Pioneer 10 Spacecraft travelling in space

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SUMMARY

The Pioneer 10 spacecraft needed to achieve a specific escape velocity to leave the solar system as it passed Jupiter's orbit. The escape velocity (v) can be calculated using the formula v = √(2GM/R), where G is the gravitational constant, M is the mass of the Sun (1.99 x 10^30 kg), and R is the radius of Jupiter's orbit (7.78 x 10^11 m). The mass of Jupiter is irrelevant in this calculation since the spacecraft is not launching from its surface but rather passing by its orbit. This approach focuses solely on the gravitational influence of the Sun.

PREREQUISITES
  • Understanding of gravitational potential energy
  • Familiarity with total orbital energy concepts
  • Knowledge of kinetic energy principles
  • Proficiency in calculating escape velocity
NEXT STEPS
  • Research the gravitational constant (G) and its value (6.674 x 10^-11 m^3 kg^-1 s^-2)
  • Study the derivation and applications of escape velocity in astrophysics
  • Explore the concept of orbital mechanics and its relevance to spacecraft trajectories
  • Learn about the historical significance and mission details of the Pioneer 10 spacecraft
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Astronomy students, physics enthusiasts, aerospace engineers, and anyone interested in the dynamics of spacecraft navigation and escape trajectories from celestial bodies.

aeromat
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Homework Statement


To escape from the solar system, how fast did the Pioneer 10 have to be traveling as it passed the orbit of Jupiter? Assume the mass of the solar system is essentially concentration in the Sun. The mass of the Sun is 1.99 x 10^30 kg and the radius of Jupiter's orbit is 7.78 x 10^11 m.


Homework Equations


Gravitational Potential Energy
Total Orbital Energy
Kinetic Energy
Escape Velocity
Escape Energy

The Attempt at a Solution


I am confused as to what quantities are relevant in this situation. I know that Jupiter must be used to carry out with escape velocity, but I don't have the mass of it.
 
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Well, I haven't gotten to this part yet, we just started the chapter concerning this type of problem.
However, looking in the book I found that the escape speed (v) = √(2GM/R)
I don't think you need the mass of Jupiter since you aren't launching from its surface, you're just flying past it's orbit. The key here is that you're finding the escape velocity of the solar system. Also, the problem states that you can assume the solar system's mass is concentrated in the sun, so you can use the M = mass of the sun, and R can be the radius of Jupiter's orbit, (since that's the distance Pioneer 10 is from the sun at this point)
 
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You have the data to substitute and solve in the escape velocity formula (at least for one of the two forms of that equations I know).

If that is not clear to you, I suspect you have the other form or are misinterpreting the variables. Can you post the equation and what the variables mean?
 

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