Comet with eccentricity of 0.7 and 200 year period

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Homework Help Overview

The discussion revolves around a comet with an eccentricity of 0.7 and a 200-year orbital period around the star Sol. Participants are exploring how to calculate the average distance of the comet from Sol, as well as its perihelion and aphelion distances, and its velocity at perihelion.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation

Approaches and Questions Raised

  • Some participants suggest using Kepler's 3rd law to find the average distance and semi-major axis based on the orbital period. Others question the definitions of perihelion and aphelion and how they relate to the average distance.

Discussion Status

There is an ongoing exploration of the relationships between the comet's orbital characteristics and the relevant equations. Some participants have provided guidance on using Kepler's laws, while others are seeking clarification on specific terms and calculations.

Contextual Notes

Participants note that the textbook being referenced does not provide information on perihelion and aphelion, leading to some uncertainty in the discussion.

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Homework Statement



A comet of the star Sol has an eccentricity of .7. It takes 200 yrs to complete on orbit

1)find the average distance of the comet from Sol.

2) Find the perihelion and aphelion distances from Sol

3)find the velocity of the comet at perihelion

Homework Equations





The Attempt at a Solution



1) i know ecentricity = (F(2) - F(1))/c where F is the foci and c is the major axis how does this help me
 
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You can use Kepler's 3rd law to find the average distance from the sun, knowing the period. By knowing the period you should also be able to find the semi-major axis of the orbit, and consequenctly the perihelion and Aphelion.

And finally the velocity at perihelion is related to the eccentricity of the orbit, and the distance of closest approach to the sun.
 


but I am looking for the average distance of the comet from Sol, not the earth

...or am i reading it wrong
 


What does Kepler's 3rd law say?
 


ohhhh i guess i should read more carefully

so r(commet)^3 / r(earth)^3 = T(commet)^2 / T(earth)^2

r(commet) = (200^2 * (2.28x10^11)^3)^1/3 = 7.797 x 10^12
 


how do i find the perihelion and aphelion, our book doesn't even mention it but i believe they are the closest and farthers points of the orbit
 


You should double check your text (what book are you using, by the way?). But I think you can use the average distance as your semi major axis. Then you might find this helpful http://en.wikipedia.org/wiki/Apsis

Those equations are probably quoted to you somewhere.
 


the book is 4th edition Physics for scientists & engineers by Giancoli
 

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