2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/108168Dust 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.8 pages, 4 figures, to appear in the proceedings of "Infrared Diagnostics of Galaxy Evolution"AstrophysicsA Dust Emission Model for Very Young Galaxies: Expected Properties and Far Infrared Diagnosticstext