
Fragments and Heat: Giant Impacts May Not Forge Oceans on Icy Moons
New simulations of head-on collisions between icy moons show that while shattering a moon injects heat, the increased surface area of debris causes rapid heat loss during reaccretion and the reorganized interior often loses its insulating layer; as a result, smaller moons are unlikely to develop long-lived oceans, while larger moons may preserve or even thicken existing ones, but giant impacts rarely create new oceans that wouldn’t have formed otherwise; heat delivery does not equal heat retention over billions of years.













