Q78370077
long period variable
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Q78370077
Summary
Q78370077 is a long-period variable star[1].
Key Facts
- Q78370077's instance of is recorded as long-period variable star[2].
- Q78370077's constellation is recorded as Dorado[3].
- Q78370077's catalog code is recorded as 2MASS J05585168-6627019[4].
- Q78370077's catalog code is recorded as OGLE LMC563.09.000037[5].
- Q78370077's catalog code is recorded as Gaia DR2 4659725060145130624[6].
- Q78370077's type of variable star is recorded as long-period variable star[7].
- Q78370077's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.51'}[8].
- Q78370077's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.31'}[9].
- Q78370077's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.86'}[10].
- Q78370077's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.725'}[11].
- Q78370077's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.7759'}[12].
- Q78370077's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0266'}[13].
- Q78370077's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+312.20'}[14].
- Q78370077's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78370077's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.71548910210430'}[16].
- Q78370077's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.45053518458490'}[17].
- Q78370077's epoch is recorded as J2000.0[18].
- Q78370077's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78370077's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.763'}[20].
- Q78370077's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.304'}[21].
Body
Definition and Type
Q78370077's instance of is recorded as long-period variable star[2].