\begin{document}$ n+1 $\end{document}. For the leading order(s), the time delay, as well as the difference between the time delays of two types of relativistic signals, is shown to take a universal form for all SSS spacetimes. This universal form depends on the mass M and a post-Newtonian parameter \begin{document}$ \gamma $\end{document} of the spacetime. The analytical result is numerically verified using the central black hole of galaxy M87 as the gravitational lensing center."> Universal time delay in static spherically symmetric spacetimes for null and timelike signals -
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