Calculate Escape Velocity to Leave Solar System

Click For Summary
SUMMARY

The discussion focuses on calculating the escape velocity required for a spacecraft to leave the solar system, considering both Earth's and the Sun's gravitational influences. The relevant formula for escape velocity is Vesc = √(2GM/r), where G is the gravitational constant (6.672 x 10^-11), M is the mass of the Sun (2 x 10^30 kg), and r is the distance from the center of the Sun. Participants clarified that instead of adding the distances from Earth and the Sun, one should calculate the potential energies separately and then combine them using the root sum of squares method to find the total escape velocity.

PREREQUISITES
  • Understanding of gravitational force and escape velocity concepts
  • Familiarity with gravitational constant (G = 6.672 x 10^-11)
  • Knowledge of potential energy equations in gravitational fields
  • Basic algebra and square root calculations
NEXT STEPS
  • Research the derivation of escape velocity formulas in astrophysics
  • Learn about gravitational potential energy and its applications
  • Explore the concept of root sum of squares in physics calculations
  • Investigate the dynamics of spacecraft propulsion and trajectory planning
USEFUL FOR

Astronomy students, aerospace engineers, and physics enthusiasts interested in spacecraft dynamics and gravitational calculations will benefit from this discussion.

hodgepodge
Messages
47
Reaction score
0

Homework Statement


when a spacecraft escapes from the earth, it still has to escape from the sun, in order to leave the solar system. at what velocity should a spacecraft be launched if it is 6.4x10^6 meters from Earth's centre and 1.5x10^11 meteres from the sun (M=2x10^30 kg) if it is to escape the solar system.

G=6.672x10^-11

Homework Equations


i think Vesc.=(2GM)/r


The Attempt at a Solution


i was thinking to plug in the sun's mass for M, but for r, i was thinking to put in 6.4x10^6 + 1.5x10^11 for r, am i even using the right formula? I'm pretty sure that i am, i just am confused over the use of 2 distances
 
Physics news on Phys.org
You certainly wouldn't add the radii together.

But you can add the potential energies together such that the potential energy that you need to overcome with respect to Earth and the potential energy you need to overcome with respect to the Sun both can be figured and added which becomes the root sum of the squares of the individual escape velocities.

PE = GMe/Re + GMs/Rs = 1/2v2 - which is the KE needed.

(The m's of the space shot cancel out.)

In case you don't recognize that what you have is:

V2 = Ve2 +Vs2
 
thank you so much
 

Similar threads

  • · Replies 15 ·
Replies
15
Views
2K
  • · Replies 11 ·
Replies
11
Views
3K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
2
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
18
Views
3K
  • · Replies 9 ·
Replies
9
Views
2K
Replies
2
Views
4K
  • · Replies 3 ·
Replies
3
Views
2K