Q79863263
Mira variable star in the constellation Musca
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Q79863263
Summary
Q79863263 is a Mira variable[1].
Key Facts
- Q79863263's instance of is recorded as Mira variable[2].
- Q79863263's instance of is recorded as infrared source[3].
- Q79863263's instance of is recorded as long-period variable star[4].
- Q79863263's instance of is recorded as near-infrared source[5].
- Q79863263's constellation is recorded as Musca[6].
- Q79863263's spectral class is recorded as M6[7].
- Q79863263's catalog code is recorded as IRAS 13455-6819[8].
- Q79863263's catalog code is recorded as UCAC2 2005788[9].
- Q79863263's catalog code is recorded as UCAC4 108-077509[10].
- Q79863263's catalog code is recorded as 2MASS J13492029-6834140[11].
- Q79863263's catalog code is recorded as Gaia DR2 5850238455010703744[12].
- Q79863263's catalog code is recorded as AX Mus[13].
- Q79863263's catalog code is recorded as TIC 429508126[14].
- Q79863263's catalog code is recorded as Gaia DR3 5850238455010703744[15].
- Q79863263's type of variable star is recorded as Mira variable[16].
- Q79863263's type of variable star is recorded as SRb semi-regular variable star[17].
- Q79863263's type of variable star is recorded as long-period variable star[18].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.80'}[19].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.61'}[20].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.12'}[21].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.908'}[22].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.16'}[23].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.715'}[24].
- Q79863263's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.777509'}[25].
- Q79863263's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.541'}[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].