Q83723895
star in the constellation Mensa
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Q83723895
Summary
Q83723895 is a star[1].
Key Facts
- Q83723895's instance of is recorded as star[2].
- Q83723895's constellation is recorded as Mensa[3].
- Q83723895's catalog code is recorded as MACHO 21.8251.1817[4].
- Q83723895's catalog code is recorded as 2MASS J05311405-7122103[5].
- Q83723895's catalog code is recorded as Gaia DR2 4651805758949270784[6].
- Q83723895's type of variable star is recorded as long-period variable star[7].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.874'}[8].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.348'}[9].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.247'}[10].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.08'}[11].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.12'}[12].
- Q83723895's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.4615'}[13].
- Q83723895's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6488'}[14].
- Q83723895's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+40.49'}[15].
- Q83723895's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1541.3070'}[16].
- Q83723895's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+82.80857258846480'}[17].
- Q83723895's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.36951616328580'}[18].
- Q83723895's epoch is recorded as J2000.0[19].
- Q83723895's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+10.606'}[20].
- Q83723895's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.188'}[21].
Body
Definition and Type
Q83723895's instance of is recorded as star[2].