Universal gravitation 9- determine the mass of planet Jupiter

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SUMMARY

The mass of planet Jupiter has been calculated using the orbital period and mean orbital radius of one of its moons, yielding a result of 1.96x1027 kg. The relevant equations employed include Kepler's 3rd law and Newton's Universal Law of Gravitation, specifically the formula Mp=4π2Rp3/GTp2. The gravitational constant used in the calculations is G=6.67x10-11 N*m2/kg2. The solution has been verified as correct based on the provided parameters.

PREREQUISITES
  • Understanding of Kepler's 3rd law of planetary motion
  • Familiarity with Newton's Universal Law of Gravitation
  • Basic knowledge of gravitational constants and their values
  • Ability to manipulate equations involving circular motion and gravitational forces
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  • Study the derivation of Kepler's laws and their applications in astrophysics
  • Explore advanced gravitational calculations using different celestial bodies
  • Learn about the implications of gravitational constants in various astronomical contexts
  • Investigate the methods for measuring the mass of other planets and celestial objects
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Astronomy students, astrophysicists, educators in physics, and anyone interested in celestial mechanics and gravitational studies will benefit from this discussion.

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Homework Statement



One of the moons of Jupiter, discovered by Galileo, has an orbital period of 1.44x106s and a mean orbital radius from the centre of Jupiter of about 1.90x109m. From this information, determine the mass of planet Jupiter.

Homework Equations


I have made a list of equations that are relevant for this entire module on universal gravitation. So although there are many of them does not mean that they all apply in this circumstance. The ones relevant to this question will be placed in bold.

Kepler's 3rd law: (Ta/Tb)2=(Ra/Rb)3

motion of planets must conform to circular motion equation: Fc=4∏2mR/T2

From Kepler's 3rd law: R3/T2=K or T2=R3/K

Gravitational force of attraction between the sun and its orbiting planets: F=(4∏2Ks)*m/R2=Gmsm/R2

Gravitational force of attraction between the Earth and its orbiting satelittes: F=(4∏2Ke)m/R2=Gmem/R2

Newton's Universal Law of Gravitation: F=Gm1m2/d2

value of universal gravitation constant is: G=6.67x10-11N*m2/kg2

weight of object on or near Earth: weight=Fg=mog, where g=9.8 N/kg
Fg=Gmome/Re2

g=Gme/(Re)2

determine the mass of the Earth: me=g(Re)2/G

speed of satellite as it orbits the Earth: v=√GMe/R, where R=Re+h

period of the Earth-orbiting satellite: T=2∏√R3/GMe

Field strength in units N/kg: g=F/m

Determine mass of planet when given orbital period and mean orbital radius: Mp=4∏2Rp3/GTp2



The Attempt at a Solution



Tj=1.44x106s
Rj=1.90x109m
G=6.67x10-11

with the equation highlighted above I was able to calculate the mass of Jupiter to be mj=1.96x1027kg

Does this seem like a valid answer? If anyone could check if I did this correctly or if I made a mistake and someone could point it out to me, that would be greatly appreciated! Thank you so much in advance :)
 
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dani123 said:

Homework Statement



One of the moons of Jupiter, discovered by Galileo, has an orbital period of 1.44x106s and a mean orbital radius from the centre of Jupiter of about 1.90x109m. From this information, determine the mass of planet Jupiter.

Homework Equations


I have made a list of equations that are relevant for this entire module on universal gravitation. So although there are many of them does not mean that they all apply in this circumstance. The ones relevant to this question will be placed in bold.

Kepler's 3rd law: (Ta/Tb)2=(Ra/Rb)3

motion of planets must conform to circular motion equation: Fc=4∏2mR/T2

From Kepler's 3rd law: R3/T2=K or T2=R3/K

Gravitational force of attraction between the sun and its orbiting planets: F=(4∏2Ks)*m/R2=Gmsm/R2

Gravitational force of attraction between the Earth and its orbiting satelittes: F=(4∏2Ke)m/R2=Gmem/R2

Newton's Universal Law of Gravitation: F=Gm1m2/d2

value of universal gravitation constant is: G=6.67x10-11N*m2/kg2

weight of object on or near Earth: weight=Fg=mog, where g=9.8 N/kg
Fg=Gmome/Re2

g=Gme/(Re)2

determine the mass of the Earth: me=g(Re)2/G

speed of satellite as it orbits the Earth: v=√GMe/R, where R=Re+h

period of the Earth-orbiting satellite: T=2∏√R3/GMe

Field strength in units N/kg: g=F/m

Determine mass of planet when given orbital period and mean orbital radius: Mp=4∏2Rp3/GTp2



The Attempt at a Solution



Tj=1.44x106s
Rj=1.90x109m
G=6.67x10-11

with the equation highlighted above I was able to calculate the mass of Jupiter to be mj=1.96x1027kg

Does this seem like a valid answer? If anyone could check if I did this correctly or if I made a mistake and someone could point it out to me, that would be greatly appreciated! Thank you so much in advance :)
"Google" the mass of Jupiter.

The problem is similar to an earlier post of yours regarding determining the mass of Earth: https://www.physicsforums.com/showthread.php?t=613991
 
Correct.
 
I need to use the information provided to answer the question properly...
 
Thank you grzz!
 
... and I agree with the advice given to you by Doc Al in some other post to start from a very small set of basic equations and derive the required equation on the spot.
 
Last edited:

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