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« Go Look At The Moon! | Main | Weekend Diversion: The Power of Periphery »

Meet our Second Moon!

Category: AstronomySolar System
Posted on: July 10, 2009 5:54 PM, by Ethan Siegel

The inner Solar System is a pretty bizarre place. Think about the giant planets in our Solar System -- the Jovian planets -- that weigh in from tens to hundreds the mass of Earth.

vt2004-if8-fig4.gif

These giant balls of gas are orbited by all sorts of interesting things, from moons so giant that they have their own substantial atmospheres like Saturn's Titan:

purple_titan.jpg

to captured Kuiper Belt objects, like Neptune's giant moon, Triton:

Triton

to regular natural satellites that formed around the giant planets as they formed, such as Saturn's Dione and Enceladus:

Occulting_Enceladus_PIA10500.jpg

All told, if we look at all the moons in the Solar System, the gas giants have a virtual monopoly on them. If we look at objects bigger than 100 km in diameter, Jupiter has 7, Saturn has 11, Uranus has 8, and Neptune has 6. Hell, even not-a-planet Pluto has 1, the same number as the entire inner Solar System:

inner_planets_small_2.jpg

That's right. Mercury and Venus have no moons, Earth has just the one big one, and Mars has two little captured asteroids (under 25 km apiece) that we generously call moons. For comparison, Jupiter has at least 49 satellites under 25 km, and Saturn has at least 43. Well, if Mars has some captured asteroids, is it possible that Earth has a few, too?

If you only knew...

Cruithne.jpg

Say hello to the (very poorly named) 3753 Cruithne, a rock only about 5 km wide that follows us in our orbit! What do I mean by that? The Earth takes roughly 365 days to orbit the Sun. 3753 Cruithne takes 364 days to orbit the Sun, an impressively close number. From the perspective of the Sun, we look like this:

Orbits_of_Cruithne_and_Earth.gif

And as seen from Earth, 3753 Cruithne makes a horseshoe-shaped orbit!

Horseshoe_orbit_of_Cruithne_from_the_perspective_of_Earth.gif

It isn't technically "our Moon" because it isn't gravitationally bound to us, and is actually expected to be ejected from our orbit in a few thousand years. It will make a close approach to us in 2292, and there will be a gravitational encounter between this satellite and Earth. The dynamics have already been worked out. 3753 Cruithne's orbit will change by about 500,000 km. Earth's orbit? Altered by 1.3 centimeters.

Why is this so neat? We've known for a long time about Trojan asteroids, a group of around 1000 objects that stably orbit the Sun near (but not around) Jupiter:

InnerSolarSystem-en.png

For the very first time, we're starting to detect objects that may do this around Earth and Mars (which is up to four)! Want to know what I find amazing? Newton's law of gravitation, good old this guy:

400px-NewtonsLawOfUniversalGravitation.svg.png

is all it takes to make all of this happen and to understand how. My mind is blown for the week, and I hope yours is, too. Enjoy the weekend!!

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Comments

1

So what effect with those 1.3 cm have on Earth's climate? Will it have any effect on our moon?

Posted by: Technonick | July 10, 2009 3:52 PM

2

Everytime when I read about this subject, I'm awed about how diverse our Solar System is. I always wonder how diverse and different (and similar!) other 'solar systems' might be.

Posted by: Nick | July 10, 2009 4:02 PM

3

I love the horse shoe orbit! It is amazing! And fun!

Posted by: Sweetwater Tom | July 10, 2009 6:48 PM

4

Awesome. :) What magnitude is the rock at perigee?

I propose we land rockets on the rock - we can slam it into the earth to create a long global winter - global warming and overpopulation solved with one space pebble! There might be a little problem with technology being set back a few thousand years though.

Posted by: MadScientist | July 11, 2009 4:39 AM

5

I remember Cruithne playing a key role in a Stephen Baxter novel. Nice to see some real-world information about it.

Posted by: Naked Bunny with a Whip Author Profile Page | July 11, 2009 9:33 AM

6

@technonick
A centimeter will not affect the climate at all. Think about it, Earth's closest and farthest approach differs by a few million kilometers. Plus, it goes closest to the sun is January, winter in the north hemisphere and summer in the south. But we don't see the northern hemisphere swept with ice caps or the south bursting into fire.
You also has to remember, the asteroid is freaking small, while in comparison, the moon is a gazillion times more massive. So its effect on the moon will be minimal.

@mad scientist
You forgot another problem, our extinction. ^_^

Posted by: IBY | July 11, 2009 11:53 PM

7

This is old news for fans of Stephen Fry's QI :-)

http://www.youtube.com/watch?v=D1zuAQAhhMI

Posted by: Heleen | July 12, 2009 12:57 AM

8

So, with the two orbits that close in duration, can we assume that the speed differential is small enough to not make all life on earth disappear should the two dots meet at the intersection of the red and blue line?

Posted by: Mu | July 13, 2009 8:12 AM

9

wow

Posted by: gerlie | October 8, 2009 10:15 AM

10

Mu, there is delta-V because the orbits around the sun aren't the same … and at the end, even if it was very low because the orbits were very similar, the Earth's gravity would take over. The rock would still fall into the Earth. It would hurt.

Posted by: Timberwoof | September 17, 2010 9:20 PM

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