<p>No, we cannot.</p>
<p>It's relatively simple math to show that we are a very long shot from changing Earth's orbit by anything significant at all: consider the kinetic energy of Earth in its current orbit, and do the same math for that in the desired orbit:</p>
<p><span class="math-container">$ E_{kin} = \frac{m_E}{2}v^2 \approx \frac{m_E}{2}\frac{GM_S}{a}$</span></p>
<p>where <span class="math-container">$m_E = 6\cdot 10^{24}$</span>kg is Earth's mass, <span class="math-container">$M_S=2\cdot 10^{30}$</span>kg is the solar mass and <span class="math-container">$a=150\cdot 10^9$</span>m is the distance from Earth to sun. I used the approximation in calculating orbital velocity <span class="math-container">$v = \sqrt{\frac{GM_S}{a}}$</span> that the Earth mass, is much smaller than the Sun's mass. So current orbital velocity is (using numbers as above) <span class="math-container">$29822$</span>m/s.</p>
<p>Now, changing oribital distance outward by 1%, thus by <span class="math-container">$1.5\cdot 10^9$</span>m, to <span class="math-container">$151.5\cdot 10^9$</span>m yields a speed of <span class="math-container">$29674$</span>m/s - and in energy that subsequently gives a difference of <span class="math-container">$2.64\cdot 10^{31}$</span>J to move Earth's orbit about 1% to further from the Sun.</p>
<p>Annual world primary energy production currently <a href="https://en.wikipedia.org/wiki/World_energy_consumption" rel="noreferrer">is around</a> <span class="math-container">$10^{20}$</span>J - so <strong>we &quot;just&quot; need to produce 100.000.000.000 times the yearly energy production of the entire world to change Earth's orbit about 1%</strong>. And that implies that we have a technique to transfer energy 100% into Earth orbital velocity - something which cannot exist either due to simple thermodynamic argument.</p>
<p>Edit to add: Another way to argue is the rocket way: typical speed of conventional rocket exhausts are a few km/s, which is less than needed to leave Earth's orbit - that's why you need multi-stage rockets to get anything into orbit. But if you want to move the whole Earth with a rocket motor, you need a propellant which is fast enough that it directly leaves Earth's gravitational field - or you will not be able to create any effective change of momentum and only move around mass in the Earth system itself. So you need to make some substantial technological advances here, too - or some entirely different technique.</p>

