# Do moons ever have moons of their own?

**URL:** <https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049>\
**Category:** Factual Questions\
**Created:** [November 30, 2003, 12:10pm UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049 "2003-11-30T12:10:18Z")\
**Posts on this page:** 10\
**Page:** 2

<div class="post-metadata">

**Author:** ![Indefatigable](https://avatars.discourse-cdn.com/v4/letter/i/9d8465/32.png) [@Indefatigable](https://boards.straightdope.com/u/Indefatigable)\
**Post date:** [November 30, 2003, 10:12pm UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/21 "2003-11-30T22:12:18Z")

</div>

That’s the thing, I think Pluto is the closest example we have in a planetary situation. Some binary star pairs are closer in mass ratio, I think. Realistically speaking, it would be pretty improbable for two objects with _precisely_ the same mass to end up orbiting each other. The center of mass of the system would be slightly closer to the slightly more massive object, so that one would be called the ‘planet’ and the other would be the ‘moon’.

Yay, my 200th post. 😃

---

<div class="post-metadata">

**Author:** ![boofy\_bloke](https://avatars.discourse-cdn.com/v4/letter/b/9e8a1a/32.png) [@boofy\_bloke](https://boards.straightdope.com/u/boofy_bloke)\
**Post date:** [December 1, 2003, 2:10am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/22 "2003-12-01T02:10:29Z")

</div>

The bigger the primary the smaller the chance of a decent sized moon-moon (i.e. tertiary). Proto-moon-moons would get sucked into the primary or flung away before they had the chance to become locked to a moon (i.e. secondary). The more spatial bodies involved in the orbital dance the more complex the mechanics required to keep them all stable. Still, it’s a Big™ universe so somewhere, there are probably even ?quaternaries.

---

<div class="post-metadata">

**Author:** ![Musicat](https://sea3.discourse-cdn.com/straightdope/user_avatar/boards.straightdope.com/musicat/32/20189_2.png) [@Musicat](https://boards.straightdope.com/u/Musicat)\
**Post date:** [December 1, 2003, 3:11am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/23 "2003-12-01T03:11:35Z")

</div>

> [@](#):
>
> \*Originally posted by Tusculan \*  
> Remember that gravity drops with the square of the distance.

Wouldn’t that be the [cube](http://216.239.41.104/search?q=cache:D3nMYt9QDIgJ:score.kings.k12.ca.us/lessons/Tides_Support_Files/worksheet2.pdf+gravity&hl=en&ie=UTF-8) of the distance?

---

<div class="post-metadata">

**Author:** ![Shalmanese](https://avatars.discourse-cdn.com/v4/letter/s/45deac/32.png) [@Shalmanese](https://boards.straightdope.com/u/Shalmanese)\
**Post date:** [December 1, 2003, 3:50am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/24 "2003-12-01T03:50:22Z")

</div>

Nope, F = Gm1m2/r^2

---

<div class="post-metadata">

**Author:** ![asrivkin](https://avatars.discourse-cdn.com/v4/letter/a/9d8465/32.png) [@asrivkin](https://boards.straightdope.com/u/asrivkin)\
**Post date:** [December 1, 2003, 4:08am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/25 "2003-12-01T04:08:21Z")

</div>

**KP** is correct, if i remember my celestial mechanics correctly. The situation is basically this: A two-body system “wants” to have both bodies locked to each other, which is to say both objects always having the same side facing each other. Most planetary systems are such that the satellites already are tidally locked to their primary, though I believe only one primary (Pluto) is locked to its secondary (Charon). The Moon is locked to the Earth, and is taking energy from Earth’s rotation to lock it. That energy is going into the Moon’s orbit, lengthening its period of revolution. Eventually, the Moon will take enough energy out of the Earth’s orbit that the day will equal a month and the Moon will stop moving (well, there are other effects, but that’s the classical picture). Because the Moon formed at a time and place where its period of revolution was longer than the day, that’s what happens.

For Phobos, the situation is different. Its period of revolution is \* shorter \* than a martian day. Going through the math shows that its orbital energy is going into speeding up the martian day, which makes its orbit smaller. Eventually it will crash into Mars. Deimos is outside the critical distance, and will evolve outward like the Moon.

To the point, then: A hypothetical satellite of the Moon would evolve relative to the Moon the same way. Either it would be orbiting the Moon faster than the lunar day (28 days) and would eventually crash into the Moon, or would be orbiting more slowly and evolve outwards. Once you get that far from the Moon, you’re dealing with a 3-body problem, not a 2-body one, and the Moon’s satellites’ orbit is unstable (not on immediate timescales necessarily, but eventually). The gravitational effect of the hypothetical third party is very small, so the Earth and Moon don’t notice its influence.

