Q78366148
long period variable
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Q78366148
Summary
Q78366148 is a long-period variable star[1].
Key Facts
- Q78366148's instance of is recorded as long-period variable star[2].
- Q78366148's constellation is recorded as Dorado[3].
- Q78366148's catalog code is recorded as 2MASS J05591077-6630282[4].
- Q78366148's catalog code is recorded as OGLE LMC563.09.000021[5].
- Q78366148's catalog code is recorded as Gaia DR2 4659723166050584960[6].
- Q78366148's type of variable star is recorded as long-period variable star[7].
- Q78366148's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.72'}[8].
- Q78366148's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.51'}[9].
- Q78366148's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.97'}[10].
- Q78366148's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.014'}[11].
- Q78366148's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0075'}[12].
- Q78366148's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0851'}[13].
- Q78366148's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+280.02'}[14].
- Q78366148's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78366148's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.79496405636990'}[16].
- Q78366148's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.50784129762510'}[17].
- Q78366148's epoch is recorded as J2000.0[18].
- Q78366148's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78366148's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.612'}[20].
- Q78366148's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.705'}[21].
Body
Definition and Type
Q78366148's instance of is recorded as long-period variable star[2].