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So you see, we started from the typical velocity of satellites on this circular orbit around Earth,

2
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and then we increase the velocity at this point and give rise to such an elliptical trajectory.

3
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So of course, when we increase not a lot of T here, this radius will get larger and larger.

4
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And now we may encounter the moon or if we go even higher, we will leave the gravitational field of

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the Earth.

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I mean, we will never really leave it, but it has one of our dependence, so it becomes basically

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not negligible.

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And this is what we want to analyze next.

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The direct earth escape where the spaceship leaves basically hit the Earth.

10
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So I will just copy what we have here and paste it here.

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And now we have a look once again at the velocity and I try to bits.

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It is already sufficient if we just briefly increase the velocity here and we can go, for example,

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to 1.5 feet orbit.

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And when they're on it, you see, this is here to position off the Earth.

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This is here the moon trajectory and this trajectory of our spaceship.

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So we start from Earth and then be straightforwardly leave it.

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And what happens then is we will enter the fields of the Sun.

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Of course, we are always in the field of the Sun.

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But now the effect of the gravity of the sun is larger than the effect of the gravity of the Earth.

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So then the motion will be more effected by the Sun than the Earth.

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So for this reason, let's re plot this whole thing here.

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Let's go ahead and copy this and make a new figure.

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And this time we will not subtract here.

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The Earth coordinates, so we will not put it in the reference systems.

25
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The system of the Earth bump in the reference system of the Sun.

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So we would have to subtract you the coordinates of the Sun.

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But since they are basically zero, we don't have to do it.

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I mean, we have seen they're not exactly zero, but we can neglect really this effect.

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So for the green, we have the moon and then the spaceship, and now I want to remind the Sun and the

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Earth from before.

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So this would be zero and one and three and four, and the colors were blue and red.

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And when I plot this, we see this is now what happens here, the Sun.

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And I think actually it was a red and blue.

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Yes.

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So this is here to sun.

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And then we have here the moon and the Earth, and we see the spaceship is moving on a different trajectory.

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So of course, now we should increase the simulation time and I will simulate here not one month, but

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I will now simulate here for years.

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So our first plot, which was with respect to the Earth, changed to this one.

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We have here the Earth and also the Moon, which is not really visible anymore, but you have to zoom

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in here to see it.

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And in this coordinate frame, the satellite will spiral away from the Earth, which is clear it's not

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anymore in a circle which is spiral away.

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And in the coordinate system of the Sun.

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This is what happens.

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We see blue and green are here.

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Actually, we can only see green, but we know that the moon and the Earth in the very similar trajectory.

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So this here to circle with the larger radius and this is here the motion of our spaceship.

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And it's pretty interesting that at some point the spaceship will come back to the Earth and to the

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Moon.

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They don't have to be here at the same time, necessarily, but at least the possibility exists that

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they re-enter the orbit.

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And it turns out that this happens already after two of these oscillations here or two of these rotations

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around the Sun rather to see.

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So we can find this out by increasing the simulation time even more.

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And I will simulated here for 16 years, which is four times the time that we had before.

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And of course, now it takes a bit longer.

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And you see, this is here to plot in the coordinate system of the Earth.

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It's no bit confusing, to be honest, because here is the Earth and the moon in the center, and then

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the satellite starts basically leaving this trajectory and then coming back, it seems.

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And it's, of course, much better to see on this trajectory.

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We go in this circle and then we on the larger circle and then eventually we come back to this point.

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So here on this whole path, there always is the possibility that the spaceship re-enters to orbit around

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the Earth and to figure out if this is happening or not.

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We will now use a different plot and I will basically take this plot here and I will just fix here to

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plot range to this area so that we can really see what's going on in the vicinity of the Earth.

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So I would right, Pulte thoughts.

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Excellent, excellent.

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And I will use three times the radius of Earth and Moon.

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So in positive and a negative direction.

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And of course, I will use the same for the wide range.

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So plotted out why Lim?

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And now we can see what's going on here.

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So at first we start from the Earth or very close to the Earth, and then we have so high velocity that

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we basically leave the Earth and the Moon and we move on this trajectory and then we move around the

76
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sun once and twice, maybe and even more times, we don't know.

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And eventually we come back very, very close to the Earth and we will almost hit it.

78
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And then we will leave it again.

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So at this point, it would in principle be possible to break or basically to use a booster and boost

80
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along the opposite direction and decrease the velocity so that we re-enter here.

81
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The orbits of coasters would cost an enormous amount of energy, but in principle it's possible to do.

82
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So the last thing that I want to analyze is, of course, to time dependence here.

83
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So I will plot the distance of our spaceship with respect to the Earth.

84
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And I think we have done this already here, so I can just copy this.

85
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Go to the bottom and look at it.

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And we see we have simulated for 16 years.

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Of course, I have tested this before, so I know that it is a good time range to simulate and we see

88
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that the distance increases with some additional fluctuations.

89
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And then we are here for the furthest apart and we get closer and we get once again further apart.

90
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And then we are here almost at zero.

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This is where we almost hit the Earth.

92
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So this is this point that we see here.

93
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So I think this is really an interesting discussion because just by increasing the starting velocity,

94
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we get such an interesting physics and such a very different behavior.

95
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So instead of having this oval trajectory, which is always the same around the Earth, we instantly

96
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leave the Earth and then we basically circle around the sun on a different trajectory.

97
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But then eventually, after two rotations after 16 years, we reenter here and we almost hit the Earth.

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So that's pretty, pretty nice.

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Physics are pretty interesting.

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OK, so the next thing I want to analyze is the surface cable, like we just did, we escaped the orbit,

101
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but I want to show you that it's even possible with the lower velocity by using a trick, by using the

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so-called moon and copter.

