• Sun: The sun could be perturbed from its current position, altering its gravitational influence on the entire solar system.
• Inner Planets: Mercury, Venus, Earth, and Mars would face significant risks due to their proximity, potentially being ejected from their orbits or colliding with one another.
• Outer Planets: Jupiter, Saturn, Uranus, and Neptune would experience changes in their orbits. Given their massive sizes, their gravitational perturbations could cascade, affecting smaller bodies and moons.
• Orbital Disruptions: Altered orbits of outer planets could destabilize the Kuiper Belt and Oort Cloud, sending comets and asteroids into the inner solar system.
• Asteroid & Comet Trajectories: The gravitational forces could redirect asteroids and comets, increasing the likelihood of collisions with planets, including Earth.
• Tidal Effects: Close encounters could induce tidal forces, leading to geological and oceanic disruptions on planets and moons.
• Solar System Configuration: The stability of the entire solar system could be compromised, with objects possibly being captured by the passing star or scattered into interstellar space.
• Habitability Changes: Earth’s orbit could shift, leading to drastic climate changes and possibly rendering it uninhabitable.

These interactions would unfold over extended periods, ranging from thousands to millions of years, depending on the specifics of the star’s trajectory.

Energy Release from Collisions

 When ordinary matter interacts with dark matter, such collisions typically result in the annihilation or scattering of dark matter particles, producing high-energy particles such as gamma rays, neutrinos, or potentially new, undiscovered particles.

Technological Challenges

• Detection and Measurement: Dark matter’s weak interaction with ordinary matter complicates direct observation and measurement of collision events.
• Particle Conversion: Energy released often manifests as high-energy particles that are difficult to capture and convert into usable forms like electricity or propulsion.
• Safety Concerns: The high-energy nature of particles emitted during collisions poses radiation hazards and challenges in spacecraft shielding and safety.
• Current Limitations: Existing technologies lack the sensitivity and precision required to reliably detect and manipulate dark matter interactions for energy purposes. Advances in detection methods and theoretical understanding are ongoing but have not yet reached a stage where practical applications for space travel are feasible.

Additional Considerations

• Fundamental Research: Understanding dark matter properties and interactions is crucial for advancing technologies that could harness its energy potential.
• Exploration Missions: Future space missions may incorporate instruments designed to detect and study dark matter interactions, contributing to our knowledge and potential applications.