Math Problem Statement
A satellite is put into orbit above the Earth (the mass of the Earth is equal to 5.97 * 10^24 kg). It is released at a height of 35,000 km above the Earth's surface. When it is released it is traveling at 3100 m/s. Would the satellite have a stable orbit?
Solution
To determine if the satellite has a stable orbit, we must check if its orbital velocity is sufficient to balance the gravitational force at the given height. Here's how to analyze this step-by-step:
1. Gravitational Force and Required Orbital Velocity
The velocity required for a stable circular orbit is given by:
Where:
- is the gravitational constant, ,
- is the mass of the Earth, ,
- is the distance from the center of the Earth to the satellite.
2. Calculate (Distance from the Center of the Earth)
The satellite is released at a height of above the Earth's surface. Adding the Earth's radius ():
3. Calculate the Required Orbital Velocity
Substitute , , and into the orbital velocity formula:
Simplify step by step:
4. Compare Given Velocity to Required Velocity
The satellite is released at , which is slightly less than . Since the velocity is insufficient:
- The satellite will not maintain a stable orbit.
- Instead, it will spiral downward unless corrective action is taken to increase its velocity.
Conclusion
The satellite does not have a stable orbit at , as the required orbital velocity at altitude is . A small adjustment to the satellite's velocity would stabilize its orbit.
Would you like detailed calculations for energy considerations or further explanations?
Here are 5 follow-up questions for deeper understanding:
- What factors influence the stability of an orbit besides velocity?
- How does elliptical motion differ from circular orbital motion?
- What happens if the satellite's speed is greater than ?
- How does Earth's atmosphere affect low-altitude satellites?
- How would the satellite's orbit change if it were launched at a different altitude?
Tip: Always ensure to consider both altitude and velocity when evaluating orbital stability.
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Math Problem Analysis
Mathematical Concepts
Gravitational Force
Orbital Mechanics
Circular Motion
Formulas
v_orbit = sqrt(GM/r)
r = R_Earth + h
Theorems
Newton's Law of Universal Gravitation
Centripetal Force Equilibrium
Suitable Grade Level
Grades 11-12