Homework Statement
potential energy function of :
$$
U(x) = 4x^2 + 3
$$
And have to
i) Work out the equation of motion
ii) Prove explicitly that the total energy is conservedHomework Equations$$
F = \frac{dU}{dt}
$$
The Attempt at a Solution
I'm not too sure how to go about this...
Sorry - that answer is correct but Its in thousands. I'd be unlikely to trust
any boss who gave me a job anyway tbh :)I thought that I had accounted for the frictional force during that, damn.
OK
$$
\text{Force net} = 10 - mg\mu_k
$$
Then we have that
$$
F_n = ma
$$
So
$$
a =...
So we have
$$
\frac{1}{2}mv_1^2 - \frac{GMm}{r_1} = \frac{1}{2}mv_2^2 - \frac{GMm}{r_2}
$$
Here we want to solve for ##M##, and can see that every term has ##m## in it (nice!)
so can just drop that :)
Dropping ##m## and multiplying through by 2 gives
$$
v_1^2 - \frac{2GM}{r_1} = v_2^2 -...
So I have ##a = 100, v = 300## after three seconds.
Then I remove the force that's pushing the object and friction slows it to a stop.
Then at three seconds I have the kinetic energy
$$
\frac{1}{2} m v^2
$$
And this is all spent on work against friction (so that the object comes to a
stop...
Ah yes >.< , whoops.
So that the force of friction would be ##0.1 \times 9.81 \times 0.2 = 0.1962##.
The means that during the acceleration phase (from ##t = 0 ## to 3) I have the net
Force would be
$$
F_n = 10 - 0.1962 = 9.8038
$$
Given this I have the work done against friction over...
Thanks - are you just using ##\vec{h}## here to represent angular momentum for
this case? (I've not seen ##\vec{h}##, just making sure that's what this was for
here).
Then from this we have that
$$
h = rv
$$
So for this problem we have, for the perihelion position (where the object is...
Homework Statement
A block of mass 100 grammes was stationary on the flat surface at ##x = 0##. At
time ##t = 0## a horizontal force of 10 Newtons was applied on the block in the
positive x direction during ##\Delta t = 3## seconds.
Find at what x position the block will stop, if the...
OK - so I have that ##f =\sqrt{21}##, and this is the distance from the star to
the 'origin' (where major / minor meet). So from this I can say that the
distance from the star to the orbiting body is
$$
dist = major - f
$$
Which here is
$$
dist = 5 - \sqrt{21} = 0.417242305
$$
So that...
cheers - so for part 4 if I consider the angular momentum ##\omega## then:
##v = \omega r##, and here we have ##r = a##, the semi-major axis and the speed is
##100##km/s.
So we have
$$
\frac{v}{r} = \omega
$$
Which gives us ##\omega = \frac{100}{5} = 20##.
But this doesn't take into...
Homework Statement
A comet moves around a stat in ##xy## plane along elliptical orbit, described by
$$
0.16 x^2 + y^2 = 4
$$
where ##x, y## are in ##AU##
1) Sketch the comet in the ##x,y## coordinate system denoting all orbit parameters
2) Find the semi major and minor axes of the orbit...