Originally posted by: Descartes
Originally posted by: Armitage
Originally posted by: Descartes
Originally posted by: Mo0o
The ball has a tangential velocity to the surface of the earth with a constant force inwards. In essen it's constantly falling into the earth but since its traveling trangentially as well, it maintains an geosynchronous orbit.
No body can maintain orbit indefinitely, I believe. There are fairly stable points referred to as Lagrange Points, but those too are only stable over a period relative to the body's masses, velocity, etc. Eventually a body will succomb to one of two things: Decay in the form of gravitational or, in the case of earth, atmospheric; An increase in orbital velocity from some influence (another planet perhaps, an Aristotelian angle pushing it around, etc.) that exceeds its escape velocity and thus pushes it beyond its orbit.
Not really - if you are out of the drag regime (say perigee about 10000 Km altitude) but still in an orbit where the earth is the primary gravitational influence by a large factor, the object will remain in orbit essentially forever. The shape and orientation will change due to various perturbative factors (3rd body, earth geopotential, solar radiation pressure, etc.). But it won't decay or escape.
What I was arguing was the idea of "essentially"; essentially by what timeframe? I'm merely pointing out that over a sufficient timeframe nothing remains forever; hence my use of the word indefinitely...
Until the sun turns into a red giant and expands to envelope the earth - at that point, all bets are off