Q83713775
star in the constellation Mensa
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Q83713775
Summary
Q83713775 is a star[1].
Key Facts
- Q83713775's instance of is recorded as star[2].
- Q83713775's constellation is recorded as Mensa[3].
- Q83713775's catalog code is recorded as MACHO 22.5590.9[4].
- Q83713775's catalog code is recorded as 2MASS J05151793-7119545[5].
- Q83713775's catalog code is recorded as Gaia DR2 4651950447796288256[6].
- Q83713775's type of variable star is recorded as long-period variable star[7].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.201'}[8].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.741'}[9].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.669'}[10].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.87'}[11].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.20'}[12].
- Q83713775's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7593'}[13].
- Q83713775's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0620'}[14].
- Q83713775's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.87'}[15].
- Q83713775's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+941.6196'}[16].
- Q83713775's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+78.82475499516640'}[17].
- Q83713775's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.33182652537910'}[18].
- Q83713775's epoch is recorded as J2000.0[19].
- Q83713775's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+11.235'}[20].
- Q83713775's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.666'}[21].
Body
Definition and Type
Q83713775's instance of is recorded as star[2].