Q89690249
Mira variable star in the constellation Horologium
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Q89690249
Summary
Q89690249 is a Mira variable[1].
Key Facts
- Q89690249's instance of is recorded as Mira variable[2].
- Q89690249's instance of is recorded as infrared source[3].
- Q89690249's instance of is recorded as long-period variable star[4].
- Q89690249's instance of is recorded as near-infrared source[5].
- Q89690249's constellation is recorded as Horologium[6].
- Q89690249's spectral class is recorded as M[7].
- Q89690249's catalog code is recorded as CSV 213[8].
- Q89690249's catalog code is recorded as IRAS 02205-6318[9].
- Q89690249's catalog code is recorded as UCAC2 3826350[10].
- Q89690249's catalog code is recorded as UCAC4 135-002140[11].
- Q89690249's catalog code is recorded as 2MASS J02214814-6305016[12].
- Q89690249's catalog code is recorded as ASAS J022148-6305.1[13].
- Q89690249's catalog code is recorded as Gaia DR2 4701206026073986560[14].
- Q89690249's catalog code is recorded as TY Hor[15].
- Q89690249's catalog code is recorded as TIC 369771580[16].
- Q89690249's catalog code is recorded as Gaia DR3 4701206026073986560[17].
- Q89690249's type of variable star is recorded as long-period variable star[18].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.05'}[19].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.17'}[20].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.86'}[21].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.27'}[22].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.32'}[23].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.90'}[24].
- Q89690249's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.935169'}[25].
- Q89690249's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8285'}[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].