SUMMARY
The Hubble Space Telescope orbits Earth at an altitude of 615 km, resulting in an orbital radius of approximately 7000 km when combined with Earth's radius. The period of the telescope's orbit can be calculated using Kepler's Third Law, specifically the formula P² = (4π²r³)/(GM), where G is the gravitational constant (6.67259 x 10^-11) and M is Earth's mass (5.9742 x 10^24 kg). The calculated period is approximately 84.43 minutes, aligning with typical low Earth orbit (LEO) durations.
PREREQUISITES
- Understanding of Kepler's Third Law of planetary motion
- Familiarity with gravitational constant (G) and Earth's mass
- Basic knowledge of orbital mechanics
- Ability to perform unit conversions and calculations in physics
NEXT STEPS
- Research the application of Kepler's Laws in different orbital scenarios
- Learn about gravitational forces and their impact on satellite orbits
- Study the calculations involved in determining orbital periods for various altitudes
- Explore the physics of low Earth orbit (LEO) satellites and their operational parameters
USEFUL FOR
Astronomy students, aerospace engineers, and anyone interested in satellite dynamics and orbital mechanics will benefit from this discussion.