  We present the hydrodynamic model of Type IIP SN 2020jfo with the unusually
short (nearly 60 days) light curve plateau. The model suggests the explosion of
about 8 Msun red supergiant that ejected nearly 6 Msun with the energy of about
0.8x10^51 erg. The presupernova wind density turns out highest among known SNe
IIP. Yet the presupernova was not embedded into a very dense confined
circumstellar shell that is a feature of some Type IIP supernovae, so the
circumstellar interaction in close environment does not contribute noticeably
to the initial (about 10 days) bolometric luminosity. Despite uncommon
appearance SN 2020jfo turns out similar to SN 1970G in the V-band light curve,
photospheric velocities, and, possibly, luminosity as well.
