Q (1 Viewer)

CM_Tutor

Moderator
Moderator
Joined
Mar 11, 2004
Messages
2,644
Gender
Male
HSC
N/A
CrashOveride said:
a projectile is fired vertically upwards from the earths surface with velocity U m/s. The retardation due to gravity is given by the law k/x^2 where x is the distance of the projectile from the centre of teh earth, and k is a constant. The acceleration due to gravity on the earths surface is g. The earths radius is R. Neglecting the air resistance show that if U^2 = gR, then the projectile reaches the height R above the earths surface. What is the time for this journey?

Ok i do all the fundamental stuff in deriving this but i get R(gR-v^2) / (v^2 + gr). Wont cancel :/
As with the method from post #23, above, we have the origin of motion (x = 0) at the centre of the Earth. We have acceleration governed by:

x'' = -k / x<sup>2</sup>, for x &ge; R

We require that x'' = -g at x = R, and so k = gR<sup>2</sup>. Thus, we have x'' = -gR<sup>2</sup> / x<sup>2</sup>, for x &ge; R.

Using this equation with the boundary condition that v = +U at x = +R and x'' = d/dx(v<sup>2</sup> / 2), we find that
v<sup>2</sup> = U<sup>2</sup> - 2gR + 2gR<sup>2</sup> / x

So, put v = 0 and U<sup>2</sup> = gR, and you get 0 = -gR + 2gR<sup>2</sup> / x, which gives x = 2R. That is, the max height (where the particle stops) is 2R from the origin, or R above the surface.

Are you also having a problem with the time part of the question?
 

CrashOveride

Active Member
Joined
Feb 18, 2004
Messages
1,488
Location
Havana
Gender
Undisclosed
HSC
2006
Oh dear, all t'was needed was to put v=0 in my expression above. I'll have a go at the time part :)
 
Joined
Jan 24, 2004
Messages
2,907
Location
northern beaches
Gender
Male
HSC
2004
y = f(x)...sketch y = Ln[f(x)]

how do you do these..? i hate these ones! :(

sorry about the diagram..it's meant to be a cubic
 

CrashOveride

Active Member
Joined
Feb 18, 2004
Messages
1,488
Location
Havana
Gender
Undisclosed
HSC
2006
CM_Tutor said:
As with the method from post #23, above, we have the origin of motion (x = 0) at the centre of the Earth. We have acceleration governed by:

x'' = -k / x<sup>2</sup>, for x &ge; R

We require that x'' = -g at x = R, and so k = gR<sup>2</sup>. Thus, we have x'' = -gR<sup>2</sup> / x<sup>2</sup>, for x &ge; R.

Using this equation with the boundary condition that v = +U at x = +R and x'' = d/dx(v<sup>2</sup> / 2), we find that
v<sup>2</sup> = U<sup>2</sup> - 2gR + 2gR<sup>2</sup> / x

So, put v = 0 and U<sup>2</sup> = gR, and you get 0 = -gR + 2gR<sup>2</sup> / x, which gives x = 2R. That is, the max height (where the particle stops) is 2R from the origin, or R above the surface.

Are you also having a problem with the time part of the question?
Ok i took dx/dt from v<sup>2</sup> = U<sup>2</sup> - 2gR + 2gR<sup>2</sup> / x and then attempted to integrate the RHS from R to 2R but i got something which i dont think is easily integratable. I tried on integrator online and it was some large expression. :/
 

Rorix

Active Member
Joined
Jun 29, 2003
Messages
1,818
Gender
Male
HSC
2005
ToO LaZy ^* said:
how do you do these..? i hate these ones! :(

sorry about the diagram..it's meant to be a cubic

ln1=0
f(x)>0
as f(x) -> 0, ln f(x) -> -infinity
so you have asymptotes x=0, whatever the 2nd intercept is
ln f(x) = 0 in the middle at the peak there
then another asymtote at the 3rd intercept, crosses x axis when f(x)=1, then f(x) -> infinity rather slooooooowly
 

CM_Tutor

Moderator
Moderator
Joined
Mar 11, 2004
Messages
2,644
Gender
Male
HSC
N/A
CrashOveride, have you tried:

Putting in expression for U<sup>2</sup> and making x the subject, then putting this into the expression for x'' (so you have a function of v), and using x'' = dv/dt, integrating with respect to v from v = &radic;(gr) to v = 0?

Just a thought - I haven't done it, so it might not work, but it looks to be worth a try...
 
Joined
Jan 24, 2004
Messages
2,907
Location
northern beaches
Gender
Male
HSC
2004
Rorix said:
ln1=0
f(x)>0
as f(x) -> 0, ln f(x) -> -infinity
so you have asymptotes x=0, whatever the 2nd intercept is
ln f(x) = 0 in the middle at the peak there
then another asymtote at the 3rd intercept, crosses x axis when f(x)=1, then f(x) -> infinity rather slooooooowly
cool..that helped a lot. thanks1!
 

