I like the fact you asked about an explanation of laws of motion, not a straight answer to a given question although the answer is really a bit of a biggy!.
The following equations are the basic ones used in most Newtonian physics motion calculations:
(^2 means squared so v^2 means v squared. * is multiply)
S=u*t+0.5*a*t^2
v^2=u^2+2*a*S
v=u+a*t
Where:
S=distance
u=starting velocity
v=ending velocity
a=acceleration
t=time
When you bring in forces and momentum you'll need the following:
f=ma
Kinetic energy e=0.5*m*v^2
p=m"v
Where:
f= force
m=mass
e=energy
p=momentum
2006-06-30 10:17:13
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answer #1
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answered by Anonymous
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How do I do it? Which equations of motion? I mean there are many systems, with multiple simplifications. I take the Bousinesq, inviscid, linearized equations under the traditional approximation and then solve. You can reduce the system to a single equation if there is no forcing. Of course this is for stratified fluid dynamics, not solid mechanics. I assume you want to calculate free bodies in a gravitational field. If so, get a good grounding in elementary calculus, then many of the introductory physics text will be easy for you. Try the site below. Have fun!
2006-06-30 10:12:50
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answer #2
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answered by Karman V 3
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Force = mass x acceleration
Velocity = integral over time of acceleration
Distance = integral over time of velocity
2006-06-30 09:57:05
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answer #3
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answered by Anonymous
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http://www.physicsclassroom.com/Class/1DKin/U1L6a.html
2006-06-30 09:55:04
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answer #4
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answered by Anonymous
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