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Parabolic Velocity

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parabolic velocity [¦par·ə¦bäl·ik və′läs·əd·ē]
(astronomy)
The velocity attained by a celestial body in a parabolic orbit.

Parabolic Velocity 

the velocity required for a body—for example, a space probe or an atmospheric particle—to escape from the gravitational field of an attracting body, such as the earth, the moon, or a planet, in a parabolic orbit. It decreases with the distance from the attracting body. Parabolic velocity is an example of a critical spacecraft velocity.



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showed that the simplifying assumptions of parabolic velocity profile, constant physical properties and isothermal operation conditions were sufficient to describe reasonably well the experimental dynamic behavior of a tubular reactor carrying out the solution polymerization of styrene, in spite of the significant flow distortions expected at the analyzed operation conditions, as computed with the help of a very detailed reactor model.
The assumption of a parabolic velocity profile is an over simplification since the tube wall viscosity is usually much greater than the tube center viscosity.
 
 
 
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