SUMMARY
Unattended objects in orbit, such as dead satellites and near-Earth objects (NEOs), maintain their orbital inclination due to inertia unless acted upon by external forces. While atmospheric drag primarily causes orbital decay, it significantly affects only low-altitude satellites. Other factors, like the Earth's oblateness and solar radiation pressure, induce minor precession in the orbital plane. Over extended periods, the Moon's gradual energy transfer results in a slow outward drift of its orbit.
PREREQUISITES
- Understanding of orbital mechanics
- Familiarity with atmospheric drag effects on satellites
- Knowledge of Earth's oblateness and its influence on orbits
- Basic concepts of solar radiation pressure
NEXT STEPS
- Research the effects of atmospheric drag on satellite orbits
- Study the principles of orbital precession and its causes
- Explore the long-term effects of lunar energy transfer on Earth's orbit
- Learn about the dynamics of near-Earth objects (NEOs) and their behavior in orbit
USEFUL FOR
Aerospace engineers, astrophysicists, satellite operators, and anyone interested in the dynamics of orbital decay and satellite behavior.