Universal gravitation + orbits question

T is the period of the orbit, \mu=G(m_{1}+m_{2}) is the gravitational parameter, and r is the semi-major axis of the orbit.In summary, to calculate the period of a 450kg satellite orbiting at an altitude of 2.45 x 10^6m above the Earth's surface, one can use the formula T^2 = (4*pi^2*mu)/(G*m1*m2)*r^3, where mu is the gravitational parameter and r is the semi-major axis of the orbit. Alternatively, if the orbit is circular, one can use the equation v_orbit = sqrt(r_orbit*g_orbit).
  • #1
davie08
115
0

Homework Statement


A 450kg satellite is to be placed at an altitude of 2.45 x 10^6m above the Earth surface. Calculate the period the satellite will have when orbiting at that altitude.


Homework Equations



m2g = Gm1m2/R^2 = m2v^2 = m2(4pie)^2 R /T^2 = m2 2pie v/T

Ac=4pie ^2 R / T^2

The Attempt at a Solution



Alt= r- rp
2.45x10^6m= r -6.37x10^6m
8.82x10^6m = r

I don't no what equation to use next
 
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  • #2
davie08 said:
Gm1m2/r^2 = m2v^2

This is wrong it should be [itex]Gm_1m_2/R^2 = m_2v^2/r[/itex]

davie08 said:
m2v^2 = m2(4pie)^2 R /T^2

Is also wrong I am not sure what you did here. You're also making one big equality chain which does not hold.

Start with [itex]Gm_1m_2/r^2 = m_2v^2/r[/itex]. Do you know a formula that relates v to T for a circular orbit?
 
  • #3
there are several aproches to this problem. If it is a circuler or bit you could use use
[tex]v_{orbit}=\sqrt{r_{orbit}g_{orbit}}[/tex]

If it is not a circuler orbit you could use,

[tex]T^{2}=\frac{4\pi^{2}\mu}{Gm_{1}m_{2}}r^{3}[/tex]
 

Related to Universal gravitation + orbits question

1. What is the theory of Universal Gravitation?

The theory of Universal Gravitation, also known as Newton's Law of Universal Gravitation, states that every object in the universe attracts every other object with a force directly proportional to their masses and inversely proportional to the square of the distance between them.

2. How does the theory of Universal Gravitation explain orbits?

The theory of Universal Gravitation explains orbits by stating that the gravitational force between two objects (such as a planet and a star) causes them to be pulled towards each other. This force is countered by the object's velocity, resulting in a circular or elliptical orbit.

3. What is the difference between geocentric and heliocentric orbits?

A geocentric orbit is one in which an object, such as a satellite, revolves around the Earth. A heliocentric orbit is one in which an object revolves around the sun. The difference lies in the center of mass around which the orbiting object revolves.

4. Why do planets in our solar system have elliptical orbits?

Planets in our solar system have elliptical orbits because of the gravitational pull of the sun. The sun's mass is not evenly distributed, which causes the planets to be pulled closer or farther away at different points in their orbit, resulting in an elliptical path.

5. Does the theory of Universal Gravitation apply to all objects in the universe?

Yes, the theory of Universal Gravitation applies to all objects in the universe. However, for objects with extremely small masses, such as atoms, the effects of gravity are negligible and other forces, such as electromagnetic forces, have a greater impact.

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