Q78362541
long period variable
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Q78362541
Summary
Q78362541 is a long-period variable star[1].
Key Facts
- Q78362541's instance of is recorded as long-period variable star[2].
- Q78362541's constellation is recorded as Dorado[3].
- Q78362541's catalog code is recorded as 2MASS J06011261-6618125[4].
- Q78362541's catalog code is recorded as OGLE LMC570.32.004239[5].
- Q78362541's catalog code is recorded as Gaia DR2 5476379006609810816[6].
- Q78362541's type of variable star is recorded as long-period variable star[7].
- Q78362541's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.11'}[8].
- Q78362541's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.98'}[9].
- Q78362541's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.63'}[10].
- Q78362541's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.184'}[11].
- Q78362541's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.3571'}[12].
- Q78362541's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0461'}[13].
- Q78362541's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+301.00'}[14].
- Q78362541's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78362541's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.30256865681120'}[16].
- Q78362541's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.30349309941240'}[17].
- Q78362541's epoch is recorded as J2000.0[18].
- Q78362541's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78362541's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.830'}[20].
- Q78362541's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.569'}[21].
Body
Definition and Type
Q78362541's instance of is recorded as long-period variable star[2].