- Q77866030's epoch is recorded as J2000.0[16].
- Q77866030's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6546'}[17].
- Q77866030's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+13000'}[18].
- Q77866030's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-17.612'}[19].
- Q77866030's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.292'}[20].
Body
Definition and Type
Q77866030's instance of is recorded as star[2].
Use and Application
Q77866030 is part of Q757175[4].