Q78373753
long period variable
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Q78373753
Summary
Q78373753 is a long-period variable star[1].
Key Facts
- Q78373753's instance of is recorded as long-period variable star[2].
- Q78373753's constellation is recorded as Dorado[3].
- Q78373753's catalog code is recorded as 2MASS J05592847-6608285[4].
- Q78373753's catalog code is recorded as OGLE LMC563.17.000013[5].
- Q78373753's catalog code is recorded as Gaia DR2 4755811037695347968[6].
- Q78373753's type of variable star is recorded as long-period variable star[7].
- Q78373753's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.22'}[8].
- Q78373753's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.11'}[9].
- Q78373753's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.74'}[10].
- Q78373753's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.420'}[11].
- Q78373753's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.5071'}[12].
- Q78373753's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0421'}[13].
- Q78373753's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+261.17'}[14].
- Q78373753's metallicity is recorded as {'unit': '1', 'amount': '-0.50'}[15].
- Q78373753's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.86864299847290'}[16].
- Q78373753's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-66.14130312182330'}[17].
- Q78373753's epoch is recorded as J2000.0[18].
- Q78373753's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4250'}[19].
- Q78373753's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.805'}[20].
- Q78373753's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.714'}[21].
Body
Definition and Type
Q78373753's instance of is recorded as long-period variable star[2].