Projectile Motion and Gravity: Calculating Height of a Projectile

AI Thread Summary
The discussion centers on calculating the height of a projectile shot straight up at a speed of 1.30×10^4 km/hr, questioning whether it is a simple projectile motion problem or one influenced by gravity. It is clarified that at such a high speed, the effects of gravity cannot be considered constant, making it a more complex gravity problem. Participants suggest using conservation of energy principles, specifically the equations for kinetic and potential energy, rather than relying solely on the basic projectile motion equations. The importance of adjusting gravitational acceleration for the projectile's upward motion is emphasized. Overall, the conversation highlights the need for a more nuanced approach to high-velocity projectile motion due to gravitational variations.
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Is this projectile motion??

Homework Statement



A projectile is shot straight up from the Earth's surface at a speed of 1.30×104 km/hr.

How high does it go?



Is this just a projectile motion problem? Or is it different because it has something to do with the theory of gravity? (because that is the section we are on in class).
 
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Just a projectile motion problem.
 
Oh, ok...

Thanks
 
I think you mean 1.30*10^4km/hr, but I could be wrong. If so then it is fast enough that you can't take g=constant. So it's a gravity problem. It might be handy to know something about conservation of energy.
 
Oops.. Yes I do mean 1.30*10^4...
 
Ok, then you just need to know an expression for gravitational potential energy that is more general than mgh.
 
I think it's a free-fall motion problem. You use the UAM (uniformly accelerated motion) formula d = (Vf^2 - Vi^2) / 2g, but make sure that g is negative since the projectile was shot upwards.
 
Rylynn97 said:
I think it's a free-fall motion problem. You use the UAM (uniformly accelerated motion) formula d = (Vf^2 - Vi^2) / 2g, but make sure that g is negative since the projectile was shot upwards.

Wrong, the projectile is moving at nearly orbital velocity. You can't take 'g' constant.
 
Use conservation of energy principle.
KE = 1/2.mv^2
PE= GMm/(R + h). Substitute GM = gR^2. Find the value of h
 
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