MZ Herculis
long period variable
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MZ Herculis
Summary
MZ Herculis is a long-period variable star[1].
Key Facts
- MZ Herculis's instance of is recorded as long-period variable star[2].
- MZ Herculis's instance of is recorded as infrared source[3].
- MZ Herculis's instance of is recorded as near-infrared source[4].
- MZ Herculis's constellation is recorded as Hercules[5].
- MZ Herculis's spectral class is recorded as M6[6].
- MZ Herculis's catalog code is recorded as BD+18 3826[7].
- MZ Herculis's catalog code is recorded as GSC 01592-00520[8].
- MZ Herculis's catalog code is recorded as DO 17049[9].
- MZ Herculis's catalog code is recorded as HD 229550[10].
- MZ Herculis's catalog code is recorded as IRAS 18460+1903[11].
- MZ Herculis's catalog code is recorded as IRC +20376[12].
- MZ Herculis's catalog code is recorded as RAFGL 5298S[13].
- MZ Herculis's catalog code is recorded as 2MASS J18481683+1906494[14].
- MZ Herculis's catalog code is recorded as Gaia DR2 4518531171370165504[15].
- MZ Herculis's catalog code is recorded as MZ Her[16].
- MZ Herculis's catalog code is recorded as TIC 348620516[17].
- MZ Herculis's catalog code is recorded as Gaia DR3 4518531171370165504[18].
- MZ Herculis's catalog code is recorded as TYC 1592-520-1[19].
- MZ Herculis's catalog code is recorded as AAVSO 1843+19[20].
- MZ Herculis's type of variable star is recorded as SRb semi-regular variable star[21].
- MZ Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.850'}[22].
- MZ Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.28'}[23].
- MZ Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.875'}[24].
- MZ Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.505'}[25].
- MZ Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.027'}[26].
Body
Designation and Status
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].
History and Context
Catalog codes include BD+18 3826[7], GSC 01592-00520[8], DO 17049[9], HD 229550[10], IRAS 18460+1903[11], and IRC +20376[12].