Q78367220
long period variable
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Q78367220
Summary
Q78367220 is a long-period variable star[1].
Key Facts
- Q78367220's instance of is recorded as long-period variable star[2].
- Q78367220's constellation is recorded as Dorado[3].
- Q78367220's catalog code is recorded as 2MASS J06032103-6619004[4].
- Q78367220's catalog code is recorded as OGLE LMC570.31.004923[5].
- Q78367220's catalog code is recorded as Gaia DR2 5284228114029803136[6].
- Q78367220's type of variable star is recorded as long-period variable star[7].
- Q78367220's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.65'}[8].
- Q78367220's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.42'}[9].
- Q78367220's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.84'}[10].
- Q78367220's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.921'}[11].
- Q78367220's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.9308'}[12].
- Q78367220's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0290'}[13].
- Q78367220's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+323.58'}[14].
- Q78367220's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78367220's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.83763831374830'}[16].
- Q78367220's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.31680891208770'}[17].
- Q78367220's epoch is recorded as J2000.0[18].
- Q78367220's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4500'}[19].
- Q78367220's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.545'}[20].
- Q78367220's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.513'}[21].
Body
Definition and Type
Q78367220's instance of is recorded as long-period variable star[2].