# How hard is space travel, in principle?

Our Earth-based intuitions about the difficulty of travelling long distances break down badly in space. It’s tempting to think that just because Saturn, say, is nearly 4,000 times further away than the moon, it must be 4,000 times more difficult to reach. After all, on Earth it takes about 10 times as much work to go 10 kilometers as it does to go 1 kilometer. But in space, where there is no friction, this intuition is entirely wrong. In fact, in this essay I’ll show that with some important caveats the situation is far more favourable, and it doesn’t take all that much more energy to get to the outer planets than it does to get to low-Earth orbit.

The numbers are striking. We’ll see that it takes about 10 times as much energy to get to the moon as it does to get to low-Earth orbit. About 4 times more energy than that will get you to Mars, despite the fact that Mars is more than 200 times further away than the moon. Tripling *that* energy gets you all the way out to Saturn! So in some sense, the gap between getting to the moon and getting to Saturn isn’t really all that much different from the difference between getting into low-Earth orbit and getting to the moon.

The calculations required to obtain these results are all simple calculations in Newtonian gravitation, and they’re done in the next section. If you want to skip the details of the calculations, you should move to the final section, where I discuss some important caveats. In particular, we’ll see that just because getting to Saturn requires only 12 times as much energy as getting to the moon *doesn’t* mean that we only need to build rockets twelve times as big. The situation is more complex than that, and depends on the details of the propulsion technologies used.

### Calculations

To see why the numbers I quoted above are true, we need to figure out how much energy is required to get into low-Earth orbit. I will assume that the only obstacle to getting there is overcoming the Earth’s gravitation. In actual fact, of course, we need to overcome many other forces as well, most notably atmospheric friction, which adds considerably to the energy cost. I’ll ignore those extra forces – because the cost of getting to low-Earth orbit is the yardstick I’m using to compare with other possibilities this will mean that my analysis is actually quite *pessimistic*.

Suppose we have a mass that we want to send into space. Let’s use to denote the mass of the Earth. We suppose the radius of the Earth is and that we want to send our mass to a radius for some . We’ll call the *distance parameter* – it’s the distance from the center of the Earth that we want to send our mass to, measured in units of the Earth’s radius. For instance, if we want to send the mass to a height of kilometers above the Earth’s surface, then , since the Earth’s radius is about kilometers. The energy cost to do this is , where is Newton’s gravitational constant. We can rewrite this energy cost as:

We can use this formula to analyse both the energy cost to send an object to low-Earth orbit and also to the moon. (We can do this because in going to the moon the main barrier to overcome is also the Earth’s gravitation). Suppose is the distance parameter for low-Earth orbit, let’s say , as above, and is the distance parameter for the moon, . Then the ratio of the energy cost to go to the moon as opposed to the energy cost for low-Earth orbit is:

.

That is, it takes times as much energy to get to the moon as to get to low-Earth orbit.

What about if we want to go further away, outside the influence of the Earth’s gravitational field, but still within the sun’s gravitational field? For instance, what if we want to go to Mars or Saturn? For those cases we’ll do a similar calculation, but in terms of parameters relevant to the gravitational field of the sun, rather than the Earth – to avoid confusion, I’ll switch to using upper case letters to denote those parameters, where before I used lower-case letters. In particular, let’s use to denote the mass of the sun, and to denote the radius at which the Earth orbits the sun. Let’s suppose we want to send a mass to a distance from the sun, i.e., now we’re measuring distance in units of the radius of the Earth’s orbit around the sun, not the radius of the Earth itself. The energy cost to do this is [1]:

The ratio of the energy required to go to a distance from the sun versus the energy required to reach low-Earth orbit is thus:

Now the sun is about times as massive as the Earth. And the radius of the Earth’s orbit around the sun is about times the radius of the Earth. Substituting those values we see that:

For Mars, is roughly , and this tells us that the energy cost to get to Mars is roughly times the energy cost to get to low-Earth orbit (but see footnote [1], below, if you haven’t already). For Saturn, is roughly , and so the energy cost to get to Saturn is roughly times the energy cost to get to low-Earth orbit. For the stars, is infinity, or close enough to make no difference, and so the energy cost to get to the stars is only about 10 percent more than the cost to get to Saturn! Of course, with current propulsion technologies it might take rather a long time to get to the stars.

### Caveats

There are important caveats to the results above. Just because sending a payload to Mars only requires giving it about four times more energy than sending it to the moon, it doesn’t follow that if you want to send it on a rocket to Mars then you’ll only need about four times as much rocket fuel. In fact, nearly all of the energy expended by modern rockets goes into lifting the rocket fuel itself, and only a small amount into the payload. An unfortunate consequence of this is that you need a lot more than four times as much fuel – either that, or a much more efficient propulsion system than the rockets we have today. In a way, we’ve been both very lucky and very unlucky with our rockets. We’ve been lucky because our propulsion systems are *just* good enough to be able to carry tiny payloads into space, using enormous quantities of fuel. And we’ve been unlucky because to give those payloads even a tiny bit more of the energy they need to go further requires a lot more fuel. See, e.g., ref,ref and the pointers therein for more discussion of these points.