CC BY-SA 4.0
2020-08-05T19:32:39.853Z
Effective exhaust velocity isn't the reason for multiple stages to orbit. It's the mass ratio element in the [Tsilokovsky rocket equation](https://en.wikipedia.org/wiki/Tsiolkovsky_rocket_equation) that's the main culprit. It's _mathematically_ possible to single-stage-to-orbit on a black powder rocket, but good luck building a light enough rocket that can contain all the black powder you'd need for it.
notovny
CC BY-SA 4.0
2020-08-05T22:54:41.857Z
@notovny, effective exhaust velocity *is* the reason why we can't use chemical rockets to move the Earth around: in order for a rocket engine to have a net effect on the Earth's momentum, the exhaust needs to be moving faster than escape velocity.  If it doesn't, the exhaust will (eventually) come back and return its momentum to Earth.
Mark
CC BY-SA 4.0
2020-08-06T01:39:34.573Z
This argument is correct but it entirely disregards the possibility of using energy sources outside of Earth, like for example the orbital energy of Jupiter (https://link.springer.com/article/10.1023%2FA%3A1002790227314). Another important point against your conclusion is the amount of time. If we operate in terms of a hundreths of thousands of years we in fact move Earth with smaller power outputs.
Swike
CC BY-SA 4.0
2020-08-06T05:14:23.360Z
If you take as long as civilisation is already old (10.000 years), you only need continuously for the next 10.000 years 10.000.000 times our current total energy production. Sources outside earth exist, and can be tapped, but don't change the energy equation.   Changing the trajectory of a body of 1/100000 of earth mass drastically and controlled does not solve but mostly moves the energy problem from earth to the asteroid or kuiper belt. Additionally it creates the problem that you willfully create a potential planet buster, an object rated most dangerous on each planetary protection scale.
planetmaker
CC BY-SA 4.0
2020-08-06T05:51:34.197Z
Interesting study, though. "optimistic minimum energy expenditure is about 10^36 erg" (1.000.000 yearly energy productions) and "this scheme would consume a number of large Kuiper Belt objects". These are 100km-diameter bodies sent to pass Earth repeatedly at 1/40 of moon distance. This makes it more concept than 'modern technology". One should also mind the last sentence of the paper: "The collision of a 100-km diameter object with the Earth at cosmic velocity would sterilize the biosphere most effectively, at least to the level ofbacteria. This danger cannot be overemphasized"
planetmaker
CC BY-SA 4.0
2020-08-05T09:51:34.690Z
2020-08-05T16:39:11.713Z
2020-08-05T16:39:11.713Z
planetmaker
<p>I'll go out on a speculative limb and say <strong>yes</strong>, maybe, depending on the definition of &quot;significant&quot;.</p>
<p><a href="https://astronomy.stackexchange.com/a/38300/34727">Planetmaker's answer</a> notes the infeasibility of raising Earth's orbit if <em>nothing else changes</em>.  But what if we also lower some other body's orbit at the same time?</p>
<p>First, let the orbital energy of an object with mass <span class="math-container">$m$</span> orbiting the Sun with mass <span class="math-container">$M_S$</span> at an average distance of <span class="math-container">$a$</span> be its kinetic plus potential energy with respect to the Sun:</p>
<p><span class="math-container">$E_k + U = \frac{1}{2}m v^2 - \frac{G M_S m}{a} = \frac{1}{2} m (\sqrt{\frac{GM_S}{a}})^2 = \frac{G M_S m}{2a} - \frac{G M_S m}{a} = -\frac{G M_S m}{2a} $</span></p>
<p>Our goal is to raise the Earth's average orbital radius by 1%.  Using the above equation and the specific values listed at the end, we need <span class="math-container">$2.62 \times 10^{31} \ \mathrm{J}$</span> to do that.  (This is all consistent with planetmaker's calculation, I just want to show my own work.)</p>
<p>Where can we get this energy? Let's try stealing <a href="https://en.wikipedia.org/wiki/Ceres_(dwarf_planet)" rel="nofollow noreferrer">Ceres</a>.  If we drop its orbital radius down to match Earth's, we gain <span class="math-container">$2.65 \times 10^{29} \ \mathrm{J}$</span>.  That's only 1% of the required energy.  But if we instead are content to change Earth's orbit by 0.01% (is that &quot;significant&quot;?) then we have enough energy to do it in Ceres.  If not, we need to get more bodies involved.  (Since Ceres alone is already about 30% of the asteroid belt mass, they will need to come from elsewhere.)</p>
<p>How do we transfer energy from Ceres to Earth?  We arrange for a series (no pun intended) of <a href="https://en.wikipedia.org/wiki/Gravity_assist" rel="nofollow noreferrer">Gravitational slingshots</a> between the two bodies, each time letting Ceres pass just ahead of the Earth, thereby transferring energy to the latter.  (As an outline of the encounter plan, my basic idea is we start by lowering its periapsis to match Earth, then all encounters happen at Ceres periapsis, thus preserving the possibility of future encounters.)</p>
<p>How do we change the orbit of Ceres to cause these slingshots?  We apply the same technique, recursively if needed.  Find something else nearby, presumably also in the asteroid belt, whose orbit we can perturb to cause encounters with Ceres, gradually steering it toward the eventual encounter with Earth.  The bottom of the recursion is some object small enough to be pushed (perhaps slowly) into an encounter with the next object using existing spacecraft and propulsion technology.</p>
<p>This would of course take a long time, at least tens to hundreds of thousands of years, but still well short of the hundred billion years planetmaker cited to move Earth using terrestrial energy sources.</p>
<p>At the core of this idea is the observation that N-body gravitational systems are chaotic, meaning that small changes in initial conditions can cause very large changes in later system state.  To move the world, <a href="https://en.wikiquote.org/wiki/Archimedes" rel="nofollow noreferrer">Archimedes</a> asked for a lever and a fulcrum.  But with modest technology, accurate foresight, and ample patience, in principle we should be able to manipulate the solar system almost at will without either.</p>
<p>The Wikipedia <a href="https://en.wikipedia.org/wiki/Asteroid_capture" rel="nofollow noreferrer">Asteroid capture</a> article discusses some related concepts.</p>
<p>Specific numbers used in calculations (generally taken from Wikipedia):</p>
<ul>
<li><span class="math-container">$G = 6.67 \times 10^{-11} \frac{\mathrm{m}^3}{\mathrm{kg} \ \mathrm{s}^2}$</span></li>
<li><span class="math-container">$M_S = 1.99 \times 10^{30} \ \mathrm{kg}$</span></li>
<li><span class="math-container">$m_\mathrm{Earth} = 5.97 \times 10^{24} \ \mathrm{kg}$</span></li>
<li><span class="math-container">$a_\mathrm{Earth} = 150 \times 10^9 \ \mathrm{m}$</span></li>
<li><span class="math-container">$m_\mathrm{Ceres} = 2.38 \times 10^{20} \ \mathrm{kg}$</span></li>
<li><span class="math-container">$a_\mathrm{Ceres} = 414 \times 10^9 \ \mathrm{m}$</span></li>
</ul>