CM_Tutor

Moderator
Moderator
Joined
Mar 11, 2004
Messages
2,644
Gender
Male
HSC
N/A
CrashOveride - I tried the method I suggested - it's messy, but it seems to work. I get the required time as

t = (&pi; + 2)&radic;R / 2&radic;g = 2077.5 ... s

Does this match your answer / the answer given in the book?
 
Last edited:

CrashOveride

Active Member
Joined
Feb 18, 2004
Messages
1,488
Location
Havana
Gender
Undisclosed
HSC
2006
That is the correct answer.

I got x as a function of v and subbed back into x'' = -gR^2.m / x^2
And it appears im going to get a -ve time now....and also how did you eliminate the m ?
 

CM_Tutor

Moderator
Moderator
Joined
Mar 11, 2004
Messages
2,644
Gender
Male
HSC
N/A
I did not have an 'm' anywhere, so I'm not sure where yours comes from. We started with x'' = -gR<sup>2</sup> / x<sup>2</sup>, so there shouldn't be an 'm'.

When I wrote this out, I actually took a slightly different approach. I

* put U<sup>2</sup> = gR into v<sup>2</sup> = U<sup>2</sup> - 2gR + 2gR<sup>2</sup> / x
* rearranged to get 1 / x = (v<sup>2</sup> + U<sup>2</sup>) / 2gR<sup>2</sup>
* then showed that x'' = -(v<sup>2</sup> + U<sup>2</sup>)<sup>2</sup> / 4gR<sup>2</sup>
* By noting x'' = dv/dt, I then showed dt/dv = -4gR<sup>2</sup> / (v<sup>2</sup> + U<sup>2</sup>)<sup>2</sup>
* It follows that the required time is t = &int; (U-->0) dt/dv dv = &int; (0-->U) 4gR<sup>2</sup> / (v<sup>2</sup> + U<sup>2</sup>)<sup>2</sup> dv

So, we now just need to do the integration, and noting that U, g and R are all constant, that isn't too bad.

I used a the substitution v = Utan &theta; to show that

&int; 1 / (v<sup>2</sup> + U<sup>2</sup>)<sup>2</sup> dv = (1 / U<sup>3</sup>) * &int; cos<sup>2</sup>&theta; d&theta;
= v / 2U<sup>2</sup>(v<sup>2</sup> + U<sup>2</sup>) + (1 / 2U<sup>3</sup>) * tan<sup>-1</sup>(v / U) + C, for some constant C

From there, it isn't difficult to evaluate the required definite integral to get

t = gR<sup>2</sup>(&pi; + 2) / 2U<sup>3</sup>

which simplifies to (&pi; + 2)&radic;R / 2&radic;g by using U = &radic;(gr)
 

CrashOveride

Active Member
Joined
Feb 18, 2004
Messages
1,488
Location
Havana
Gender
Undisclosed
HSC
2006
Ok i get up to a point where i have

t = 2gR<sup>2</sup>/U<sup>2</sup> [ 1 / (U<sup>2</sup> + v<sup>2</sup>) + (1/U).arctan(v/U) ] with limits 0 --> U

Evaluating that i end up getting a U<sup>4</sup> on the denominator and i have a minus inconveniencing the numerator
 

CM_Tutor

Moderator
Moderator
Joined
Mar 11, 2004
Messages
2,644
Gender
Male
HSC
N/A
The U<sup>4</sup> has occured because there is a v missing from the numerator of the first term. As for it being negative, it isn't when I do it. The expression you have is correct, apart from the missing v. Here it is:

t = (2gR<sup>2</sup> / U<sup>2</sup>) [ v / (U<sup>2</sup> + v<sup>2</sup>) + (1 / U) * arctan(v / U) ] with limits 0 --> U
= (2gR<sup>2</sup> / U<sup>2</sup>) [ U / (U<sup>2</sup> + U<sup>2</sup>) + (1 / U) * arctan(U / U) ] - (2gR<sup>2</sup> / U<sup>2</sup>) [ 0 / (U<sup>2</sup> + 0<sup>2</sup>) + (1 / U) * arctan(0) ]
= (2gR<sup>2</sup> / U<sup>2</sup>) [ (1 / 2U) + (1 / U) * &pi; / 4], as arctan(0) = 0
= (2gR<sup>2</sup> / gR) * (1 / U) * [(1 / 2) + (&pi; / 4)], using U<sup>2</sup> = gR
= (2R / U) * [(1 / 2) + (&pi; / 4)]
= (R / U) + (R&pi; / 2U)
= R(2 + &pi;) / 2U
= [R(2 + &pi;) / 2] * 1 / &radic;(gR), using U = &radic;(gR)
= (&pi; + 2)&radic;R / 2&radic;g, as required / expected
 
Last edited:

mojako

Active Member
Joined
Mar 27, 2004
Messages
1,333
Gender
Male
HSC
2004
nope.. it cant be a right angle...
the diagram is delberately misleading
(or else there's a typo in the letters)

im still trying to solve it.. ill give it 10-20 minutes or so before i give up :p
 

Users Who Are Viewing This Thread (Users: 0, Guests: 1)

Top