?!
We don't need to compare but to explain the Poldo
Tackle systems shown in this thread.
--dl*
====
<
I'm sorry, I made a mistake in this post:
I'm correcting the original post using red color!
errata corrige:
4L <correct>, 2L <wrong>
F = 1/4 W <correct>, F = 1/2 W <wrong>
and so IMA is 4:1 <correct>, and so IMA is 2:1 <wrong>
we have F_righthand + F_lefthand= 1/4W <correct>, we have F_righthand + F_lefthand= 1/2W <wrong>
and so F_righthand = F_lefthand = 1/8W <correct>, and so F_righthand = F_lefthand = 1/4W <wrong>
please see Reply #19Hi Dan,
you are right, here I am.
The principle of conservation of energy helps us to solve the (ideal) problem (i.e. only conservative forces act).
(for reference see Feynman Lectures on Physics Vol.1,ch.4)
The general principle is:
<change in energy> = <force> x <distance force acts through>
The formula for gravitational potential energy is:
<grav. pot. energy> = <weight> x <height>
Let's consider a rope 6L in length and a load of weight W:
- at its maximum extension Poldo tackle is 3L in length, (we can suppose <grav. pot. energy> = 0, i.e. <height> = 0)
- at its minimum extension, Poldo tackle is 2L in length, (<grav. pot. energy> = W x 1L)
(see figure Poldo_max-min_ext.jpg)
We have gained a change of energy (from 0 to WxL) as "our" force (let's call it F) has been acting on the Poldo tackle, but we have pulled the rope for a displacement of
4L in length (our force F has done a work of Fx
4L) whilst we have lifted the load only by 1L in length (the force of gravity has done a work of Wx1L (remember W is the force of gravity acting on the load)).
Now, F x
4L has to be equal to W x 1L (for the principle of conservation of energy)
and then
F = 1/
4 W
and so IMA is
4:1
Note: if we use both hands (simultaneously and with the same force acting on points RH and LH in the figure (right hand upwards, left hand downwards))
we have F_righthand + F_lefthand= 1/
4 W
and so F_righthand = F_lefthand = 1/
8 W
Curiosity: look at figure Poldo_Super.jpg for a super-min-extension of Poldo tackle!
s.