Your "correct" version on the other hand, leaves more questions than answers, not least of which being how do we ever get 46B ly distance in something 13.8B years old. Then you have to cover the expansion, relativity, and hey presto you've written the article. Just skimming the other comments here makes it clear it's not a topic that's well understood or intuitive.
Clickbait it ain't, and the title is a very fair question.
I'm really disappointed to see this the top voted HN answer right now...
https://en.wikipedia.org/wiki/Hubble%27s_law
"(...) the notion of the universe expanding at a calculable rate was first derived from the general relativity equations in 1922 by Alexander Friedmann"
The space expands. It's been known for a long time.
We might not know why exactly this happens and there is still some discussion about ultimate fate of the universe although prevalent theory is that it will expand at an ever faster rate until every molecule will be torn from each other and matter will no longer be able to form.
When tracks start moving as well it gets mind bending, and no longer intuitive. Now we have multiple scenarios where the combination of track movement (universe expansion), and train movement result in it being "obvious" you have to exceed C somewhere, which we're told is impossible. Otherwise how can the distances end up where they are. It's between these two points most non-physicists stop as it starts to feel deeply contradictory.
Sure he goes for clickbaity articles now and then, but he's pretty good at them in my experience, and your summary is both incorrect (there is no "current" over that distance scale) and leaves all explanation out.
> In physical cosmology, peculiar velocity refers to the components of a galaxy's velocity that deviate from the Hubble flow. ....
> Galaxies are not distributed evenly throughout observable space, but are typically found in groups or clusters, where they have a significant gravitational effect on each other. Velocity dispersions of galaxies arising from this gravitational attraction are usually in the hundreds of kilometers per second, but they can rise to over 1000 km/s in rich clusters.
-- https://en.wikipedia.org/wiki/Peculiar_velocity
Granted, 1000 km/s isn't even 1% of light speed, so clearly this motion couldn't contribute much to a distant object's recession.
The metaphor I normally see is a balloon being blown up.
This comment heavily reminds me of the mannerisms of professors that have the mentality of "I deeply understand this subject from years of past studies, so you should be able to understand it from my vague and half assed explanation alone".
The correct way to state it would be to say: "We are seing things that are currently 46B light years away but since they are so far away we see them as they were 13.8B years ago when they were much closer than they are now."
I see absolutely nothing difficult about that statement unless you really need to create some piece of content and you figured out you will make something difficult so that you can then make it a little bit easier and be a hero.