  It is widely comprehended that temperature may cause phonon-exciton
scattering, enhancing the energy level's linewidth and leading to some spectrum
shifts. However, in the present paper, we suggest a different mechanism that
allows the thermal motion of the exciton's center of mass (c.m.) to affect the
magnetoexciton energies in monolayer dichalcogenides (TMDCs). By the nontrivial
but precise separation of the c.m. motion from an exciton in a monolayer TMDC
with a magnetic field, we obtain an equation for the relative motion containing
a motional Stark term proportional to the c.m. pseudomomentum, related to the
temperature of the exciton gas but neglected in the previous studies. Solving
the Schr\"odinger equation without omitting the motional Stark potential at
room temperature shows approximately a few meV thermal-magnetic shifts in the
exciton energies, significant enough for experimental detection. Moreover, this
thermal effect causes a change in exciton radius and diamagnetic coefficient
and enhances the exciton lifetime as a consequence. Surprisingly, the
thermoinduced motional Stark potential breaks the system's SO(2) symmetry,
conducting new peaks in the exciton absorption spectra at room temperature
besides those of the $s$ states. This mechanism could be extended for other
magnetoquasiparticles such as trions and biexcitons.