CC BY-SA 4.0
2020-08-05T23:44:28.910Z
Very interesting approach! Thanks
luchonacho
CC BY-SA 4.0
2020-08-06T01:41:57.967Z
The actual core idea has been studied by researchers. With a carefully planed strategy we could use a bunch of asteroids to transfer a bit of Jupiter's orbital energy to Earth's. With current technology we would be able to move our planet at a rate that allow us to mantain a priviledged position in the habitable zone of our star as it gets hotter (and thus the habitable zone gets farther away). https://arxiv.org/pdf/astro-ph/0102126.pdf
Swike
CC BY-SA 4.0
2020-08-05T23:16:45.020Z
2020-08-05T23:49:53.623Z
2020-08-05T23:49:53.623Z
Scott McPeak
<p>It is well known that, according to Newton's 3rd law, spacecrafts entering or leaving Earth provoke tiny (insignificant) changes to Earth's orbit (see related question <a href="https://astronomy.stackexchange.com/questions/834/changes-to-earths-orbit">here</a>).</p>
<p>My question is about <strong>significant changes</strong>. For instance, say we would like to shift the Earth's orbit closer to that of Mars (forget about the <a href="https://astronomy.stackexchange.com/questions/23348/how-much-could-earths-orbit-shift-without-causing-an-ecological-catastrophe?noredirect=1&amp;lq=1">ecological consequences</a> of this). Do we currently have the technology capable of doing this? For instance, something like a huge nuclear explosion? <a href="https://astronomy.stackexchange.com/questions/22935/the-consequences-and-the-mechanisms-of-a-shift-of-the-earth-away-from-the-sun?rq=1">This question</a> only deals with &quot;natural&quot;, non-human ways to change a planet's orbit. I am interested about technology-based changes.</p>

