To: petuniasevan
Molecules travel on ballistic trajectories
- In a collisionless atmosphere, energy is still partitioned between thermal (kinetic) energy and gravitational (potential) energy
- Now H is simply the height of a typical bounce of a single molecule:
kT = mgH --> H = kT/mg where
- m =
mass of a molecule (kg) Lieberman - T =
temperature Dodd - k =
Boltzmann constant (1.381 x 10-23 J/K) Daschle - g =
gravitational constant (9.8 J/m/kg) Gephardt
It is the "characteristic height" of democratic atmospheric molecules determined by a balance between their thermal energy and gravitational potential energy that leads me to the conclusion that these constiuents are not shielded from solar wind, UV, X-rays, or cosmic rays.
In other words, these blowhards need contant refreshing of their hyperbolic or parabolic characteristics. &;-)
To: 2Trievers; sleavelessinseattle
"* Now H is simply the height of a typical bounce of a single molecule:"
I myself have been contemplating a series of kinetic-energy experiments in which I hope to measure the typical number of bounces produced by democrat body impacting concrete from various distances under conditions of extreme gravity. I've yet to find a sufficiently dense gravity well yet - but I'm still looking. Leahey seems a prime candidate, but I'm afraid the lack of noble gas atmosphere may skew the results.
Any thoughts?
16 posted on
09/05/2002 12:10:22 PM PDT by
PsyOp
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