Q78367590
long period variable
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Q78367590
Summary
Q78367590 is a long-period variable star[1].
Key Facts
- Q78367590's instance of is recorded as long-period variable star[2].
- Q78367590's constellation is recorded as Dorado[3].
- Q78367590's catalog code is recorded as 2MASS J06010438-6605219[4].
- Q78367590's catalog code is recorded as OGLE LMC571.06.000015[5].
- Q78367590's catalog code is recorded as Gaia DR2 5476399828611662336[6].
- Q78367590's type of variable star is recorded as long-period variable star[7].
- Q78367590's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.27'}[8].
- Q78367590's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.45'}[9].
- Q78367590's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.37'}[10].
- Q78367590's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.643'}[11].
- Q78367590's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.2187'}[12].
- Q78367590's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0880'}[13].
- Q78367590's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+301.33'}[14].
- Q78367590's metallicity is recorded as {'unit': '1', 'amount': '+0.00'}[15].
- Q78367590's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.26834763655260'}[16].
- Q78367590's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.08947289339430'}[17].
- Q78367590's epoch is recorded as J2000.0[18].
- Q78367590's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4750'}[19].
- Q78367590's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.953'}[20].
- Q78367590's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.026'}[21].
Body
Definition and Type
Q78367590's instance of is recorded as long-period variable star[2].