SUMMARY
Astronauts do not observe the Earth's rotation due to its relatively slow spin of approximately 460 m/s at the equator, which is not noticeable from their vantage point in low Earth orbit (250-350 km altitude). The Earth orbits the Sun at about 30 km/s, but this speed is unrelated to the perception of rotation. The discussion highlights the conservation of angular momentum as a fundamental principle explaining why celestial bodies, including planets and galaxies, spin. The current understanding of planetary spin is largely based on the Nebular Model, which describes the formation of the solar system from a rotating cloud of gas and dust.
PREREQUISITES
- Understanding of angular momentum and its conservation
- Familiarity with the Nebular Model of solar system formation
- Basic knowledge of planetary motion and orbital mechanics
- Awareness of the differences between prograde and retrograde rotation
NEXT STEPS
- Research the Nebular Model and its implications for planetary formation
- Study the principles of angular momentum in astrophysics
- Explore the differences between prograde and retrograde motion in celestial bodies
- Investigate the rotation speeds of other planets and their formation theories
USEFUL FOR
Astronomy enthusiasts, astrophysicists, educators, and students interested in planetary science and the dynamics of celestial bodies.