Q78362003
long period variable
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Q78362003
Summary
Q78362003 is a long-period variable star[1].
Key Facts
- Q78362003's instance of is recorded as long-period variable star[2].
- Q78362003's constellation is recorded as Dorado[3].
- Q78362003's catalog code is recorded as 2MASS J05574881-6627269[4].
- Q78362003's catalog code is recorded as OGLE LMC563.09.000036[5].
- Q78362003's catalog code is recorded as Gaia DR2 4659727121729343488[6].
- Q78362003's type of variable star is recorded as long-period variable star[7].
- Q78362003's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.57'}[8].
- Q78362003's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.42'}[9].
- Q78362003's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.99'}[10].
- Q78362003's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.693'}[11].
- Q78362003's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.8052'}[12].
- Q78362003's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0317'}[13].
- Q78362003's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+281.63'}[14].
- Q78362003's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78362003's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.45345163591140'}[16].
- Q78362003's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.45750817536000'}[17].
- Q78362003's epoch is recorded as J2000.0[18].
- Q78362003's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78362003's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.594'}[20].
- Q78362003's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.546'}[21].
Body
Definition and Type
Q78362003's instance of is recorded as long-period variable star[2].