Q78367100
long period variable
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Q78367100
Summary
Q78367100 is a long-period variable star[1].
Key Facts
- Q78367100's instance of is recorded as long-period variable star[2].
- Q78367100's constellation is recorded as Dorado[3].
- Q78367100's catalog code is recorded as 2MASS J06025964-6613469[4].
- Q78367100's catalog code is recorded as OGLE LMC570.31.004941[5].
- Q78367100's catalog code is recorded as Gaia DR2 5476386050356254080[6].
- Q78367100's type of variable star is recorded as long-period variable star[7].
- Q78367100's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.32'}[8].
- Q78367100's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.17'}[9].
- Q78367100's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.78'}[10].
- Q78367100's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.484'}[11].
- Q78367100's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.6302'}[12].
- Q78367100's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0119'}[13].
- Q78367100's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+251.07'}[14].
- Q78367100's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78367100's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.74843024914950'}[16].
- Q78367100's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.22972129695830'}[17].
- Q78367100's epoch is recorded as J2000.0[18].
- Q78367100's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4000'}[19].
- Q78367100's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.023'}[20].
- Q78367100's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.514'}[21].
Body
Definition and Type
Q78367100's instance of is recorded as long-period variable star[2].