Q86437535
Mira variable star in the constellation Carina
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Q86437535
Summary
Q86437535 is a Mira variable[1].
Key Facts
- Q86437535's instance of is recorded as Mira variable[2].
- Q86437535's instance of is recorded as carbon star[3].
- Q86437535's instance of is recorded as infrared source[4].
- Q86437535's instance of is recorded as long-period variable star[5].
- Q86437535's instance of is recorded as near-infrared source[6].
- Q86437535's constellation is recorded as Carina[7].
- Q86437535's spectral class is recorded as C[8].
- Q86437535's catalog code is recorded as CGCS 2795[9].
- Q86437535's catalog code is recorded as IRAS 10331-6027[10].
- Q86437535's catalog code is recorded as [W71b] 060-15[11].
- Q86437535's catalog code is recorded as 2MASS J10345600-6042374[12].
- Q86437535's catalog code is recorded as Gaia DR2 5254321256027358976[13].
- Q86437535's catalog code is recorded as TU Car[14].
- Q86437535's catalog code is recorded as AAVSO 1031-60[15].
- Q86437535's catalog code is recorded as TIC 460730500[16].
- Q86437535's catalog code is recorded as Gaia DR3 5254321256027358976[17].
- Q86437535's type of variable star is recorded as Mira variable[18].
- Q86437535's type of variable star is recorded as long-period variable star[19].
- Q86437535's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.16'}[20].
- Q86437535's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.07'}[21].
- Q86437535's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.52'}[22].
- Q86437535's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.618682'}[23].
- Q86437535's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3443'}[24].
- Q86437535's metallicity is recorded as {'unit': '1', 'amount': '+0.8'}[25].
- Q86437535's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+158.73333244476'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], carbon star[3], infrared source[4], long-period variable star[5], and near-infrared source[6].