Exploring Pluto’s Mysterious Formation: The ‘Kiss And Capture’ Theory

NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute/Wikimedia Commons

In the vast expanse of our solar system, Pluto and its largest moon, Charon, engage in a celestial mystery that has long puzzled scientists. Recent research introduces the ‘kiss and capture’ theory, which offers a fresh perspective on their relationship. Wondering what this means? Here’s everything you need to know about the Pluto-Chiron bond and its formation theories.

The Unusual Pluto-Charon Duo

Lanthanum-138/Wikimedia Commons

Pluto and Charon are a remarkable pair, with Charon’s diameter being just over half that of Pluto. This significant size ratio results in both bodies orbiting a shared center of mass in the space between them rather than within either body, a configuration that is rare among known planetary systems. 

Traditional Theories Challenged

Earth: NASA, Moon: Gregory H. Revera, Charon: NASA/JHUAPL/SWRI/ Wikimedia Commons

Previously, it was believed that Charon formed from a massive collision, similar to Earth’s moon’s origin. However, this hypothesis doesn’t fully account for the distinct characteristics observed in the Pluto-Charon system. The need for a more fitting explanation became evident.

Introducing The ‘Kiss And Capture’ Theory

NASA Hubble/Wikimedia Commons

Most recently, the ‘kiss and capture’ theory proposed a gentler cosmic event to explain Pluto-Charon’s formation. Charon grazed Pluto, briefly merging into a celestial snowman before separating into orbit. Though a compelling hypothesis, it’s one of several under investigation, with ongoing research evaluating its alignment with observed planetary characteristics.

The Role Of Material Strength

PlanetUser and AstroChara/Wikimedia Commons

This theory is key to considering Pluto and Charon’s material composition. Unlike larger planetary bodies that behave fluidly during collisions, these worlds possess structural integrity. Their strength allows them to withstand these encounters without disintegrating.

Implications For Subsurface Oceans

NASA/JPL/Solar System Simulator/Wikimedia Commons

Researchers say the gentle collision would have generated internal heat, potentially forming subsurface oceans on both bodies. The heat from the impact, combined with tidal forces as Charon moved away, could have maintained these oceans over geological timescales.

Supporting Evidence From Computer Simulations

Dtvardovskyi/Wikimedia Commons

Advanced computer models support this theory, demonstrating that such an encounter could result in the current orbits and characteristics of Pluto and Charon. These simulations consider factors like spin rates, impact angles, and material properties, which provide a comprehensive understanding of the event.

Surface As A Marker

NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Wikimedia Commons

Distinct geological features on Pluto and Charon, such as fractures and ice flows, may serve as records of their early interactions. By analyzing these formations, scientists reconstruct past thermal events and impact histories to understand the broader mechanisms.

Other Geological Features As Clues

NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Wikimedia Commons

The geographical depths of Pluto and Charon exhibit more features that align with this theory. For instance, tectonic structures and possible cryovolcanic activity could be remnants of their ancient close encounter’s internal heating and stresses.

Tidal Forces And Binary System Formation

Dr. R. Albrecht, ESA/ESO Space Telescope European Coordinating Facility; NASA/Wikimedia Commons

Tidal forces played a vital role in Pluto and Charon’s orbital evolution, gradually shifting Charon into a synchronized rotation. This process likely shaped their long-term stability and could explain similar dynamics in other binary systems.

A Common Event In The Kuiper Belt

WilyD/Wikimedia Commons

Interestingly, many large Kuiper Belt objects possess sizable moons. This observation raises the possibility that ‘kiss and capture’ events were common in the early solar system, contributing to the forming of other binary systems beyond Pluto and Charon.