Q78366403
long period variable
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Q78366403
Summary
Q78366403 is a long-period variable star[1].
Key Facts
- Q78366403's instance of is recorded as long-period variable star[2].
- Q78366403's constellation is recorded as Dorado[3].
- Q78366403's catalog code is recorded as 2MASS J06022768-6609028[4].
- Q78366403's catalog code is recorded as OGLE LMC571.05.000019[5].
- Q78366403's catalog code is recorded as Gaia DR2 5476384710326445696[6].
- Q78366403's type of variable star is recorded as long-period variable star[7].
- Q78366403's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.69'}[8].
- Q78366403's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.56'}[9].
- Q78366403's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.15'}[10].
- Q78366403's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.815'}[11].
- Q78366403's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.9471'}[12].
- Q78366403's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0287'}[13].
- Q78366403's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+318.05'}[14].
- Q78366403's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78366403's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.61530967798900'}[16].
- Q78366403's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.15076355530990'}[17].
- Q78366403's epoch is recorded as J2000.0[18].
- Q78366403's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78366403's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.889'}[20].
- Q78366403's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.568'}[21].
Body
Definition and Type
Q78366403's instance of is recorded as long-period variable star[2].