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

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Homework Help Overview

The problem involves calculating the orbital radius and speed of an asteroid in the asteroid belt, given its orbital period of 4.2 Earth years. The context is rooted in celestial mechanics and gravitational theory.

Discussion Character

  • Conceptual clarification, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the manipulation of an equation related to orbital mechanics, questioning the use of the gravitational constant and the validity of the equation employed. There are inquiries about the source of the gravitational field and the application of Kepler's laws.

Discussion Status

The discussion is ongoing, with participants seeking clarification on the correct values and equations to use. Some guidance has been offered regarding the need to reference Kepler's laws and the universal gravitational constant, but no consensus has been reached on the correct approach.

Contextual Notes

There is a noted lack of familiarity with Kepler's laws among participants, which may affect their understanding of the problem. Additionally, the original poster's use of Earth's gravitational acceleration has been questioned, indicating a potential misunderstanding of the problem's context.

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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