In 1972 it was decided that the best way to compensate for this is to insert (and sometime remove) leap seconds, so that the difference between UTC and Earth’s rotation is kept below one second. A certain subset of astronomical and navigational/satellite applications rely on that condition being true. If this is changed, some decades-old systems, some of which may be critical infrastructure, may have to be substantially modified to account for leap seconds in some other way. The mention of GLONAS in the article is one such example.

In the international standard body responsible for UTC (ITU-R), there was up to now no sufficient majority in favor of abolishing leap seconds, due to those concerns. (Never change a running system, so to speak.) By now it has become apparent that the benefits of dropping leap seconds should vastly outweigh the potential drawbacks, at least for the next few decades. But it took some time for that realization, and probably also some older participants whose minds couldn’t be changed to die off.