Q83841367
Mira variable star in the constellation Triangulum Australe
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Q83841367
Summary
Q83841367 is a Mira variable[1].
Key Facts
- Q83841367's instance of is recorded as Mira variable[2].
- Q83841367's instance of is recorded as infrared source[3].
- Q83841367's instance of is recorded as long-period variable star[4].
- Q83841367's instance of is recorded as near-infrared source[5].
- Q83841367's constellation is recorded as Triangulum Australe[6].
- Q83841367's spectral class is recorded as Me[7].
- Q83841367's catalog code is recorded as GSC 09274-04088[8].
- Q83841367's catalog code is recorded as IRAS 16353-6809[9].
- Q83841367's catalog code is recorded as ASAS J164031-6815.3[10].
- Q83841367's catalog code is recorded as 2MASS J16403406-6815055[11].
- Q83841367's catalog code is recorded as Gaia DR1 5809291916107035904[12].
- Q83841367's catalog code is recorded as Gaia DR2 5809291920414569984[13].
- Q83841367's catalog code is recorded as EF TrA[14].
- Q83841367's catalog code is recorded as AAVSO 1630-68[15].
- Q83841367's catalog code is recorded as TYC 9274-4088-1[16].
- Q83841367's catalog code is recorded as TIC 363649136[17].
- Q83841367's catalog code is recorded as Gaia DR3 5809291920414569984[18].
- Q83841367's type of variable star is recorded as long-period variable star[19].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.21'}[20].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.054'}[21].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.78'}[22].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.270'}[23].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.958'}[24].
- Q83841367's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.85146'}[25].
- Q83841367's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6107'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], infrared source[3], long-period variable star[4], and near-infrared source[5].