Planetary Motion HW: Orbit Radius & Speed Around Jupiter

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Homework Help Overview

The discussion revolves around a homework problem related to planetary motion, specifically focusing on determining the orbital radius and speed of a satellite intended to orbit Jupiter. The original poster outlines the parameters of the problem, including Jupiter's rotational period and relevant constants.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to apply gravitational equations to find the required orbital radius and speed. They express uncertainty about their approach and seek validation of their calculations. Other participants engage by discussing the implications of varying orbital speeds on the shape of the orbit, questioning how changes in speed would affect the orbit's characteristics.

Discussion Status

Some participants affirm the correctness of the original poster's method, while others explore the consequences of incorrect orbital speeds. The conversation indicates a productive exchange of ideas regarding the relationship between speed and orbital characteristics, though no consensus is reached on the specifics of elliptical orbits.

Contextual Notes

The discussion includes assumptions about circular motion and the effects of speed variations on orbital radius, with participants acknowledging uncertainties regarding real-life orbital dynamics.

k-rod AP 2010
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Homework Statement


An explorer plans a mission to place a satellite into a circular orbit around Jupiter, the radius of the planned orbit would be R.

a)The explorer wants the satellite to be sychronized w/ Jupiter's rotation. Determine the required orbital radius in meters.
b) What must the orbital speed of this satellite be in order to maintain this orbital period?



Homework Equations


RJ=7.14x107m
MJ=1.9x1027kg
Jupter's rotational period=3.55x104s
G\ =\ 6.673(10)\ \times\ 10^{-11}\ m^{3} kg^{-1} s^{-2}

The Attempt at a Solution


a) T=√(4π2R3/GMJ)
3.55x104s=√(4π2R3/GMJ)
R=1.59374x108 m

b)v=√(GMJ/R)
v=√(GMJ/1.59374x108 m)
v=28207.7 m/s

arm I following the correct procedure on these problems? i am trying to get a handle on this planetary motion stuff and i am not sure if i have yet.
 
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Your method is correct.
 
ok, that's what i thought thanks for the help. and another question pertaining to this hw,...

if the orbital speed were mistakingly made slower than needed the orbit would be smaller than desired, and if it were faster than needed the orbit would be larger and more elliptical than wanted right?
 
k-rod AP 2010 said:
ok, that's what i thought thanks for the help. and another question pertaining to this hw,...

if the orbital speed were mistakingly made slower than needed the orbit would be smaller than desired, and if it were faster than needed the orbit would be larger and more elliptical than wanted right?

Not too sure how elliptical it would be in real life, but with the assumption of circular motion

Fc=mv2/r, if 'v' were smaller, the 'r' would need to be smaller to maintain the same Fc, and if 'v' were larger, 'r' would be larger as well. So yes you are correct, but once again, I am not too sure how elliptical the motions would become.
 
ok that's what i was thinking, thanks again for all your help with this problem
 

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