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Does Gravity bend Gravity? |
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| Oct4-12, 08:35 PM | #18 |
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Does Gravity bend Gravity?http://en.wikipedia.org/wiki/Gravitoelectromagnetism Very fascinating stuff. |
| Oct5-12, 01:41 AM | #19 |
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Also, it's an interesting fact that if you write Einstein's equations in five dimensions, you get Maxwell's equations
http://en.wikipedia.org/wiki/Kaluza_Klein This is a deep and profound fact although people aren't sure exactly what it means. |
| Oct5-12, 09:08 AM | #20 |
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I'd love to do research in GR if I didn't care about ever finding a job. :) |
| Oct5-12, 06:14 PM | #21 |
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A "gravitational collective" bending another, singular gravitational force. A very good question actually when one deeply thinks about this. I immediately look towards black holes for a possibility of two gravitational forces bending each other, and/or individually yielding to another gravitational source. A gravitational collective (as I call it just to simplify the meaning), such as the sun, moon, and planets within the inner and outer solar system would effect each others individual gravitational forces, yet, the effects are shared so this would happen as one whole collective. For example, the earths gravity effects the moon, and thus the moons gravity effects the earth (Jupiters gravity effects its moons, as well as every other planet in the system to separate but certain degrees). The stability of our system is due to the forces from each body acting on one another and therefore keeping each other 'in-line', such as the orbits, and planetary rotations.
My further question towards this topic would be how did our system balance itself out, down to the tiniest fractions of earths position relative to the sun, to the position of the moon to balance earth, to the rate of it's rotation and orbital path which are the effects which caused our apparently perfect 24 hour days, and 12 month calendars? I could get into details on how seemingly perfectly placed each planet is but then this would be too long a post, so I'm simply asking was our goldilocks position simply a result of murphys law over time or something else? |
| Oct6-12, 01:28 AM | #22 |
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If you have four dimensions where three are space and one is time, a curious thing happens when you define the surface of a 4D "sphere" of constant radius where the definition is that all surface points have the same distance to the origin... d=sqrt(x^2 + y^2 + z^2 - c^2t^2). Its three dimensional space projection, a 3d sphere, grows hyperbolically for t>0. |
| Oct8-12, 07:10 AM | #23 |
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| Oct8-12, 07:20 AM | #24 |
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The way that people have worked the problem since the 19th century is to calculate things in terms of "fields." An object creates a gravitational, electromagnetic or whatever field, and the field then influences the behavior of other objects. So if you have two objects, their gravitational fields will add up. And if you have two situations in which you have the same field, it doesn't matter what the original objects were. Now there *are* situations called resonances in which objects do end up in perfect synchronization. For example, one revolution of the moon is one rotation. What happens is that you end up in situations where a synchronized system happens to be the state with the lowest energy, and that happens a lot in the solar system. |
| Oct8-12, 11:38 AM | #25 |
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I know of no particular reason earth orbit could not be substantially different than it is and still be stable. |
| Oct8-12, 08:23 PM | #26 |
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The assumption before exoplanet observation was that our solar system was typical, and even with our limited data, it's pretty clear that this is not the situation. It turns out that it's very hard to keep N-bodies dynamically stable. I know people who have at least speculated that Titus-Bode is an application of the anthropic principle. Most solar systems don't have well spaced planets, but solar systems without well spaced planets end up without astronomers. |
| Oct9-12, 02:26 AM | #27 |
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| Oct9-12, 02:58 AM | #28 |
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http://www.nature.com/nature/journal...ture03539.html http://www.nature.com/nature/journal...ture03540.html http://www.nature.com/nature/journal...ture03676.html |
| Oct9-12, 04:52 AM | #29 |
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See http://en.wikipedia.org/wiki/Stabili...e_Solar_System for a counter example.
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| Oct10-12, 01:31 PM | #30 |
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Observational biases in determining extrasolar planet eccentricities in single-planet systems http://arxiv.org/abs/1008.4152v1 Based on 2006 data, you could argue that as many as one third of large planets have circular orbits, but that's enough to make the solar system uncommon. With the new Kepler data, the solar system also looks pretty uncommon since most of the planets have non-circular orbits.... The Exoplanet Eccentricity Distribution from Kepler Planet Candidates http://arxiv.org/abs/1203.1631 The argument is whether the solar system is atypical-uncommon or atypical-rare.... The fact that most planets have eccentric orbits was a big shock. The belief in 1990 was that since gas and dust go into circular orbits in a disk, that they would end up with nice circular planetary orbits. This wasn't what people found.... as far as See http://en.wikipedia.org/wiki/Stabili...e_Solar_System for a counter example. Our solar system is pretty stable. However what people are finding is that if you just put some random planets into a solar system, it's hard to keep them from hitting each other, and doing some very complex things. http://arxiv.org/abs/0903.4700 Planet-planet scattering leads to tightly packed planetary systems http://arxiv.org/abs/0801.3226 Extrasolar Planet Interactions This is all starting to form a nice picture. Solar systems go through a phase in which planets are in eccentric orbits and they hit each other. Most never leave that state, but we were lucky, and our solar system ended up in a stable system. http://arxiv.org/abs/0706.1235 From mean-motion resonances to scattered planets: Producing the Solar System, eccentric exoplanets and Late Heavy Bombardments |
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