The Earth's precession is a function of the Earth's oblateness. In simple terms, right now Polaris is the Earth's "North Star," but it wasn't always that way, nor will it always be that way in the future. The Earth's celestial poles gradually rotate in a circle with respect to the stars every 26,000 years or so. This axial "precession" wouldn't happen if the Earth was completely spherical. Scientists have known about Earth's precession to some degree or another for thousands of years, believe it or not. (General relatively [GR] isn't so critical here. You can model it with Newtonian mechanics quite well. But the oblateness is still a key factor when modeling.)
The effects of Earth's oblateness is probably most pronounced in anything dealing with low-Earth-orbit (LEO) satellites. And this is also one application where general relativity (GR) is also critical. For example, GPS, GLONASS, or other global positioning satellite systems absolutely must account for both.
A while ago, I wrote a computer program to track satellites based on their orbital elements (not dissimilar to what
heavens-above.com implements). The program does not take GR into account and models orbits as Kepplerian. I still had to model ground locations (i.e., observing locations) based on Earth being a oblate spheroid, not a sphere. Had I modeled Earth as a sphere, it would have caused significant pointing errors. To elaborate, there are several different types of latitude: geocentric latitude and geodetic latitude, being most used. It's often important to distinguish between the two (or any other type). (See more:
https://en.wikipedia.org/wiki/Latitude#Auxiliary_latitudes.)
Geodetic latitude [itex]( \phi)[/itex] and geocetric latitude [itex](\theta)[/itex].
If I'm not mistaken, most maps use geodetic latitude which takes into account the Earth being an ellipsoid. So that's another application where the Earth's oblateness is considered: maps.