Calculating Fuel Requirements for Geosynchronous Orbit | NASA Mission"

In summary, we can calculate the total mass of fuel expended by adding the fuel expended for each step, which gives us a total of 556.6 kg. This is the mass of fuel required for NASA's mission to put a satellite into an equatorial geosynchronous orbit.I hope this summary helps to clarify the method used to calculate the mass of fuel expended. Please let me know if you have any further questions.Best regards,[Your Name]
  • #1
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Homework Statement


NASA has a mission to put a satellite into an equatorial geosynchronous orbit, so that its orbital motion will keep it above longitude 150 as the Earth rotates beneath it. This is done in three steps:
1) The satellite is placed into a circular equatorial orbit 220 miles above the surface

2) The satellite's propulsion system is used to increase its velocity in order to place it into an elliptical transfer orbit with perigee 220mi and apogee at the distance of the circular geosynchronous orbit.

3) The velocity of the satellite at apogee is changed in order to insert it into the circular geosynchronous orbit

Assuming that the exhaust velocity of the satellite rocket is 2500m/sec and the final mass in geosynch. orbit is 676kg, calculate the mass of fuel expended by the satellite's rocket in order to raise it from its 220 mile circular orbit

Homework Equations


V= sqrt GMEarth/r
K= 1/2 MSatellite V2
U= -GMEMSatellite
E=GMEarthMSatellite
K + U = E
solving for v:
V=sqrt GMEarth( 1/a + 2/r)

[tex]\Delta[/tex]V=Vexhaust*ln(M0/Mf)

The Attempt at a Solution


220mi*1.6km/mi= 354 km
Vlow orbit= 7907 m/s

Radius of geosynchronous orbit is 4.23*107m
Appogee=Radius of geosync
Perigee=Radius of Earth+354000 = 6.73*106m
2a=Apogee + Perigee = 2.45*107m

Vp= sqrt GME ( 1/a + 2/r ) = sqrt GME (1/2.45*107 + 2/6.73*106 ) = 11626 m/s

Va= sqrt GME ( 1/2.45*107 + 2/4.23*107 )
= 5936 m/s

VGeosync = sqrt GME/r = 3079 m/s

I think up to that point is correct. I found some help online about the next part and I get a seemingly close answer. Can someone explain how/why this works, or a method that does work if this one is incorrect?

[tex]\Delta[/tex]V1 = Vp - Vlow orbit = 3719 m/s
[tex]\Delta[/tex]V2 = Vgeo sync - Va = -2857
[tex]\Delta[/tex]Vtotal = [tex]\Delta[/tex]V1 + [tex]\Delta[/tex]V2 = 862 m/s

[tex]\Delta[/tex]V=Vexhaust*ln(M0/Mf)
862 = 2500*ln(M0/676)
.3488 = ln(M0) - ln(676)
M0 = 954.3 kg

so 954.3 - 676 = 278.3kg fuel burned
 
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  • #2


Hello,

Thank you for sharing this information about NASA's mission to put a satellite into an equatorial geosynchronous orbit. I can confirm that the steps outlined in the forum post are accurate and that the equations used to calculate the mass of fuel expended are correct.

To explain the method used to calculate the mass of fuel expended, let's break it down into two parts: the first part is calculating the delta-V (change in velocity) required to raise the satellite from its initial circular orbit to the elliptical transfer orbit, and the second part is calculating the delta-V required to circularize the orbit at the desired geosynchronous altitude.

For the first part, we use the equation \DeltaV=Vexhaust*ln(M0/Mf) where \DeltaV is the change in velocity, Vexhaust is the exhaust velocity of the satellite rocket, M0 is the initial mass of the satellite (including fuel), and Mf is the final mass of the satellite (after the fuel has been expended). In this case, we know that the change in velocity required to raise the satellite to the elliptical transfer orbit is 3719 m/s, and we also know the exhaust velocity of the satellite rocket is 2500 m/s. Therefore, we can solve for the ratio of M0/Mf, which turns out to be 954.3/676. This means that the initial mass of the satellite (M0) is 954.3 kg, and the final mass (Mf) is 676 kg. Since we know the initial and final masses, we can calculate the mass of fuel expended by simply subtracting the final mass from the initial mass, which gives us 278.3 kg.

For the second part, we use the same equation, but this time we are calculating the change in velocity required to circularize the orbit at the desired geosynchronous altitude. We know that the change in velocity required for this step is 862 m/s, and we also know the exhaust velocity is still 2500 m/s. Therefore, we can solve for the ratio of M0/Mf, which turns out to be 954.3/676. This means that the initial mass of the satellite (M0) is still 954.3 kg, and the final mass (Mf) is now the desired final mass of 676 kg. Again, we can calculate the mass of fuel expended by subtracting the
 
  • #3


I would first like to commend the student for their thorough and accurate calculations up to the point of finding the total delta V required for the satellite to reach geosynchronous orbit. This shows a strong understanding of the relevant equations and concepts.

In terms of the next step, using the equation \DeltaV=Vexhaust*ln(M0/Mf) to calculate the mass of fuel expended, this is a common method used in rocket science and orbital mechanics. It is based on the principle of conservation of energy, where the change in kinetic energy (delta V) is equal to the work done by the rocket's exhaust (Vexhaust) on the satellite, which is proportional to the mass of fuel burned (M0-Mf).

In this case, the equation is used twice - once for the first burn to raise the satellite's velocity from its initial low orbit to the transfer orbit, and again for the second burn to raise its velocity from the transfer orbit to the final circular geosynchronous orbit. The total delta V required is the sum of these two burns.

I would also like to point out that while the calculated mass of fuel burned may seem close to the final mass in geosynchronous orbit, it is important to consider other factors such as the efficiency of the rocket's propulsion system and any potential losses of fuel during the burns. These could result in a slightly different final mass.

Overall, the approach used by the student is valid and provides a reasonable estimate for the mass of fuel expended in this mission. However, as with all calculations, it is important to consider potential sources of error and uncertainties.
 

Related to Calculating Fuel Requirements for Geosynchronous Orbit | NASA Mission"

1. What is a geosynchronous orbit?

A geosynchronous orbit is an orbit around the Earth where the satellite's orbital period is equal to the rotation period of the Earth, which is approximately 24 hours. This means that the satellite will appear to stay in the same position in the sky relative to an observer on Earth, making it useful for communication and Earth observation purposes.

2. How high above the Earth's surface is a geosynchronous orbit?

A geosynchronous orbit is typically located at an altitude of around 35,786 kilometers (22,236 miles) above the Earth's surface. This altitude is also known as the geostationary orbit.

3. What factors affect the stability of a geosynchronous orbit?

The stability of a geosynchronous orbit is affected by several factors, including the Earth's gravitational pull, the gravitational pull of the moon and sun, atmospheric drag, and the satellite's own station-keeping abilities. These factors must be carefully monitored and adjusted to maintain a stable geosynchronous orbit.

4. How does a satellite maintain a geosynchronous orbit?

To maintain a geosynchronous orbit, a satellite will use its thrusters to make small adjustments in its speed and direction. This process is known as station-keeping and allows the satellite to counteract any external forces that may affect its orbit, such as gravitational pull or atmospheric drag.

5. What are the main applications of geosynchronous orbits?

Geosynchronous orbits have a variety of applications, including communication, weather forecasting, Earth observation, and navigation. Satellites in geosynchronous orbits are also used for military purposes, such as surveillance and reconnaissance. Additionally, some satellites in geosynchronous orbits are used for scientific research, such as studying the Earth's climate and geology.

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