  We present the distance priors from the finally released $Planck~
\textrm{TT,TE,EE}+\textrm{lowE}$ data in 2018. The uncertainties are around
$40\%$ smaller than those from $Planck$ 2015 TT$+$lowP. In order to check the
validity of these new distance priors, we adopt the distance priors to
constrain the cosmological parameters in different dark energy models,
including the $\Lambda$CDM model, the $w$CDM model and the CPL model, and
conclude that the distance priors provide consistent constraints on the
relevant cosmological parameters compared to those from the full $Planck$ 2018
data release.