CC BY-SA 4.0
2020-08-05T09:07:04.150Z
In short: no, we cannot. You can do the simple math by considering the kinetic energy of earth in its current orbit and the orbit you want to move it to and compare that to the annual world energy generation
planetmaker
CC BY-SA 4.0
2020-08-05T09:20:53.730Z
@planetmaker why not make than an answer?
Steve Linton
CC BY-SA 4.0
2020-08-05T17:24:32.793Z
See "The Wandering Earth," by Cixin Liu.   Keep in mind that's fiction, so it has semi-magical engineering to produce the energy required.
Carl Witthoft
CC BY-SA 4.0
2020-08-05T22:08:05.943Z
@SteveLinton Answers have quality control. Comments, unless outright deleted get to appear at the top of the page.
Comic Sans Seraphim
CC BY-SA 4.0
2020-08-05T22:52:24.177Z
@antispinwards, pointing out the relative scales involved certainly does fall within the scope of Astronomy.
Mark
CC BY-SA 4.0
2020-08-06T05:55:32.660Z
@CarlWitthoft And semi-magical gravity that can suddenly increase or decrease just as your trying to slingshot around Jupiter (at least in the film version on Netflix).  That was about the the point I just threw the whole idea of finishing it out the window.  I probably should have done so earlier with how they described what was happening with the sun, but I'm more willing to forgive a nonsensical background element than I am a nonsensical plot device mid-story.
zibadawa timmy
<orbit><earth><earths-orbit>
Can we change Earth's orbit with modern technology?
luchonacho
# Can we change Earth's orbit with modern technology?

(Asked by: username_0 on 2020-08-05)

It is well known that, according to Newton's 3rd law, spacecrafts entering or leaving Earth provoke tiny (insignificant) changes to Earth's orbit (see related question [here](https://astronomy.stackexchange.com/questions/834/changes-to-earths-orbit)).

My question is about **significant changes**. For instance, say we would like to shift the Earth's orbit closer to that of Mars (forget about the [ecological consequences](https://astronomy.stackexchange.com/questions/23348/how-much-could-earths-orbit-shift-without-causing-an-ecological-catastrophe?noredirect=1&lq=1) of this). Do we currently have the technology capable of doing this? For instance, something like a huge nuclear explosion? [This question](https://astronomy.stackexchange.com/questions/22935/the-consequences-and-the-mechanisms-of-a-shift-of-the-earth-away-from-the-sun?rq=1) only deals with "natural", non-human ways to change a planet's orbit. I am interested about technology-based changes.

**Tags:** orbit, earth, earths-orbit

> **Comments:**
> **username_1**: In short: no, we cannot. You can do the simple math by considering the kinetic energy of earth in its current orbit and the orbit you want to move it to and compare that to the annual world energy generation  
> **username_2**: @username_1 why not make than an answer?  
> **username_3**: See "The Wandering Earth," by Cixin Liu.   Keep in mind that's fiction, so it has semi-magical engineering to produce the energy required.  
> **username_4**: @SteveLinton Answers have quality control. Comments, unless outright deleted get to appear at the top of the page.  
> **username_5**: @antispinwards, pointing out the relative scales involved certainly does fall within the scope of Astronomy.  
> **username_6**: @CarlWitthoft And semi-magical gravity that can suddenly increase or decrease just as your trying to slingshot around Jupiter (at least in the film version on Netflix).  That was about the the point I just threw the whole idea of finishing it out the window.  I probably should have done so earlier with how they described what was happening with the sun, but I'm more willing to forgive a nonsensical background element than I am a nonsensical plot device mid-story.  

---

## 2 answers

### Answer by username_1 on 2020-08-05. Score: 19

No, we cannot.

It's relatively simple math to show that we are a very long shot from changing Earth's orbit by anything significant at all: consider the kinetic energy of Earth in its current orbit, and do the same math for that in the desired orbit:

$ E\_{kin} = \frac{m\_E}{2}v^2 \approx \frac{m\_E}{2}\frac{GM\_S}{a}$

where $m\_E = 6\cdot 10^{24}$kg is Earth's mass, $M\_S=2\cdot 10^{30}$kg is the solar mass and $a=150\cdot 10^9$m is the distance from Earth to sun. I used the approximation in calculating orbital velocity $v = \sqrt{\frac{GM\_S}{a}}$ that the Earth mass, is much smaller than the Sun's mass. So current orbital velocity is (using numbers as above) $29822$m/s.

