  Multiple stellar populations (MPs) in most star clusters older than 2 Gyr, as
seen by lots of spectroscopic and photometric studies, have led to a
significant challenge to the traditional view of star formation. In this field,
space-based instruments, in particular the Hubble Space Telescope (HST), have
made a breakthrough as they significantly improved the efficiency of detecting
MPs in crowding stellar fields by images. The China Space Station Telescope
(CSST) and the HST are sensitive to a similar wavelength interval, but it
covers a field of view which is about 5-8 times wider than that of HST. One of
its instruments, the Multi-Channel Imager (MCI), will have multiple filters
covering a wide wavelength range from NUV to NIR, making the CSST a potentially
powerful tool for studying MPs in clusters. In this work, we evaluate the
efficiency of the designed filters for the MCI/CSST in revealing MPs in
different color-magnitude diagrams (CMDs). We find that CMDs made with MCI/CSST
photometry in appropriate UV filters are powerful tools to disentangle stellar
populations with different abundances of He, C, N, O and Mg. On the contrary,
the traditional CMDs are blind to multiple populations in globular clusters
(GCs). We show that CSST has the potential of being the spearhead instrument
for investigating MPs in GCs in the next decades.
