What is the orbital velocity at pericenter and apocenter

In summary, one way to lift a satellite into geosynchronous orbit is by using the space shuttle to place it in a low-earth orbit and then using a booster rocket to transfer it to a circular geosynchronous orbit. The orbital velocity of the satellite in low-earth orbit can be found using the formula v = sqrt(g*m/r), and the orbital velocity at pericenter and apocenter of the Hohmann transfer orbit can be found using the formulas Vp = sqrt(mu(2/r-1/a) and Va = sqrt(mu(2/r-1/a)). The time it takes for the satellite to travel from low-earth orbit to geosynchronous orbit can be calculated once the parameters of the Hohmann transfer orbit are
  • #1
dairycat
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One way of lifting a satellite into geosynchronorous orbit is to use the space shuttle to lift it into a circular, low-earth orbit(h=300km) and then use a booster rocket to place the satellite on a hohmann transfer orbit up to a circular geosynchronous orbit. what is the orbital velocity of the satellite while it is still in low-earth orbit? what is the orbital velocity at pericenter, of the appropriate hohmann transfer orbit? what is the orbital velocity at apocenter of the hohmann transfer orbit? how long does it take the satellite to travel from the low-earth orbit to the geosynchronous orbit?

Homework Equations


v=sqrt(g*m/r)
i think Vp=sqrt(U(2/r-1/a)
Va=sqrt(U(2/r-1/a)


The Attempt at a Solution


i found the orbital velocity of low-earth orbit using v=sqrt(g*m/r) = 7.67km/s
i don't know how to find the rest. a little help please?
 
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  • #2
Hi Dairycat, welcome to PF.

First you'll want to determine the parameters of the required Hohmann transfer orbit; it's starting radius, it's ending radius, then it's semimajor axis (a). You'll need the orbital radius of a geosynchronous satellite. Once you have that you can apply the formulas that you've stated.

By the way, it's traditional to refer to Newton's gravitational constant as G (capital G), since small g is "reserved" for the acceleration due to gravity near the Earth's surface. The mass of the large body that something of negligible mass orbits, like the Earth in this problem, is also usually granted capital letter status. Thus [itex] \mu = GM[/itex], where here M would be the mass of the Earth.
 

FAQ: What is the orbital velocity at pericenter and apocenter

What is the definition of orbital velocity at pericenter and apocenter?

The orbital velocity at pericenter is the speed at which an object travels when it is closest to the body it is orbiting. The orbital velocity at apocenter is the speed at which an object travels when it is farthest away from the body it is orbiting.

How is the orbital velocity at pericenter and apocenter calculated?

The orbital velocity at pericenter and apocenter can be calculated using the formula v = √(GM(2/r - 1/a)), where G is the gravitational constant, M is the mass of the body being orbited, r is the distance between the two objects at pericenter or apocenter, and a is the semi-major axis of the orbit.

What factors affect the orbital velocity at pericenter and apocenter?

The orbital velocity at pericenter and apocenter are affected by the mass of the body being orbited, the distance between the two objects, and the shape of the orbit. The more massive the body being orbited, the higher the orbital velocity at pericenter and apocenter. The closer the distance between the two objects, the higher the orbital velocity. And the more elliptical the orbit, the greater the difference between the orbital velocities at pericenter and apocenter.

How does the orbital velocity at pericenter and apocenter impact an object's orbit?

The orbital velocity at pericenter and apocenter determine the shape and size of an object's orbit. A higher velocity at pericenter and apocenter will result in a larger and more elongated orbit, while a lower velocity will result in a smaller and more circular orbit.

Can the orbital velocity at pericenter and apocenter change over time?

Yes, the orbital velocity at pericenter and apocenter can change over time due to various factors such as the gravitational pull of other objects, atmospheric drag, and the changing mass or size of the body being orbited. These changes can cause the object's orbit to become more elliptical or circular.

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