For a slowly moving particle in the weak-field approximation, and terms containing two spatial velocities may be neglected. The spatial geodesic equation reduces to
For , the Levi-Civita connection is
Hence the Newtonian limit of general relativity is
Along the radial curve at fixed , the spatial line element is . To first order,
so
A radial null geodesic satisfies
so for the outgoing ray
The coordinate-time interval is therefore
The stationary observer at measures proper time . Hence
Put . Expanding the quotient consistently to first order gives
Thus
Because as ,
This local limit is the expected speed of a massless particle measured in a freely falling local inertial frame; the finite-interval effective velocity combines nonlocal length and clock comparisons.

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