Q83730440
star in the constellation Mensa
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Q83730440
Summary
Q83730440 is a star[1].
Key Facts
- Q83730440's instance of is recorded as star[2].
- Q83730440's constellation is recorded as Mensa[3].
- Q83730440's catalog code is recorded as MACHO 28.11885.9[4].
- Q83730440's catalog code is recorded as 2MASS J05534430-7107476[5].
- Q83730440's catalog code is recorded as Gaia DR2 4656894638028205696[6].
- Q83730440's type of variable star is recorded as long-period variable star[7].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.979'}[8].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.706'}[9].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.630'}[10].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.86'}[11].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.91'}[12].
- Q83730440's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.0115'}[13].
- Q83730440's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1902'}[14].
- Q83730440's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.54'}[15].
- Q83730440's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+313.4600'}[16].
- Q83730440's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+88.43462963669180'}[17].
- Q83730440's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-71.12987384505080'}[18].
- Q83730440's epoch is recorded as J2000.0[19].
- Q83730440's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+42.357'}[20].
- Q83730440's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.392'}[21].
Body
Definition and Type
Q83730440's instance of is recorded as star[2].