For the binary asteroids, there is no third body involved, so orbits can theoretically be stable.

---

<div class="post-metadata">

**Author:** ![Thaumaturge](https://avatars.discourse-cdn.com/v4/letter/t/858c86/32.png) [@Thaumaturge](https://boards.straightdope.com/u/Thaumaturge)\
**Post date:** [December 1, 2003, 8:46am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/26 "2003-12-01T08:46:04Z")

</div>

> [@](#):
>
> \*Originally posted by Musicat \*  
> \*\*Wouldn’t that be the [cube](http://216.239.41.104/search?q=cache:D3nMYt9QDIgJ:score.kings.k12.ca.us/lessons/Tides_Support_Files/worksheet2.pdf+gravity&hl=en&ie=UTF-8) of the distance? \*\*

As your own link says, it’s _tidal_ forces that drop with the cube of the distance. The Actual force only drops with the square. Hence the tidal force of the sun on earth is smaller than the tidal force of the moon, even though the gravitational force of the sun is greater. Tidal forces might be why moons don’t have moons.

---

<div class="post-metadata">

**Author:** ![Thaumaturge](https://avatars.discourse-cdn.com/v4/letter/t/858c86/32.png) [@Thaumaturge](https://boards.straightdope.com/u/Thaumaturge)\
**Post date:** [December 1, 2003, 8:47am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/27 "2003-12-01T08:47:13Z")

</div>

that’s odd

---

<div class="post-metadata">

**Author:** ![Noone\_Special](https://sea3.discourse-cdn.com/straightdope/user_avatar/boards.straightdope.com/noone_special/32/2863_2.png) [@Noone\_Special](https://boards.straightdope.com/u/Noone_Special)\
**Post date:** [December 1, 2003, 10:55am UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/28 "2003-12-01T10:55:47Z")

</div>

> [@](#):
>
> \*Originally posted by Vetch \*  
> \*\*[This](http://www.ast.cam.ac.uk/HST/press/pluto.html) might back up that statement.  
> Charon is approx. half the size of Pluto.
> 
> V \*\*

Eh… no.

Charon is approx. half the **diameter** pf pluto. All else being equal, that would make pluto **8 times** (2^3) more massive than Charon - so “half the size” is not really correct.

Dan Abarbanel

---

<div class="post-metadata">

**Author:** ![Musicat](https://sea3.discourse-cdn.com/straightdope/user_avatar/boards.straightdope.com/musicat/32/20189_2.png) [@Musicat](https://boards.straightdope.com/u/Musicat)\
**Post date:** [December 1, 2003, 3:10pm UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/29 "2003-12-01T15:10:10Z")

</div>

**Thaumaturge,** the link got screwed up cause vB interpreted an internal string as a smiley. To prevent that, check “Disable Smilies” just before submitting (problems like that should show up on preview).

I confess I have forgotten my physics (how often do I have to compute the attraction of two bodies other than near my girlfriend? 🙂 ). But the site linked to above says

> [@](#):
>
> The force of gravity varies inversely with the cube of the distance.
> 
> Examples: If the distance doubles, the force of gravity is divided by 8 (2[sup]3[/sup]).If the distance is 50% greater (1.5), the force of gravity is divided by 3.375(1.5[sup]3[/sup])

Is this site wrong? If so, are tides (water) subject to a different equation than other parts of the same celestial body like rocks and gases?

---

<div class="post-metadata">

**Author:** ![Tusculan](https://avatars.discourse-cdn.com/v4/letter/t/ecd19e/32.png) [@Tusculan](https://boards.straightdope.com/u/Tusculan)\
**Post date:** [December 1, 2003, 3:24pm UTC](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049/30 "2003-12-01T15:24:32Z")

</div>

> [@](#):
>
> “The force of Newtonian gravity falls off as the square of the distance,” explains Lebo, “but tidal forces decline as its cube. Tides are caused by gravity, so why aren’t they the same? The reason is simply that tidal stretching comes from a difference in the gravitational pull felt on two sides of a body. In a 1/r2 gravitational field, the difference in gravity between any two points falls off as the cube of the distance, not the square.”

[Science@NASA](http://science.nasa.gov/headlines/y2000/ast04may_1m.htm)

See also Wikipedia on [gravity](http://en2.wikipedia.org/wiki/Gravity) and [tidal force](http://en2.wikipedia.org/wiki/Tidal_force).

[Previous page](https://boards.straightdope.com/t/do-moons-ever-have-moons-of-their-own/216049.md?page=1)