Now, changing oribital distance outward by 1%, thus by $1.5\cdot 10^9$m, to $151.5\cdot 10^9$m yields a speed of $29674$m/s - and in energy that subsequently gives a difference of $2.64\cdot 10^{31}$J to move Earth's orbit about 1% to further from the Sun.

Annual world primary energy production currently [is around](https://en.wikipedia.org/wiki/World_energy_consumption) $10^{20}$J - so **we "just" need to produce 100.000.000.000 times the yearly energy production of the entire world to change Earth's orbit about 1%**. And that implies that we have a technique to transfer energy 100% into Earth orbital velocity - something which cannot exist either due to simple thermodynamic argument.

Edit to add: Another way to argue is the rocket way: typical speed of conventional rocket exhausts are a few km/s, which is less than needed to leave Earth's orbit - that's why you need multi-stage rockets to get anything into orbit. But if you want to move the whole Earth with a rocket motor, you need a propellant which is fast enough that it directly leaves Earth's gravitational field - or you will not be able to create any effective change of momentum and only move around mass in the Earth system itself. So you need to make some substantial technological advances here, too - or some entirely different technique.

> **Comments:**
> **username_7**: Effective exhaust velocity isn't the reason for multiple stages to orbit. It's the mass ratio element in the [Tsilokovsky rocket equation](https://en.wikipedia.org/wiki/Tsiolkovsky_rocket_equation) that's the main culprit. It's _mathematically_ possible to single-stage-to-orbit on a black powder rocket, but good luck building a light enough rocket that can contain all the black powder you'd need for it.  
> **username_5**: @username_7, effective exhaust velocity *is* the reason why we can't use chemical rockets to move the Earth around: in order for a rocket engine to have a net effect on the Earth's momentum, the exhaust needs to be moving faster than escape velocity.  If it doesn't, the exhaust will (eventually) come back and return its momentum to Earth.  
> **username_8**: This argument is correct but it entirely disregards the possibility of using energy sources outside of Earth, like for example the orbital energy of Jupiter (https://link.springer.com/article/10.1023%2FA%3A1002790227314). Another important point against your conclusion is the amount of time. If we operate in terms of a hundreths of thousands of years we in fact move Earth with smaller power outputs.  
> **username_1**: If you take as long as civilisation is already old (10.000 years), you only need continuously for the next 10.000 years 10.000.000 times our current total energy production. Sources outside earth exist, and can be tapped, but don't change the energy equation.   Changing the trajectory of a body of 1/100000 of earth mass drastically and controlled does not solve but mostly moves the energy problem from earth to the asteroid or kuiper belt. Additionally it creates the problem that you willfully create a potential planet buster, an object rated most dangerous on each planetary protection scale.  
> **username_1**: Interesting study, though. "optimistic minimum energy expenditure is about 10^36 erg" (1.000.000 yearly energy productions) and "this scheme would consume a number of large Kuiper Belt objects". These are 100km-diameter bodies sent to pass Earth repeatedly at 1/40 of moon distance. This makes it more concept than 'modern technology". One should also mind the last sentence of the paper: "The collision of a 100-km diameter object with the Earth at cosmic velocity would sterilize the biosphere most effectively, at least to the level ofbacteria. This danger cannot be overemphasized"  

---

### Answer by username_9 on 2020-08-05. Score: 3

I'll go out on a speculative limb and say **yes**, maybe, depending on the definition of "significant".

[Planetmaker's answer](https://astronomy.stackexchange.com/a/38300/34727) notes the infeasibility of raising Earth's orbit if *nothing else changes*. But what if we also lower some other body's orbit at the same time?

