Q77364253
Mira variable star in the constellation Telescopium
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Q77364253
Summary
Q77364253 is a Mira variable[1].
Key Facts
- Q77364253's instance of is recorded as Mira variable[2].
- Q77364253's instance of is recorded as red supergiant[3].
- Q77364253's instance of is recorded as infrared source[4].
- Q77364253's instance of is recorded as long-period variable star[5].
- Q77364253's instance of is recorded as near-infrared source[6].
- Q77364253's constellation is recorded as Telescopium[7].
- Q77364253's spectral class is recorded as M2Ib:ep[8].
- Q77364253's catalog code is recorded as CF 18291[9].
- Q77364253's catalog code is recorded as GCRV 68624[10].
- Q77364253's catalog code is recorded as IRAS 18456-4957[11].
- Q77364253's catalog code is recorded as ASAS J184931-4954.5[12].
- Q77364253's catalog code is recorded as 2MASS J18493171-4954295[13].
- Q77364253's catalog code is recorded as Gaia DR2 6655927830980413184[14].
- Q77364253's catalog code is recorded as BH Tel[15].
- Q77364253's catalog code is recorded as Gaia DR3 6655927830980413184[16].
- Q77364253's catalog code is recorded as TIC 292217772[17].
- Q77364253's type of variable star is recorded as long-period variable star[18].
- Q77364253's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.80'}[19].
- Q77364253's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.469'}[20].
- Q77364253's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.680'}[21].
- Q77364253's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.237'}[22].
- Q77364253's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.200472'}[23].
- Q77364253's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2204'}[24].
- Q77364253's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.0'}[25].
- Q77364253's metallicity is recorded as {'unit': '1', 'amount': '-0.45'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], red supergiant[3], infrared source[4], long-period variable star[5], and near-infrared source[6].