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

In summary, the conversation discusses the attempt to find the orbital radius and speed of an asteroid in the asteroid belt using the equation T = 2pi sqrt(r/g). However, the attempt was unsuccessful due to incorrect use of the equation and confusion about which value to use for g. It is also mentioned that the equation used is related to Kepler's laws, but the person is not familiar with them.
  • #1
aligass2004
236
0

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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  • #3
I used 9.81 for the value of g.
 
  • #4
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,

[tex]T = 2\pi \sqrt{\frac r g}[/tex]

is not quite. What are Kepler's laws?
 
  • #5
I have no idea. We didn't discuss them in depth.
 
  • #6
You were trying to use one of Kepler's laws here,

[tex]T = 2\pi \sqrt{\frac r g}[/tex]

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

What is the definition of orbital radius?

Orbital radius refers to the average distance between an object in orbit and the object it is orbiting, such as a planet and its moon or a satellite and its host planet. It is typically measured in kilometers or astronomical units (AU).

How is orbital speed calculated?

Orbital speed is calculated using the formula v = sqrt(GM/r), where v is the orbital speed, G is the gravitational constant, M is the mass of the object being orbited, and r is the orbital radius. This formula is known as Kepler's Third Law of Planetary Motion.

What factors affect an object's orbital radius and speed?

The two main factors that affect an object's orbital radius and speed are the mass of the object it is orbiting and the distance between the two objects. The larger the mass of the object being orbited, the larger the orbital radius and slower the orbital speed will be. Conversely, the smaller the distance between the two objects, the smaller the orbital radius and faster the orbital speed will be.

Why do objects in orbit travel at high speeds?

Objects in orbit travel at high speeds because of the balance between the gravitational pull of the object they are orbiting and their own inertia. As the object falls towards the center of the gravitational pull, its inertia keeps it moving forward, resulting in a circular or elliptical orbit.

How does the orbital radius and speed of an object change over time?

The orbital radius and speed of an object can change over time due to various factors, such as gravitational pull from other objects, atmospheric drag, and changes in the mass or density of the object. These changes can result in the object's orbit becoming more elliptical or unstable, causing it to either move closer or farther away from the object it is orbiting.

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