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I'm writing a novel and I'm quite confused if this system could be possible in the real universe. Is it possible that a system exist, where 5 identical planets which could be of same characteristics (Inclination, speed, planetary mass and others) revolve around a single star. Also, What effects would the 5 planets undergo if they are so close? (including the climatic changes and the gravitational, magnetosphere interference.)

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"Klemperer rosette". The five mass figure with no central body has already appeared in fiction (Larry Niven's Ringworld and related novels). –  dmckee Apr 21 '13 at 17:55
I look into it :) I haven't read any of d novels!! –  Karthikeyan KC Apr 21 '13 at 18:11
@dmckee Only he wants a central star :) –  Bernhard Apr 21 '13 at 18:19
Why do you say, "if they are so close?" Are you imagining them as not equally spaced around the circle? –  Ben Crowell Apr 21 '13 at 19:14
What do you say about Asteroid ring? –  Mr.ØØ7 Apr 22 '13 at 11:15
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up vote 6 down vote accepted

No more than two objects in co-orbital configuration have been observed so far. It'd be easy if there existed atleast one satellite (instead of a planet) to one of the planets orbiting around the star. The reason I say this is because, the orbital configuration of the planets can then be thought of as Lagrangian points.

Lagrangian points

Though the L1, L2 and L3 are much less stable compared to L4 and L5, we can infer now that atleast 4 bodies can orbit the star. By this way, we can declare that they share their orbit. Still, the configurations are less likely. A slight perturbation can modify their orbit or sometimes (if unlucky), slam one onto the other...

But it's OK to say that five planets can orbit at the same time. As dmckee and John said, Klemperer rosette might be a good start. Be sure that you still maintain the symmetry (very necessary in Physics) (i.e) a triangle in case of 3 objects, a pentagonal configuration in case of 5, etc...

IIRC, this system is very very rare. As I've told already - during a planetary formation, it's still very unlikely that such a system (with more than three co-orbital config) can be formed.

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It's not just rare. It's so statistically improbably that it's essentially impossible. –  Brandon Enright Apr 21 '13 at 18:27
Does it involves a central star? –  Karthikeyan KC Apr 22 '13 at 17:12
@KarthikeyanKC: I can't understand what you mean by the phrase "central star". But, the lagrangian positions are the approximate solutions for the famous 3-body problem. Two masses revolve around their common barycenter and a third one is kept at one of these points so that they're in equilibrium. The masses should be somewhat comparable. That's all. It can be a star for sure as you can see in the image. In fact, it's real for many satellites have (and have been proposed) to orbit at these points ;-) –  Waffle's Crazy Peanut Apr 22 '13 at 17:22
I referred the Klemperer rosette system here... And i'm more confused... If two masses have to be in equilibrium when they revolve around a common barycenter why need a third mass? –  Karthikeyan KC Apr 22 '13 at 17:29
@KarthikeyanKC: First, I suggest you to have a look at Lagrange points. Roughly speaking, these why questions are pretty complicated to answer directly. Say, two masses are in equilibrium. The necessity of a third mass is because that is the one which is gonna stay in orbit at one of the L-points relative to the other two. If you don't want successive masses, you can stop at 2 for sure ;-) –  Waffle's Crazy Peanut Apr 22 '13 at 17:56
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At least according to these numerical simulations by Bob Jenkins, systems with a small number of equal-sized planets orbiting a massive central body can, in fact, be "stable, in an odd sort of way."

Specifically, the planets do not stay equally spaced around the star, even if they start out (approximately) that way. Rather, they appear to move along their shared orbit on complicated, and likely chaotic, horseshoe-like orbits, while still maintaining an approximately circular shared orbit around the sun and a surprisingly well defined minimum separation between each other.

It should, of course, be noted that these simulations are only suggestive, but not conclusive. I'm not aware of anyone having simulated such as system for periods comparable to the age of solar system, nor of any analytical results on its long-term stability. If you know of any such studies, please tell me!

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I don't have a definitive reference for this, but I'm fairly certain such configurations are unstable to small perturbations. That means the slightest deviation from perfect symmetry will grow and the planets will collide or eject each other into different orbits. The planets could only share an orbit if their prelative positions were being actively maintained.

The Wikipedia article on Klemperer rosettes agrees that they are unstable, but doesn't provide a good reference either.

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This is a Klemperer rosette with a star added at the center, so WP's statement doesn't necessarily tell us much. If we make $n=5$ into a variable, then the large-$n$ limit is unstable with respect to perturbations of the central star, for the same reasons that a ringworld is unstable: physics.stackexchange.com/questions/41254/… . The high-$n$ limit is simpler, because the mass distribution is static, so Earnshaw's theorem applies to the stability of the star, which is at rest. –  Ben Crowell Apr 21 '13 at 19:09
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