Find the distance from the sun to the planet known the orbital period problem

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SUMMARY

The discussion focuses on calculating the distance from the sun to a planet based on its orbital period of 27 years. The initial approach used the circumference formula, c = 2πr, leading to an incorrect result of 4.29 km, which is a misinterpretation of the units involved. The correct methods to solve this problem involve applying Kepler's Third Law or Newton's Law of Universal Gravitation, both of which require additional information such as the mass of the sun or the distance and period of another planet for accurate calculations.

PREREQUISITES
  • Understanding of Kepler's Third Law of Planetary Motion
  • Familiarity with Newton's Law of Universal Gravitation
  • Basic knowledge of circular motion and circumference calculations
  • Ability to convert units of time into distance using gravitational constants
NEXT STEPS
  • Study Kepler's Third Law and its applications in celestial mechanics
  • Learn about Newton's Law of Universal Gravitation and its implications for orbital dynamics
  • Explore unit conversion techniques for astronomical calculations
  • Investigate the relationship between orbital period and distance for various celestial bodies
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Astronomy students, physics enthusiasts, and anyone interested in understanding planetary motion and gravitational dynamics will benefit from this discussion.

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Homework Statement


the problem asks to find the distance from the sun to a planet. the only information the question gives the the orbital period of 27 years and asks for the answer in km.


Homework Equations


c= (2)(pi)(r)


The Attempt at a Solution


assuming the planet revolves around the sun, i was assuming this is a simple problem using the circumference of a circle and solver for r to get the radius which is also the distance to the sun. here's my attempt.
c=(2)(pi)(r)
27=(2)(pi)(r)
r= 27/(2)(pi)
r= 4.29

thats my solution, but is seems really close to the sun, 4.29 km. have i done something wrong? can someone help?
 
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Take a look at units - your result is 4.29 years, not kilometers. So obviously there is something wrong.

This is either application of Kepler's third law (but then you need infomation about some other planet distance and period) or of Newton's law of universal gravitation combined with equations of motion (but then you need mass of the Sun). Not knowing in what context this question has been asked it is not possible to decide which approach will be correct (although they will both give the same result, as Kepler's laws can be derived from Newton's law).
 
yup it is calculatet in years not in km
 

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