The Mystery of TOI-4860
How planets form is by no means an exact science, there's a general agreed framework, but even this occasionally falls foul of actual observations, and that's what happened when scientists actually went out looking for model breaking examples.
In this case, the theory suggests that small low mass stars can't have had enough material to create large gas giants, as most of the gas would have ran out in the creation of the star, however TOI-4860b begs to differ, a super Jupiter type planet almost one third of the mass of the host star puzzles the team in quite how it got there.
It's possible of course that such a large planet was captured somehow, but investigation into the planets makeup has shown it's high in metallicity, as is the star itself, so it looks like both were made from the same accretion disk.
The scientists involve suspect the high metallicity could be the clue, that in some way this has accelerated the process of forming gas giants where otherwise it would not have occurred.
If this is true, it could add a new dimension to the model of planet formation, and hint at new processes that ultimately lead to Jupiter type planets. Of course, one planet/star doesn't make a theory, but the team will continue their work looking at such scenarios to strengthen the evidence for such a mechanism.








