Q78360613
long period variable
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Q78360613
Summary
Q78360613 is a long-period variable star[1].
Key Facts
- Q78360613's instance of is recorded as long-period variable star[2].
- Q78360613's constellation is recorded as Dorado[3].
- Q78360613's catalog code is recorded as 2MASS J06012071-6616021[4].
- Q78360613's catalog code is recorded as OGLE LMC570.32.004255[5].
- Q78360613's catalog code is recorded as Gaia DR2 5476379315847465984[6].
- Q78360613's type of variable star is recorded as long-period variable star[7].
- Q78360613's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.70'}[8].
- Q78360613's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.51'}[9].
- Q78360613's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.08'}[10].
- Q78360613's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.860'}[11].
- Q78360613's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.9379'}[12].
- Q78360613's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0220'}[13].
- Q78360613's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+307.64'}[14].
- Q78360613's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78360613's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+90.33633876657920'}[16].
- Q78360613's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.26725478956720'}[17].
- Q78360613's epoch is recorded as J2000.0[18].
- Q78360613's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4500'}[19].
- Q78360613's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.806'}[20].
- Q78360613's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.334'}[21].
Body
Definition and Type
Q78360613's instance of is recorded as long-period variable star[2].