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The contribution of the thermal dust component in galactic halo rotation isexplored based on the microwave data of Planck satellite. The temperatureasymmetry of Doppler nature revealed for several edge-on galaxies at severalmicrowave frequencies is analyzed regarding the contribution of the thermaldust emission. We derive the dust contribution to the galactic halo rotationusing the data in three bands, 353GHz, 545GHz and 857GHz for two nearbygalaxies M81 and M82. The relevance of the revealed properties on the halorotation is then discussed in the context of the modified gravity theoriesproposed to describe the dark matter configurations.

On the role of dust in the microwave emission of galactic halos