Q78366001
long period variable
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Q78366001
Summary
Q78366001 is a long-period variable star[1].
Key Facts
- Q78366001's instance of is recorded as long-period variable star[2].
- Q78366001's constellation is recorded as Dorado[3].
- Q78366001's catalog code is recorded as 2MASS J05582663-6656084[4].
- Q78366001's catalog code is recorded as OGLE LMC562.27.009474[5].
- Q78366001's catalog code is recorded as Gaia DR2 4659684687450446848[6].
- Q78366001's type of variable star is recorded as long-period variable star[7].
- Q78366001's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.82'}[8].
- Q78366001's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.54'}[9].
- Q78366001's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.89'}[10].
- Q78366001's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.067'}[11].
- Q78366001's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0726'}[12].
- Q78366001's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0158'}[13].
- Q78366001's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+277.29'}[14].
- Q78366001's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78366001's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.61092251089310'}[16].
- Q78366001's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.93573451730900'}[17].
- Q78366001's epoch is recorded as J2000.0[18].
- Q78366001's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78366001's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.866'}[20].
- Q78366001's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.641'}[21].
Body
Definition and Type
Q78366001's instance of is recorded as long-period variable star[2].