Spacecraft Launches: Perigee & Apogee - Why Terminate?

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SUMMARY

Spacecraft launches are typically terminated at either perigee or apogee to facilitate the transition into geosynchronous orbits. A geosynchronous transfer orbit (GTO) is established with an apogee of 35,786 km (22,236 miles), where the spacecraft's engine is fired to circularize the orbit. The discussion highlights the importance of understanding the definitions of perigee and apogee, as well as the calculations involved in determining orbital radius based on period. Key formulas include those for centripetal force and gravitational force, which are essential for calculating the radius of orbit.

PREREQUISITES
  • Understanding of orbital mechanics, specifically geosynchronous orbits
  • Familiarity with the concepts of perigee and apogee
  • Knowledge of gravitational force and centripetal force equations
  • Basic proficiency in physics formulas and calculations
NEXT STEPS
  • Study the derivation of the radius of orbit from the period using gravitational and centripetal force equations
  • Learn about the specifics of geosynchronous transfer orbits (GTO)
  • Research the implications of geostationary orbits for satellite communication
  • Explore the relationship between orbital velocity, radius, and period in circular motion
USEFUL FOR

Aerospace engineers, astrophysicists, and students studying orbital mechanics will benefit from this discussion, particularly those focused on satellite deployment and orbital calculations.

jose medina pedraza
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why spacecraft launches are usually terminated at either perigee or apogee?
 
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jose medina pedraza said:
why spacecraft launches are usually terminated at either perigee or apogee?
Who says they are? I'm not even sure what you are talking about as it doesn't seem to make sense.
 
jose medina pedraza said:
why spacecraft launches are usually terminated at either perigee or apogee?

As Phinds said ... that didn't make a lot of sense

do you understand what the definitions perigee or apogee are ?
Describe what you think they are and we can work from there :smile:D
 
Perhaps the OP is referring to the practice of launching satellites into Geosynch.

From here: http://www.braeunig.us/space/orbmech.htmGeosynchronous orbits (GEO) are circular orbits around the Earth having a period of 24 hours. A geosynchronous orbit with an inclination of zero degrees is called a geostationary orbit. A spacecraft in a geostationary orbit appears to hang motionless above one position on the Earth's equator. For this reason, they are ideal for some types of communication and meteorological satellites. A spacecraft in an inclined geosynchronous orbit will appear to follow a regular figure-8 pattern in the sky once every orbit. To attain geosynchronous orbit, a spacecraft is first launched into an elliptical orbit with an apogee of 35,786 km (22,236 miles) called a geosynchronous transfer orbit (GTO). The orbit is then circularized by firing the spacecraft 's engine at apogee.

 
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Drakkith said:
Perhaps the OP is referring

I hope this thread doesn't turn into the guessing game "maybe the OP means..."
 
Yes Drakkith, that's what I meant, but which formulas do I use to calculate the radius 35,786 km (22,236 miles), by knowing that its period is 24 H.
 
I can't help you there at the moment. I'd have to dig around to see if it's just basic mechanics stuff, or if it's something more complicated.
 
Yep I tried but I don't understand the programming language
 
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jose medina pedraza said:
Yes Drakkith, that's what I meant, but which formulas do I use to calculate the radius 35,786 km (22,236 miles), by knowing that its period is 24 H.
The radius of the orbit is not 22,236 miles. Take a trip to Google and look up what reference point that 22,236 figure is measured from.

Now, to determine the radius of the orbit from the period, you need to know two formulas:

The centripetal force required to keep a body in circular motion: ##f=\frac{mv^2}{r}## where m is the mass of the object, v is its velocity and r is its distance from the center of the earth.

The force of gravity: ##f=\frac{GmM}{r^2}## where G is Newton's universal gravitational constant, M is the mass of the Earth, m is the mass of the object and r is the distance of the object from the center of the earth.

Solve these two equations for the radius at which gravity is exactly equal to the required centripetal force.
[Hint: the orbital velocity is easily found from the orbital radius and period.]
[Hint: pick a consistent set of units (e.g. meters, kilograms, seconds) and use that]
[Hint: keep everything symbolic until you have a formula for the quantity you are after in terms of things that you know]
 
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Thanks
 

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