SUMMARY
The planets in our solar system are not locked in their orbits indefinitely; they are influenced by the Sun's gravitational pull and its mass loss over time. As the Sun burns fuel, it gradually loses mass, causing the planets to slowly drift away from it. In approximately a few billion years, the Sun will expand into a red giant, which will engulf the inner planets, altering their orbits significantly.
PREREQUISITES
- Understanding of gravitational forces and their effects on celestial bodies
- Basic knowledge of stellar evolution and the life cycle of stars
- Familiarity with orbital mechanics and planetary motion
- Awareness of the concept of mass loss in stars
NEXT STEPS
- Research the effects of solar mass loss on planetary orbits
- Study the life cycle of stars, focusing on the transition to red giants
- Explore gravitational interactions in multi-body systems
- Learn about the long-term evolution of the solar system
USEFUL FOR
Astronomy enthusiasts, astrophysicists, and students studying celestial mechanics and stellar evolution will benefit from this discussion.