The extent to which any of this is a problem depends on your launch technology. Ideas like space guns and the space elevator don’t require any fuel to be carried along with the payload, and so escape the above problem. Of course, they’re also still pretty speculative ideas at this point! Still, I think it’s an interesting observation that the energy required to get a large mass to a distant part of the solar system is not, in principle, all that far beyond what we’ve already achieved in getting to the moon.

### Footnote

[1] Note that the object needs to first escape out of the Earth’s gravitational field, and this imposes an extra energy cost. This extra cost is roughly 10 times the cost of getting to low Earth orbit, by a calculation similar to that we did for getting to the moon. Strictly speaking, this energy cost should be added on to the numbers we’ll derive later for Mars and Saturn. But for the rough-and-ready calculation I’m doing, I won’t worry about it – we’re trying to get a sense for orders of magnitude here, not really detailed numbers!

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I am reminded of Charlie Stross’ essay on space colonization, which I would like to excerpt but can’t due to the piece’s complexity. But I will say that it expresses much greater skepticism than this post (partially because you’re mainly talking about the solar system and he’s talking about space colonization), but the larger point concerning the sheer amounts of energy involved still make it worth citing to someone interested in the subject.

You’re not even taking into account gravitational slingshots! You can certainly steal energy from other celestial objects to get you where you want to go.

And once you’re up there, it doesn’t necessary get any easier. You’ve got temperature deltas that run into the hundreds of degrees depending on whether you’re facing the sun or not. You’ve got radiation with particles flying through your spacecraft burning holes in the traces of your integrated circuits. And you’ve got static electricity potentials that run into the millions of volts, with no easy way to get rid of it all.

Any way you add it up, space flight is incredibly daunting to initiate, and incredibly difficult to maintain. Sad but true.

Very nice article, Michael! Another quantity to consider might be the gravitational field of Saturn itself. That will help you quite a bit once you’re close enough. Also, if we want to send humans holding a return ticket to Saturn, they need to carry an even bigger amount of fuel to lift off from Saturn (or they need to find a good energy source on Saturn…). ðŸ˜‰

Is this article about “space travel” – as per the headline – or about “space shipping”?

It reads as if it were concerned solely with shipping cargo in space – and is thus concerned primarily with energy requirements, a significant portion of the cost of space shipping.

To most of us, space travel implies travellers. Energy is no longer the main consideration, keeping the travellers alive is.

In principle, space shipping is relatively inexpensive and straightforward.

In principle, space travel is expensive and complex because of the need for pesky radiation shielding, pesky food, pesky waste disposal, pesky exercise facilities, etc.

I’m pretty sure the problem with space travel is not energy the way you’ve formulated it here, but travel-time. If we could travel fast enough to get anywhere interesting without the travelers all getting old in the meantime, we’d be doing it right now.

There’s a very important wrinkle in the problem of getting out of the solar system. Yes, the nominal energy required to get away from the sun is very large, much larger than the nominal energy required to get off the earth, as you’ve correctly pointed out. But you’re making the assumption that the only way to get away from the sun is similar to how you get off the earth, which is by brute force acceleration. That isn’t even vaguely true.

Once you’re off the earth and trying to get away from the sun, you can accelerate by slingshotting off of planets, a clever and largely passive technique in which you use the relative motions of the planets to speed yourself up. All that is required to do this is some careful steering, and since the only thing necessary to get it to work is the planets, and planets are huge things with massive amounts of movement relative to each other, there is an essentially limitless amount of energy which can be easily tapped into for getting out of the solar system.

There’s a common misconception that slingshotting is an obscure technique. It’s not. In fact it’s basically the only way to get away from the sun.

Doing the math on escape velocity from the sun and interstellar distances, it looks like once you got away from the sun at all you could probably get to alpha centauri in a few thousand years, which while long on the scale of a human lifetime is nothing in geologic terms.

Yes, slingshotting helps quite a lot. It doesn’t change the energy calculation, but does give you a relatively easy way of picking up some kinetic energy along the way, without having to carry additional fuel. It’s wrong, though, to say that this gives “limitless energy which can be easily tapped”. On a single pass slingshotting by a planet moving with speed V (in the sun’s frame), the maximal speed increase is, I believe, 2V. It is possible to get more than this by doing multiple slingshots past the same planet, but that’s much trickier. I haven’t done a calculation to see how much this helps cut down the fuel problem, although I imagine it’s pretty significant.

I would suggest it’s even more favorable than this, because the real figure of merit is change in velocity, which scales with the square root of energy.

Going to the Moon is easy – just apply the right force to your space ship and soon you are there. Question is how to stop … ? I offer anybody â‚¬1M to solve the problem.