  We calculate the production of ultra-light axion-like particles (ALPs) in a
nearby supernova progenitor. Once produced, ALPs escape from the star and a
part of them is converted into photons during propagation in the Galactic
magnetic field. It is found that the MeV photon flux that reaches Earth may be
detectable by gamma ray telescopes for ALPs lighter than ~1 neV when Betelgeuse
undergoes oxygen and silicon burning. The dependence of the gamma ray flux on
the stellar mass is much smaller than the uncertainty that originates from the
Galactic magnetic field. If ALPs are lighter than ~0.1 neV and the supernova
progenitor is close enough to the Solar System, the gamma ray flux is
insensitive to the distance d because the ALP-photon conversion probability is
proportional to d^2. (Non-)detection of gamma rays from a supernova progenitor
with next-generation gamma ray telescopes just after pre-supernova neutrino
alerts would lead to an independent constraint on ALP parameters as stringent
as a SN 1987A limit.
