How to Calculate Satellite Launch Speed for an Elliptical Orbit?

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In summary, a satellite is to be launched from the surface with a speed vo at 300 to the local vertical. If M is the mass of the planet, show that v0=5GM/R.
  • #1
clarabelle
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Homework Statement



It is required to put a satellite into an orbit with apogee of 5R/2, where R is the radius of the planet. The satellite is to be launched from the surface with a speed vo at 300 to the local vertical. If M is the mass of the planet show that v0=5GM/R (use conservation of energy and angular momentum). Assume that the planet is not rotating and that effects due to the planetary atmosphere can be ignored.

Homework Equations



E= 1/2mv2 +J2/(2mr2)- GMm/r

J=mvr

l/r= 1+ecos(x)

The Attempt at a Solution



i have attempted the question more than once, the following working is the attempt which i thought was closest to the answer.

rearranging the first equation gives

2E/m+2GM/r -J2/(m2r2)=0

at rmax, r=5R/2, dr/dt=0, x=pi

therefore
rmax= -GMm/2E [ 1+ sqrt(1+2EL2/G2m3M2)]

i don't know where to go from here.

2nd attempt:

v=v0sin30 (using launch angle)

therefore E= mv02/4- GMm/r

E= -2.integral[Fdr] + 2GMm/r

therefore
2GM/r= v02/4- GM/r

v02= 12GM/r and r=5R/2

therefore
v02= 24GM/5R
 
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  • #2
I don't quite follow what you're doing exactly, especially your first attempt at a solution. As for the second attempt. The kinetic energy of an object is related to its velocity not a component of its velocity. That said are you sure you listed the value we should get for v0 correctly?. First of all the units don't match, although this is fixed by squaring it. Secondly I get a factor 5/4 instead of 5.

Either way you should make good use of the hint.

Both energy and angular momentum is conserved.
So E(launch)=E(apogee). What is the total energy at the launch, potential and kinetic?
What is the total energy when the satellite reaches apogee?

Same questions for angular momentum, however keep in mind that you have to take the angle into account here. What is the angle between r and p at apogee?
 
  • #3
That said are you sure you listed the value we should get for v0 correctly?. First of all the units don't match, although this is fixed by squaring it. Secondly I get a factor 5/4 instead of 5.

this is correct, sorry i typed it wrong the question was supposed to say
v02= 5GM/4R.

i've attempted the question as you suggested but my answer is a factor of 2/3 outs maybe you could spot where I've gone wrong as i can't see any mistakes.

E(launch)= 1/2 mv02+ 3mMG/5R

E(apogee)= J2/2mr2 - GMm/r

J(launch)=J(apogee)= mvorsin30= mv0r/2

therefore E(apogee)= mv02/8 -2GMm/5R

equating the two values for E gives

3/8v02= GM/5R

which gives v02=8Gm/15R.
 
  • #4
The first mistake is:

E(launch)= 1/2 mv0^2+ 3mMG/5R

During launch the distance between the satellite and the center of the planet is not (5/3)R, but is...?

The second mistake comes into life from being a bit sloppy with notation.

E(apogee)= J^2/2mr^2 - GMm/r

This expression is correct, but you are given r at apogee so enter it in the equation right here this will prevent you from making the mistake you're about to make.

J(launch)=J(apogee)= mvorsin30= mv0r/2

Same problem here. You know the r for J(launch) so you can express J(apogee) in terms of that.

The mistake that follows from this is going to this step:

E(apogee)= mv0^2/8 -2GMm/5R

You say that J^2/2mr^2=mv0^2/8, but this is not true. You used J^2=(mv0r/2)^2/(2mr^2). This results in the radii cancelling, but these radii are not the same!

What you should have is: J^2=(mv0 r(launch)/2)^2/(2mr(apogee)^2). Would you have entered the appropriate radii in E(apogee) and J(launch) from the start you wouldn't have made this mistake.

I hope it's clear now, if not just ask again.
 
Last edited:
  • #5
Thank you, that was really helpful.
 

What is an elliptical orbit?

An elliptical orbit is a type of orbit in which an object, such as a planet or satellite, follows an oval-shaped path around another object, typically a larger body like a star or planet.

What causes objects to have elliptical orbits?

Elliptical orbits are caused by the gravitational pull of another object. The strength of this pull depends on the mass of the objects and the distance between them. The closer an object is to the center of the gravitational pull, the more circular its orbit will be. However, if the object is further away, the orbit will become more elliptical.

What are some real-life examples of elliptical orbits?

The most well-known example of an elliptical orbit is the orbit of Earth around the Sun. Other examples include the orbit of the Moon around Earth and the orbits of comets around the Sun.

How do scientists calculate the shape of an object's elliptical orbit?

To calculate the shape of an object's elliptical orbit, scientists use Kepler's laws of planetary motion. These laws state that the orbit of a planet or satellite around a larger object is an ellipse, and the speed of the planet or satellite changes depending on its distance from the larger object.

Can elliptical orbits change over time?

Yes, elliptical orbits can change over time due to external forces such as the gravitational pull of other objects or the effects of tidal forces. These changes can cause an object's orbit to become more circular or more elliptical.

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