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In the 1969 film Doppelganger, scientists discover and then visit an Earth-like planet sharing our orbit but on exactly the other side of the Sun.
Since then, astronomers have ruled out the possibility of such a planet on the grounds that its gravitational effects on other planets and spacecraft would be easy to see.
But that doesn't rule out the possibility of smaller objects sharing Earth's orbit and today, Apostolos Christou and David Asher at the Armagh Observatory in Northern Ireland say they've found one--an asteroid called 2010 SO16.
Near-Earth asteroids are common but SO16 is in a category of its own. First and foremost, it has an exotic horseshoe-shaped orbit (see diagram above) which astronomers believe to be very rare.
Its worth taking a few moments to think about horseshoe orbits. Two points are worth bearing in mind. First, objects further from the Sun than Earth, orbit more slowly. Second, objects that are closer to the Sun orbit more quickly than Earth.
So imagine an asteroid with an orbit around the Sun that is just a little bit smaller than Earth's. Because it is orbiting more quickly, this asteroid will gradually catch up with Earth.
When it approaches Earth, the larger planet's gravity will tend to pull the asteroid towards it and away from the Sun. This makes the asteroid orbit more slowly and if the asteroid ends up in a orbit that is slightly bigger than Earth's, it will orbit the Sun more slowly than Earth and fall behind.
After that, the Earth will catch up with the slower asteroid in the bigger orbit, pulling it back into the small faster orbit and process begins again.
So from the point of view of the Earth, the asteroid has a horseshoe-shaped orbit, constantly moving towards and away from the Earth without ever passing it. (However, from the asteroid's point of view, it orbits the Sun continuously in the same direction, sometimes more quickly in smaller orbits and sometimes more slowly in bigger orbits.)
For SO16, the period of this effect is about 350 years
Horseshoe orbits are thought to be very unstable, since any small gravitational tug can destroy the fragile resonance that has been set up. However, SO16's orbit is surprisingly robust.
Christou and Asher simulated its orbit with slightly different values for parameters such as its semi-major axis. In these simulations, SO16 remained in a horseshoe-shaped orbit for at least 120,000 years and sometimes for more than a million years.
Astronomers know of three other horseshoe companions for Earth but these are all much smaller (SO16 is a few hundred meters across) and none have orbits that are likely to survive for more than a few thousands years.
That makes SO16 kind of special. For anybody willing and able to look, it is currently near one of its points of closest approach, with an absolute magnitude of about 20, lagging the Earth by 0.13 AU, like a stray puppy.
And it will be there for some time, say Christou and Asher. "It will remain as an evening object in the sky for several decades to come."
Originally posted by Illegal Alien
Hi. Interesting thread.
I was thinking of starting one myself about this kind of thing, but you beat me to it.
Is this asteroid the same one as this one en.wikipedia.org... ?
There was another thread on this (Cruithne) in about 2005, but it seemed to generate little interest.
Hopefully yours will remedy this.
Thanks.
Ultimately, Christou and Asher would like to know where it came from, and they have already thought of several possibilities. It could be an ordinary asteroid coming from the Main Belt between Mars and Jupiter. In that case, the random gravitational pull of the different planets would be responsible for its present orbit, something that Tolis and David think is an unlikely proposition. It could also be a piece of the Moon that escaped the gravity of the Earth-Moon system and went into an independent orbit around the Sun. However, the very stability of its orbit means that there is currently no way to transport it from the Moon to where it is now. Finally, 2010 SO16 could represent leakage from a population of objects near the so-called triangular equilibrium points 60 degrees ahead of and behind the Earth in its orbit. Such a population has been postulated in the past but never observed as such objects are always near the Sun in the sky. If they do exist, they may represent relic material from the formation of Earth, Moon and the other inner planets 4.5 billion years ago.
For the time being, the astronomers would like to see the physical properties of the object studied from the ground, especially its colour. "Colour, a measure of an asteroid's reflectivity across the electromagnetic spectrum, can tell you a lot about its origin", they explain. "With this information we can start testing possible origin scenarios with hard data. If it proves to be unique in some way, it may be worth sending a probe to study it up close, and perhaps bring back a sample for laboratory scrutiny."