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PiRsq
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How do I find out the minimum speed required for a satellite to place it in a geosynchronous orbit(24 h per orbit)?
I know the height of the satellites orbit. I also know the period.
Originally posted by PiRsq
Yes but how can I calculate the speed at which the satellite was launched at to reach this height?
Originally posted by PiRsq
The books answer is 11.2 km/s which is the escape speed. I am guessing that it was probably required to find the speed at which the satellite should be launched to just escape the Earths gravitational field. Then after that the satellite can be steered to its geosynchronous orbit. Do you think so?
Thus it would take approximately 3125 seconds to get there at a speed of 11.2 km/s, isn't it?
Originally posted by PiRsq
The problem is listed like so:
Consider a geosynchronous satellite with an orbital period of 24h.
a)What is the satellite's speed in orbit?
b)What speed must the satellite reach during launch to attain the geosynchronous orbit?(Assume all fuel is burned in a short period and neglect air resistance)
The answers are :
a)3.1 x 10^3 m/s
b)1.1 x 10^4 m/s (Which I assumed to be 11200 m/s)
Originally posted by Janus
An orbit need not be circular to be geosynchronous. It only needs to be circular to be a geostationary orbit. (And not all 24 hr, circular orbits are geostationary either. )
A geosynchronous orbit is a type of orbit around a planet in which a satellite completes one orbit in the same amount of time it takes for the planet to rotate once on its axis. This results in the satellite remaining in a fixed position relative to the planet's surface, making it ideal for communication and observation purposes.
The minimum speed for a satellite in geosynchronous orbit can be calculated using the formula:
Minimum speed (in meters per second) = sqrt(G * M / r)
where G is the universal gravitational constant, M is the mass of the planet, and r is the distance between the satellite and the center of the planet.
The minimum speed for a satellite in geosynchronous orbit is affected by the mass and size of the planet, as well as the altitude of the orbit. The closer the satellite is to the planet, the faster it must travel to maintain a geosynchronous orbit.
Celestial mechanics is the branch of physics that studies the motion of objects in space, including planets, moons, and satellites. Geosynchronous orbit is a result of the gravitational forces between a planet and a satellite, which are governed by celestial mechanics.
Geosynchronous orbit is commonly used for communication and navigation satellites, as well as weather and Earth observation satellites. It is also used for military and scientific purposes, such as monitoring natural disasters and studying the Earth's climate.