Sputnik Planitia is the bright nitrogen ice deposit within the larger Sputnik Basin, which is part of Tombaugh Regio. Tombaugh Regio encompasses both the western lobe (Sputnik Planitia) and the eastern lobe of Pluto's heart-shaped feature.
Sputnik Planitia is located near Pluto's equator, which is unusual for a large impact basin. Typically, such features migrate toward the poles due to mass redistribution, but the basin's placement suggests a mass positive rather than a mass negative.
The 'splat' theory suggests that Sputnik Planitia formed from a large, oblique impact that hit Pluto at a glancing angle, creating an elliptical crater. This theory challenges the idea that a subsurface ocean is responsible for the basin's stability.
The presence of a subsurface ocean could explain the mass positive at Sputnik Planitia, as water is denser than ice. This would stabilize the basin near the equator, but other explanations, like a buried rocky core, are also possible.
The ridge trough system is the oldest feature on Pluto's surface, with Sputnik Planitia forming later and overprinting it. This suggests a complex geological history spanning billions of years.
Pluto and Charon likely formed from a giant impact, similar to the Earth-Moon system. This impact would have created the binary system, with Charon tidally locking to Pluto relatively quickly after the collision.
Computer modeling, such as smooth particle hydrodynamics (SPH) simulations, helps scientists simulate impacts and predict how features like Sputnik Planitia might have formed. These models provide insights into Pluto's history but are approximations of real-world processes.
Debris from the impact likely scattered across Pluto and possibly reached Charon. Some of this material could still be present in the system, though tracking its exact distribution requires further exploration.
A Pluto orbiter would provide detailed gravity and topography data, helping to confirm whether a subsurface ocean or a buried rocky core is responsible for the mass anomaly at Sputnik Planitia.
The 'splat' theory could be applied to other binary systems in the Kuiper Belt, such as Eris or Haumea, which have complex formations and multiple satellites. Understanding these systems could provide insights into their impact histories.
This week, we investigate the mysteries of Pluto's iconic heart-shaped feature. We explore recent research on the origins of the Sputnik Planitia region and what it can tell us about whether or not the dwarf planet has a subsurface ocean. Our guest, Adeene Denton from the University of Arizona, discusses her team's work investigating oblique impact basins, or "splats," and their implications for planetary formation. Then Bruce Betts, chief scientist at The Planetary Society, joins host Sarah Al-Ahmed for a roundup of the most significant impacts in our Solar System in What's Up.
Discover more at: https://www.planetary.org/planetary-radio/2024-pluto-splat)
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