Johio said:
1. In the continuum between a completely circular orbit, and a maximally elliptical orbit, what characteristics of the orbital body and the gravitational source are the prime determinants of the degree of ellipticality?
Energy, angular momentum, and mass. Closed orbits (circles and ellipses) result if the total mechanical energy is negative. A non-negative energy means the objects aren't in what most people think of as orbits. They are instead on an escape trajectory.
Given a fixed set of masses and a fixed energy, a circular orbit will arise only for one exact value for angular momentum. This means circular orbits never really happen in nature. There is always going to be some deviation between the ideal value and the real value. Everything else (assuming a negative energy) corresponds to an elliptical orbit. Eccentricity becomes one in the extreme of zero angular momentum. This is a radial orbit where the objects are moving in a straight line right toward one another.
Another reason circular orbits never occur in our solar system is that these circular orbits, elliptical orbits, parabolic orbits, and hyperbolic orbits only occur with two bodies that are gravitationally isolated from the rest of the universe. Our solar system is not an isolated 2-body system; those Keplerian orbits are an approximation of reality.
2. As the orbit becomes more and more elliptical, wouldn't the speed of the body increasingly vary? (ie. Speed up as it "falls" towards the sun and slow down once it slingshots past and is recaptured by gravity - much in the pattern of a comet falling from the Oort cloud...)
Yes. One way to express this is via the
vis viva equation,
v^2 = G(M+m)\left(\frac 2 r - \frac 1 a\right)
Google "vis viva equation" for more.
3.1 Is it true that everything in the universe is in (to some degree) circular/spiralic motion around something else? In other words, as with fractals; on a micro scale, electrons orbit the nuclei in all known matter, and on a macro scale, planets orbit around a sun, and so on up the scale?
No.
First off, the only thing electron orbitals have in common with planetary orbits is that both have the letters o-r-b-i-t in them. The model of electrons circling the nucleus as planets orbit the Sun was one of the earliest attempts to model the atom. It is demonstrably false.
Going down from stars to planets to moons, it is very hard for moons to have moons, and essentially impossible further down the scale. Moons are the end of the line for all practical purposes. Going up from stars, stars orbit about the galaxy in which the stars reside, groups of galaxies form clusters, groups of clusters form superclusters, but that's about it.
The concept of Keplerian orbits is not valid for galaxies and larger structures. There's no large central mass about which smaller masses orbit. Another problem, particular for those very large structures, is the expansion of space.
If so, is our solar system in rotation around something? Is it the Sirius cluster?
The solar system is a part of the Milky Way galaxy, which in turn is a member of the Local Group, which in turn is a part of the Virgo Supercluster.
3.2 If that is true, do we know what the length (in time) of the cycle is?
Yes, for the Sun about Milky Way. It's about 250 million years, but its a bit tough calling this an "orbit" in the sense you are thinking of. Larger structures: No. They just aren't orbits any more in the sense that you are thinking. Note: The Milky Way appears to be on a collision course with the Andromeda galaxy.
3.3. Also, do we know the degree of ellipticality of the orbit? (Is it more like a cometary orbit, or more like a planetary orbit?
None of the above. It's not even quite right to talk about eccentricity any more.