Calculating orbital radius and speed of an asteroid in the asteroid belt

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SUMMARY

The discussion focuses on calculating the orbital radius and speed of an asteroid in the asteroid belt, specifically one with a period of 4.2 Earth years. The correct approach involves using Kepler's laws of planetary motion, particularly the equation T = 2π√(r/G), where G is the universal gravitational constant. The initial attempt to use Earth's gravitational acceleration (9.81 m/s²) was incorrect, as the problem requires the application of the universal gravitational constant. Participants emphasized the importance of understanding Kepler's laws to solve such problems accurately.

PREREQUISITES
  • Understanding of Kepler's laws of planetary motion
  • Familiarity with the universal gravitational constant (G)
  • Basic algebraic manipulation skills
  • Knowledge of orbital mechanics
NEXT STEPS
  • Study Kepler's laws in detail, focusing on their applications in orbital mechanics
  • Learn how to calculate orbital radius using the formula T = 2π√(r/G)
  • Explore the concept of gravitational forces and their role in celestial mechanics
  • Review examples of orbital calculations for various celestial bodies
USEFUL FOR

Astronomy students, physics enthusiasts, and anyone interested in understanding the mechanics of celestial bodies and their orbits.

aligass2004
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Homework Statement



The asteroid belt circles the sun between the orbits of Mars and Jupiter. One asteroid has a period of 4.2 Earth years. What are the asteroid's orbital radius and speed?

Homework Equations



T = 2pi sqrt(r/g)

The Attempt at a Solution



I tried manipulating the above equation to solve for r. I got 4.383, but it was wrong.
 
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I used 9.81 for the value of g.
 
Why did you do that? You need to use the universal gravitational constant G, not the Earth's standard gravitational acceleration, g. Moreover, this equation,

T = 2\pi \sqrt{\frac r g}

is not quite. What are Kepler's laws?
 
I have no idea. We didn't discuss them in depth.
 
You were trying to use one of Kepler's laws here,

T = 2\pi \sqrt{\frac r g}

but you did it wrong. Where did you get that equation from? Look over your text and your notes.
 

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