A New Theory on How Pluto Acquired Its Largest Moon
Previous models often treated these bodies as fluids during collisions, which is not accurate for small rocky and icy objects. The new study emphasizes that Pluto and Charon’s collision happened slowly enough that their icy and rocky compositions behaved more like solid materials under stress. This slower impact led to heat being deposited into Pluto, potentially triggering new geological activity. As Charon separated, it began to slowly migrate outward, shaping their current orbital dynamics, where both bodies orbit a shared center of gravity.
This “kiss-and-capture” event may not be unique to Pluto and Charon. The researchers suggest that similar collisions could have been common across the Kuiper Belt during the solar system’s early formation. Many of the largest icy bodies found in this region could have formed through similar interactions, leading to the creation of moons in a more gradual and less destructive way than previously thought. This finding challenges longstanding assumptions about moon formation and opens new avenues for understanding the broader dynamics of the outer solar system.
Overall, this theory shifts the way scientists think about moon formation in the Kuiper Belt, highlighting how smaller bodies like Pluto and Charon create moons through slow, steady interactions rather than violent collisions. It also provides new insights into the geological history of Pluto and Charon and their possible subsurface activity.
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