<p>Since you are talking about real bodies with some extent, yes. The case for point-particles is somewhat different.</p>
<p>Any dissipative system will (by definition) gradually lose energy, and that means that the positions and velocities of the constituent bodies will be confined to (hyper)surfaces in <a href="https://en.wikipedia.org/wiki/Phase_space" rel="nofollow noreferrer">phase space</a> with less and less energy, <span class="math-container">$E=V(\mathbf{x})+K(\mathbf{v})$</span>. Potential energy <span class="math-container">$V(\mathbf{x})$</span> decreases with distance between the bodies and there is a minimum possible separation giving a minimum potential energy, and kinetic energy is always positive <span class="math-container">$K(\mathbf{v})&gt;0$</span>. So as <span class="math-container">$E$</span> declines the distances and velocities have to decline accordingly. Typically things getting close move faster, with kinetic energy increasing as potential energy decreases, but since there is a limit to how much potential energy can decrease before things collide there will eventually be a collision (or, in systems allowing it - not the case here - losing all kinetic energy and ending up in perpetual rest).</p>
<p>(Point particles can cheat in Newtonian gravity by performing weird and physically unrealistic collision or oscillating orbits since they can reduce their potential energy arbitrarily far, see <a href="https://en.wikipedia.org/wiki/Painlev%C3%A9_conjecture" rel="nofollow noreferrer">the Painleve conjecture</a>)</p>
<p>In practice dissipation effects are tiny in planetary systems, and for most planets their orbits will instead be disrupted by rare stellar encounters, chaotic resonances with other planets, or mass-loss from the star when it leaves the main sequence. Planets near stars may be dragged in because of tidal effects, but this matters most if one is a few stellar radii away. In the truly long run gravitational radiation will force any planet to spiral in, but the timescales are staggeringly long.</p>
<p>The number of bodies does not change things, but for many-body systems (<span class="math-container">$N\geq 3$</span>) some bodies can gain enough energy to permanently escape while the rest merge.</p>

CC BY-SA 4.0
2020-12-19T23:31:28.187Z
Are you saying even a two body system on a planetary scale would theoretically eventually merge, if nothing from an outside system interfered? Would this just be from super-slow energy loss through tidal heat?
Connor Garcia
CC BY-SA 4.0
2020-12-20T18:53:18.420Z
Yes, two-body systems with gravitational waves or any other way of shedding angular momentum will move closer. The tidal case is funny, since tides heat up the bodies but conserve angular momentum - they will move closer and orbit faster until they merge.
Anders Sandberg
CC BY-SA 4.0
2020-12-21T11:44:46.840Z
This is a *beautiful answer!*
uhoh
CC BY-SA 4.0
2020-12-19T22:50:38.660Z
2020-12-19T22:50:38.660Z
Anders Sandberg
<p>Suppose we have two gravitating bodies, which are rotating around each other. They are bodies and are affected by deformation caused by tidal forces. Moving tidal waves suck energy from the axial rotation of these bodies. After some time their axial rotation will be synced with orbital rotation and tidal waves will be stopped. Like Moon orbital rotation around Earth is synced with its axial rotation. Maybe I missed some additional effects but it seems to be a quite accurate assumption.<br />
Except for some special cases, if we have three orbiting bodies, their orbital rotation cannot be synced with axial rotation altogether.  Tidal waves in such a system will exist and suck energy indefinitely. And the only source of energy is potential body energy. Will they fall?</p>
<p>I understand that such effects should be very small; it hardly can be measured in the solar system, because the variation of mass of planets and the Sun causes a much higher effect.</p>
<p>But anyway are there any measures that support the existence of such an effect for <em>something</em>? Or is there theoretical proof that this effect does not work for some reasons I missed?</p>

CC BY-SA 4.0
2020-12-18T22:36:13.793Z
Maybe belongs on Physics SE?
WarpPrime
CC BY-SA 4.0
2020-12-18T22:51:36.440Z
It seems to be astrophysical, so I think it's on topic here.
James K
CC BY-SA 4.0
2020-12-19T00:25:15.160Z
Alpha Centauri is doin' fine.
notovny
CC BY-SA 4.0
2020-12-19T18:13:23.543Z
@notovny  Alpha Centarui CorProxima is so far from the other two that it was only confirmed to gravitaionally bound to them in the last few years.  Most of the trinary stars listed here https://en.wikipedia.org/wiki/Star_system#Trinary should be closer and thus better examples than Alpha Centauri.
M. A. Golding
CC BY-SA 4.0
2020-12-21T11:45:53.187Z
@notovny it was four years ago at least ;-)
uhoh
<orbit><rotation><tidal-forces><tidal-locking>
Is a three body gravitating system doomed to collapse?
Askold Ilvento
# Is a three body gravitating system doomed to collapse?

