Q78367102
long period variable
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Q78367102
Summary
Q78367102 is a long-period variable star[1].
Key Facts
- Q78367102's instance of is recorded as long-period variable star[2].
- Q78367102's constellation is recorded as Dorado[3].
- Q78367102's catalog code is recorded as 2MASS J05585255-6648130[4].
- Q78367102's catalog code is recorded as OGLE LMC563.01.000024[5].
- Q78367102's catalog code is recorded as Gaia DR2 4659690013210331776[6].
- Q78367102's type of variable star is recorded as long-period variable star[7].
- Q78367102's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.39'}[8].
- Q78367102's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.21'}[9].
- Q78367102's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.77'}[10].
- Q78367102's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.613'}[11].
- Q78367102's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.6866'}[12].
- Q78367102's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0580'}[13].
- Q78367102's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+279.29'}[14].
- Q78367102's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78367102's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.71904081032660'}[16].
- Q78367102's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.80360209857550'}[17].
- Q78367102's epoch is recorded as J2000.0[18].
- Q78367102's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4000'}[19].
- Q78367102's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.823'}[20].
- Q78367102's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.512'}[21].
Body
Definition and Type
Q78367102's instance of is recorded as long-period variable star[2].