First, let the orbital energy of an object with mass $m$ orbiting the Sun with mass $M\_S$ at an average distance of $a$ be its kinetic plus potential energy with respect to the Sun:

$E\_k + U = \frac{1}{2}m v^2 - \frac{G M\_S m}{a} = \frac{1}{2} m (\sqrt{\frac{GM\_S}{a}})^2 = \frac{G M\_S m}{2a} - \frac{G M\_S m}{a} = -\frac{G M\_S m}{2a} $

Our goal is to raise the Earth's average orbital radius by 1%. Using the above equation and the specific values listed at the end, we need $2.62 \times 10^{31} \ \mathrm{J}$ to do that. (This is all consistent with username_1's calculation, I just want to show my own work.)

Where can we get this energy? Let's try stealing [Ceres](https://en.wikipedia.org/wiki/Ceres_(dwarf_planet)). If we drop its orbital radius down to match Earth's, we gain $2.65 \times 10^{29} \ \mathrm{J}$. That's only 1% of the required energy. But if we instead are content to change Earth's orbit by 0.01% (is that "significant"?) then we have enough energy to do it in Ceres. If not, we need to get more bodies involved. (Since Ceres alone is already about 30% of the asteroid belt mass, they will need to come from elsewhere.)

How do we transfer energy from Ceres to Earth? We arrange for a series (no pun intended) of [Gravitational slingshots](https://en.wikipedia.org/wiki/Gravity_assist) between the two bodies, each time letting Ceres pass just ahead of the Earth, thereby transferring energy to the latter. (As an outline of the encounter plan, my basic idea is we start by lowering its periapsis to match Earth, then all encounters happen at Ceres periapsis, thus preserving the possibility of future encounters.)

How do we change the orbit of Ceres to cause these slingshots? We apply the same technique, recursively if needed. Find something else nearby, presumably also in the asteroid belt, whose orbit we can perturb to cause encounters with Ceres, gradually steering it toward the eventual encounter with Earth. The bottom of the recursion is some object small enough to be pushed (perhaps slowly) into an encounter with the next object using existing spacecraft and propulsion technology.

This would of course take a long time, at least tens to hundreds of thousands of years, but still well short of the hundred billion years username_1 cited to move Earth using terrestrial energy sources.

At the core of this idea is the observation that N-body gravitational systems are chaotic, meaning that small changes in initial conditions can cause very large changes in later system state. To move the world, [Archimedes](https://en.wikiquote.org/wiki/Archimedes) asked for a lever and a fulcrum. But with modest technology, accurate foresight, and ample patience, in principle we should be able to manipulate the solar system almost at will without either.

The Wikipedia [Asteroid capture](https://en.wikipedia.org/wiki/Asteroid_capture) article discusses some related concepts.

Specific numbers used in calculations (generally taken from Wikipedia):

* $G = 6.67 \times 10^{-11} \frac{\mathrm{m}^3}{\mathrm{kg} \ \mathrm{s}^2}$
* $M\_S = 1.99 \times 10^{30} \ \mathrm{kg}$
* $m\_\mathrm{Earth} = 5.97 \times 10^{24} \ \mathrm{kg}$
* $a\_\mathrm{Earth} = 150 \times 10^9 \ \mathrm{m}$
* $m\_\mathrm{Ceres} = 2.38 \times 10^{20} \ \mathrm{kg}$
* $a\_\mathrm{Ceres} = 414 \times 10^9 \ \mathrm{m}$

> **Comments:**
> **username_0**: Very interesting approach! Thanks  
> **username_8**: The actual core idea has been studied by researchers. With a carefully planed strategy we could use a bunch of asteroids to transfer a bit of Jupiter's orbital energy to Earth's. With current technology we would be able to move our planet at a rate that allow us to mantain a priviledged position in the habitable zone of our star as it gets hotter (and thus the habitable zone gets farther away). https://arxiv.org/pdf/astro-ph/0102126.pdf  

---