(Asked by: username_0 on 2020-12-18)

Suppose we have two gravitating bodies, which are rotating around each other. They are bodies and are affected by deformation caused by tidal forces. Moving tidal waves suck energy from the axial rotation of these bodies. After some time their axial rotation will be synced with orbital rotation and tidal waves will be stopped. Like Moon orbital rotation around Earth is synced with its axial rotation. Maybe I missed some additional effects but it seems to be a quite accurate assumption.  
Except for some special cases, if we have three orbiting bodies, their orbital rotation cannot be synced with axial rotation altogether. Tidal waves in such a system will exist and suck energy indefinitely. And the only source of energy is potential body energy. Will they fall?

I understand that such effects should be very small; it hardly can be measured in the solar system, because the variation of mass of planets and the Sun causes a much higher effect.

But anyway are there any measures that support the existence of such an effect for *something*? Or is there theoretical proof that this effect does not work for some reasons I missed?

**Tags:** orbit, rotation, tidal-forces, tidal-locking
> **Comments:**
> **username_1**: Maybe belongs on Physics SE?  
> **username_2**: It seems to be astrophysical, so I think it's on topic here.  
> **username_3**: Alpha Centauri is doin' fine.  
> **username_4**: @notovny  Alpha Centarui CorProxima is so far from the other two that it was only confirmed to gravitaionally bound to them in the last few years.  Most of the trinary stars listed here https://en.wikipedia.org/wiki/Star_system#Trinary should be closer and thus better examples than Alpha Centauri.  
> **username_5**: @notovny it was four years ago at least ;-)  

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## 1 answers

### Answer by username_6 on 2020-12-19. Score: 3 | Accepted answer

Since you are talking about real bodies with some extent, yes. The case for point-particles is somewhat different.

Any dissipative system will (by definition) gradually lose energy, and that means that the positions and velocities of the constituent bodies will be confined to (hyper)surfaces in [phase space](https://en.wikipedia.org/wiki/Phase_space) with less and less energy, $E=V(\mathbf{x})+K(\mathbf{v})$. Potential energy $V(\mathbf{x})$ decreases with distance between the bodies and there is a minimum possible separation giving a minimum potential energy, and kinetic energy is always positive $K(\mathbf{v})>0$. So as $E$ declines the distances and velocities have to decline accordingly. Typically things getting close move faster, with kinetic energy increasing as potential energy decreases, but since there is a limit to how much potential energy can decrease before things collide there will eventually be a collision (or, in systems allowing it - not the case here - losing all kinetic energy and ending up in perpetual rest).

(Point particles can cheat in Newtonian gravity by performing weird and physically unrealistic collision or oscillating orbits since they can reduce their potential energy arbitrarily far, see [the Painleve conjecture](https://en.wikipedia.org/wiki/Painlev%C3%A9_conjecture))

In practice dissipation effects are tiny in planetary systems, and for most planets their orbits will instead be disrupted by rare stellar encounters, chaotic resonances with other planets, or mass-loss from the star when it leaves the main sequence. Planets near stars may be dragged in because of tidal effects, but this matters most if one is a few stellar radii away. In the truly long run gravitational radiation will force any planet to spiral in, but the timescales are staggeringly long.

The number of bodies does not change things, but for many-body systems ($N\geq 3$) some bodies can gain enough energy to permanently escape while the rest merge.

> **Comments:**
> **username_7**: Are you saying even a two body system on a planetary scale would theoretically eventually merge, if nothing from an outside system interfered? Would this just be from super-slow energy loss through tidal heat?  
> **username_6**: Yes, two-body systems with gravitational waves or any other way of shedding angular momentum will move closer. The tidal case is funny, since tides heat up the bodies but conserve angular momentum - they will move closer and orbit faster until they merge.  
> **username_5**: This is a *beautiful answer!*  

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