Q78373140
long period variable
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Q78373140
Summary
Q78373140 is a long-period variable star[1].
Key Facts
- Q78373140's instance of is recorded as long-period variable star[2].
- Q78373140's constellation is recorded as Dorado[3].
- Q78373140's catalog code is recorded as 2MASS J05580282-6651106[4].
- Q78373140's catalog code is recorded as OGLE LMC562.27.009506[5].
- Q78373140's catalog code is recorded as Gaia DR2 4659691009642793984[6].
- Q78373140's type of variable star is recorded as long-period variable star[7].
- Q78373140's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.97'}[8].
- Q78373140's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.73'}[9].
- Q78373140's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.12'}[10].
- Q78373140's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.206'}[11].
- Q78373140's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.2264'}[12].
- Q78373140's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1393'}[13].
- Q78373140's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+252.04'}[14].
- Q78373140's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78373140's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.51171054513530'}[16].
- Q78373140's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.85303288908800'}[17].
- Q78373140's epoch is recorded as J2000.0[18].
- Q78373140's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4500'}[19].
- Q78373140's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.856'}[20].
- Q78373140's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.562'}[21].
Body
Definition and Type
Q78373140's instance of is recorded as long-period variable star[2].