Trip to the Moon: How to Reach with Speed

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Homework Help Overview

The discussion revolves around calculating the necessary speed to reach the moon from Earth without traditional rocket propulsion. Participants are examining gravitational forces, energy conservation, and the relevant equations to determine the distances and speeds involved in the journey.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation, Assumption checking

Approaches and Questions Raised

  • Participants are attempting to apply the conservation of energy principle and gravitational potential energy formulas to solve for the distance and speed of a spacecraft traveling to the moon. There are questions about the correct use of variables and equations, particularly regarding the gravitational potential energy and kinetic energy at different points in the journey.

Discussion Status

Some participants have shared their attempts at calculations and are seeking clarification on specific values and equations. There is an ongoing exploration of the relationships between potential and kinetic energy, as well as the implications of different initial speeds. No consensus has been reached, but productive questions are being raised.

Contextual Notes

Participants are navigating constraints such as the need for accurate values in their calculations and the definitions of variables like mass in the context of gravitational equations. There is also confusion regarding the application of certain formulas, particularly in relation to the distances involved in the Earth-moon system.

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Homework Statement


You plan to take a trip to the moon. Since you do not have a traditional spaceship with rockets, you will need to leave the Earth with enough speed to make it to the moon. Some information that will help during this problem:

mearth = 5.9742 x 1024 kg
rearth = 6.3781 x 106 m
mmoon = 7.36 x 1022 kg
rmoon = 1.7374 x 106 m
dearth to moon = 3.844 x 108 m (center to center)
G = 6.67428 x 10-11 N-m2/kg2


Homework Equations


On your first attempt you leave the surface of the Earth at v = 5534 m/s. How far from the center of the Earth will you get?


2.
Since that is not far enough, you consult a friend who calculates (correctly) the minimum speed needed as vmin = 11068 m/s. If you leave the surface of the Earth at this speed, how fast will you be moving at the surface of the moon? Hint carefully write out an expression for the potential and kinetic energy of the ship on the surface of earth, and on the surface of moon. Be sure to include the gravitational potential energy of the Earth even when the ship is at the surface of the moon!



The Attempt at a Solution


In our lecture concerning this topic we discussed distance= v(not) /2(μ)g, but there is no μ here clearly, so I tried not using the μ and that did not work and I don't know if I should use the formula for PE gravity close to Earth or not close to earth, -G(m1m2/r)+U(not) or -G(m1m2/r^2)r. I don't understand how to get my distance without using μ.
 
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Use the -GMm/r formula; it's universal.

Use conservation of energy to determine the interchange of PE and KE. Remember that both the Earth and Moon will be trading energy with the ship :wink:

What speed will the first "unsuccessful" shot have when it reaches its maximum distance from the Earth? What then will be its KE?
 
I, too have the same question. However, my question is with the second part of the problem:

Since that is not far enough, you consult a friend who calculates (correctly) the minimum speed needed as vmin = 11068 m/s. If you leave the surface of the Earth at this speed, how fast will you be moving at the surface of the moon? Hint carefully write out an expression for the potential and kinetic energy of the ship on the surface of earth, and on the surface of moon. Be sure to include the gravitational potential energy of the Earth even when the ship is at the surface of the moon!

Here is my attempt at a solution:

I know that when the traveler is at the surface of the Earth, there are two potentials at work: the potential of the Earth and the potential of the moon. Let d be the distance between the centers of the moon and the earth, and let v_0 be the initial velocity. Then the relation of kinetic energy equals the following equation:

\frac{1}{2} mv_0^2 - \frac{GM_em}{r_e} - \frac{GM_mm}{d-r_e} = \frac{1}{2} mv^2 - \frac{GM_em}{d-r_m} - \frac{GM_mm}{r_m}.

However, solving for v does not give the right solution. What gives?
 
TMO said:
\frac{1}{2} mv_0^2 - \frac{GM_em}{r_e} - \frac{GM_mm}{d-r_e} = \frac{1}{2} mv^2 - \frac{GM_em}{d-r_m} - \frac{GM_mm}{r_m}.

However, solving for v does not give the right solution. What gives?

What value did you calculate?
 
gneill said:
What value did you calculate?

I got 2263.52 m/s. Apparently, this is the correct answer (I didn't square the right value for the initial velocity).
 
what did you use for me "m" in 1/2mv^2
 
also in the first part of the question when solving for "D" I am still confused, in the equation you told me to use "-GMm/r, is Mm the mass of the moon or did you mean mass of moon times mass of earth?
 

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