  Dust plays crucial roles in galaxy formation and evolution. In the early
epoch of galaxy evolution dust is only supplied by supernovae (SNe). With the
aid of a new physical model of dust production by SNe, we constructed a model
of dust emission from forming galaxies. We show the evolution of the spectral
energy distribution (SED). Then we adopt this model to a local starbursting
dwarf galaxy SBS 0335$-$052. Further we discuss the SEDs of high redshift
galaxies, and consider their observational feasibility.
