I am curious if there is still enough disk remaining to degrade its orbit, or if there is enough T-Tauri like tantrums that would cause migration, or both. At such an early age for the system, perhaps migration is likely.

[V838 Mon comes to mind ever since Cress et. al. proposed, in their paper, the idea that the flashes (light echos) may have been caused by planetary plunges into the star.]

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Lighten up! This is a stellar board!