  We release the first grid of stellar limb-darkening coefficients (LDCs) and
intensity profiles (IPs) computed by the consortium of the PLAnetary Transits
and Oscillations of stars (PLATO), the next medium-class (M3) mission under
development by the European Space Agency (ESA) to be launched in 2026. We have
performed spectral synthesis with \texttt{TurboSpectrum} on a grid of
\texttt{MARCS} model atmospheres. Finally, we adopted \texttt{ExoTETHyS} to
convolve the high-resolution spectra ($R=2\times10^5$) with the
state-of-the-art response functions for all the PLATO cameras, and computed the
LDCs that best approximate the convolved IPs. In addition to the PLATO
products, we provide new LDCs and IPs for the Kepler mission, based on the same
grid of stellar atmospheric models and calculation procedures. The data can be
downloaded from the following link:
\url{https://doi.org/10.5281/zenodo.7339706}.
