Escape velocity of solar system

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SUMMARY

The escape velocity from Saturn's orbit in the solar system is calculated using the formula v = sqrt(2GM/r). The mass (M) should include the mass of the Sun and the planets, while the radius (r) is the distance from the center of the Sun to Saturn. The calculated escape velocity is 13.72 km/s, which is significantly higher than Saturn's orbital speed of 9.7 km/s. Including the masses of other celestial bodies, such as moons and asteroids, does not significantly affect the result.

PREREQUISITES
  • Understanding of gravitational physics
  • Familiarity with the formula for escape velocity
  • Basic knowledge of the solar system's structure
  • Ability to perform calculations involving mass and distance
NEXT STEPS
  • Research the mass distribution of the solar system, focusing on the Sun's mass percentage
  • Learn about gravitational influences of moons and asteroids on escape velocity
  • Explore variations in escape velocity calculations for different celestial bodies
  • Study the implications of escape velocity in space missions and planetary exploration
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Astronomy students, astrophysicists, and anyone interested in gravitational physics and space exploration calculations.

oldspice1212
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Hey guys so this question I'm kind of stuck on,

Our solar system, starting from Saturn's orbit.


So I know the formula is v = sqrt(2GM/r)

But not sure what to put for the mass and radius, am i including saturn and planets like uranus and neptune only or all the satellites and stuff to like moons, asteroids, etc. Or am I simply over thinking this lol?

Thank you.
 
Last edited:
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Look up the percentage of the solar system's mass that is contained in the Sun. Will including planetary masses affect your result significantly?
 
Ok so I calculated it to be 13.72 km/s since saturns orbital speed is 9.7 km/s.
 
Last edited:
That'll do.
 
Thanks :)
 

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