Q78362301
long period variable
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Q78362301
Summary
Q78362301 is a long-period variable star[1].
Key Facts
- Q78362301's instance of is recorded as long-period variable star[2].
- Q78362301's constellation is recorded as Dorado[3].
- Q78362301's catalog code is recorded as 2MASS J05594145-6610546[4].
- Q78362301's catalog code is recorded as OGLE LMC563.17.000031[5].
- Q78362301's catalog code is recorded as Gaia DR2 4755810625378334336[6].
- Q78362301's type of variable star is recorded as long-period variable star[7].
- Q78362301's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.75'}[8].
- Q78362301's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.58'}[9].
- Q78362301's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.03'}[10].
- Q78362301's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.048'}[11].
- Q78362301's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0451'}[12].
- Q78362301's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0471'}[13].
- Q78362301's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+320.60'}[14].
- Q78362301's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78362301's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.92271756918930'}[16].
- Q78362301's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.18187629208770'}[17].
- Q78362301's epoch is recorded as J2000.0[18].
- Q78362301's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78362301's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.814'}[20].
- Q78362301's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.429'}[21].
Body
Definition and Type
Q78362301's instance of is recorded as long-period variable star[2].