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Q&A

What could cause Earth to drift out of orbit over a period of months to years?

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I would like to have Earth slowly move away from the sun, taking somewhere between several months and a couple of years to reach the point where human life on the surface is no longer possible. (The story revolves around efforts to get protected in time and the resulting conflicts. So yes, we have some level of spaceflight, but not FTL -- the people who get out will be taking their chances on something like generation ships. Or, as pointed out in the comments, by building shelters on earth to give them longer to come up with a permanent solution.)

My problem is that I don't know what could cause this. I can think of ways to knock the earth out of its orbit quickly that involve killing most or all of the inhabitants, but I need something that leaves many people alive and gives them time to stew about what's next. I want them to be slowly freezing, not slowly cooking -- moving away from, not falling into, the sun. Is this possible? If so how?

It's ok to vaporize a region if that's needed. I'm not fussy about which people survive, only that many do.

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When you want the orbit of earth around the sun to get higher, earth isn't falling out of orbit, it is raising out of orbit. To get an object in orbit to a higher orbit, you need to add rotation energy to it. That energy needs to come from somewhere.

A massive object passing through the solar system and disturbing orbits (as Kent described) would be an option, but it would not be a continuous development but a rather sudden event. Also, it likely would put earth on an excentric orbit and not a round one like it currently has.

Another option would be to leave Earth alone and instead reduce the mass of the sun. When the sun would gradually lose mass, its gravity would also be reduced and all planets would go onto higher orbits. However, whatever causes the sun to lose mass would likely also affect its energy output in one way or another. So the main problem for life on Earth would likely not be Earths changing orbit but rather the sun becomming hotter or colder than usual.

This leaves the question: What could cause the sun to suddenly start losing a significant amount of mass?

One possible path how the sun could lose mass would be through a sudden increase of coronal mass ejections (preferably in polar direction so the resulting solar winds don't destroy all life on earth). Truth be told, we don't actually know much about what is going on inside a star. Most of what we believe to know is based on unconfirmed hypotheses. So you can get away with quite a lot of plausible explanations why this is suddenly happening.

Another option would be teleportation (when you want to allow it - it's a very soft sci-fi trope). Something or someone teleports large amounts of mass from inside the sun to somewhere else.

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You're going to need a lot of energy. As we'll see in a moment, too much energy to do it quickly.

Assuming we want to reduce incoming solar energy by roughly 20% (should lower mean global temperatures by roughly 15C), we need to increase the earth-sun distance by 10% (incident solar power drops with the square of distance). That means moving the earth 15 million kilometres further from the sun.

The gravitational potential U of a body of mass m at distance r from a mass M is given by $U=\frac{-GMm}{r}$. We add a factor of two to account for the kinetic energy: $U=\frac{-GMm}{2r}$

To get the change in potential, $\Delta U=\frac{-GMm}{2.2r}-\frac{-GMm}{2r}=\frac{.1GMm}{2.2r}$

That will need around $2.5\times 10^{32}$ Joules, which is more power than all the world's reserves of fossil ($4\times10^{24} $J) and nuclear ($2\times10^{23}$J) fuel, or around 50 million years worth of solar energy. It also happens to be around equal to the earth's gravitational binding energy. That's the energy you need to remove every part of the earth from every other part and bring them so far from each other that they won't reform. If you apply this energy in an -even slightly - unstructured way (say, by vaporising a continent), you're not going to be worried about the planet cooling down, you're going to be worried about the fact that the floor is made of lava.

You could have gravitational interaction with one of the gas giants do it, but it will take a lot longer than you want and you'll need to justify why it's only starting now.

Probably your best bet is a rogue planet passing through the system and raising earth's aphelion (you can't switch to a new circular orbit with just one interaction, but an elliptical orbit will do fine. Even at perihelion the earth will be colder than now due to thermal inertia).

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Roaming around interstellar space are rogue planets and rogue stars. These are planets and stars that have been thrown out of the star systems where they were formed. I have seen an estimate that says that as much as 50% of the planets formed within a star system are ejected by the time the system matures.

If one of these planets or stars swept through our solar system, a number of things could happen.

  1. The path of our star (the Sun) could be perturbed. There are many ways in which the Sun's path could be perturbed. Worst case, it could simply be sent careening away from the planets and the planets, no longer having something to orbit would begin travelling in a straight line along their current path. The lights would go out on Earth pretty quickly in this case: days/weeks. A more "mild" case of the Sun's path being perturbed could shift its trajectory in such a way that the Sun slowly begins moving through the orbital disk of the planets. In this case, depending on the speed of the Sun's progression, the planets might slam into the Sun or they might pass very near the Sun and be thrown into highly elliptical orbits.
  2. If the rogue element passes through some part of the orbital disk of the planets around the Sun, it could perturb the orbit any planets it passes near. For example, if a very large rogue planet passes behind Mars in its orbit, it could slow Mars down such that Mars' orbit could become elliptical and at its perihelion its orbit could be inside the Earth's orbit. If this were to occur, it's possible that we could use orbital projections to determine that in 3 or 30 or 300 years, the Earth and Mars would collide.
  3. If the rogue body passes near Earth, the Earth could be sped up or slowed down in its orbit, in either case causing an elliptical orbit. If the Earth is sped up, it would go through periods of substantial cooling during aphelion when the Earth was farther away from the Sun. If the Earth was slowed down, it would go through periods of substantial heating when at perihelion the Earth was much closer to the Sun.
  4. The rogue body could pass inside the Oort cloud way out at the extreme edge of our solar system. The Oort cloud is thought to contain comets and planetesimals left over from the formation of the solar system. Most of the comets, asteroids, and other leftovers from the early solar system have either collided with the Sun, the planets, or have been ejected from our solar system. Thus our current solar system is "relatively" uneventful in terms of heavy collisions. Something passing inside of the Oort cloud could dump a very large amount of that debris into the inner solar system which depending on the amount material dumped could overwhelm our ability to even detect if something were on a collision course with Earth. It would take quite a long time for this material to approach the Earth and we would see a lot of it coming for at least a decade, probably 3-5 decades. And as the material passed by any outer planets on the way in, those planets would fling the material off in various new directions. And some of it would slam into the outer planets and create impacts as we saw with Shoemaker-Levy and Jupiter. So there would be a lot of new stuff for the Earth to run into for a few 100 or 1000 years. So that would suck...

It's possible that we could detect the rogue element approaching our system and predict its effects relatively far in advance. For literary purposes, it could be decades, or we could detect it in the last few years of its approach (in the case of an Oort cloud intersection) leaving us little time to react.

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