Q78372236
long period variable
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Q78372236
Summary
Q78372236 is a long-period variable star[1].
Key Facts
- Q78372236's instance of is recorded as long-period variable star[2].
- Q78372236's constellation is recorded as Dorado[3].
- Q78372236's catalog code is recorded as 2MASS J05572237-6619158[4].
- Q78372236's catalog code is recorded as OGLE LMC563.10.006609[5].
- Q78372236's catalog code is recorded as Gaia DR2 4659729698709710848[6].
- Q78372236's type of variable star is recorded as long-period variable star[7].
- Q78372236's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.78'}[8].
- Q78372236's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.59'}[9].
- Q78372236's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.17'}[10].
- Q78372236's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.963'}[11].
- Q78372236's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0251'}[12].
- Q78372236's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0552'}[13].
- Q78372236's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+311.62'}[14].
- Q78372236's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78372236's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.34324977632110'}[16].
- Q78372236's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.32108471769440'}[17].
- Q78372236's epoch is recorded as J2000.0[18].
- Q78372236's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78372236's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.557'}[20].
- Q78372236's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.472'}[21].
Body
Definition and Type
Q78372236's instance of is recorded as long-period variable star[2].