How Do You Calculate Satellite Travel Times and Orbits?

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SUMMARY

The discussion focuses on calculating satellite travel times and orbits using Kepler's laws. For a satellite traveling from Earth to a newly identified planet at 7.30 AU, the calculated travel time is approximately 4.277 years after correcting the semi-major axis. Additionally, the radius of a GPS satellite's orbit, with a 12-hour period, is determined using the formula T^2=(4*pi^2*r^3)/GM, yielding a radius of 2.6613E7 meters. The calculations emphasize the importance of unit consistency and proper application of Kepler's third law.

PREREQUISITES
  • Understanding of Kepler's laws of planetary motion
  • Familiarity with gravitational equations, specifically T^2=(4*pi^2*r^3)/GM
  • Basic knowledge of astronomical units (AU) and their conversions
  • Ability to manipulate and solve algebraic equations
NEXT STEPS
  • Study Kepler's laws in detail, focusing on their applications in orbital mechanics
  • Learn about gravitational constants and their significance in satellite calculations
  • Explore the concept of semi-major and semi-minor axes in elliptical orbits
  • Investigate the relationship between orbital period and radius for various celestial bodies
USEFUL FOR

Astronomy students, aerospace engineers, and anyone involved in satellite mission planning or orbital mechanics will benefit from this discussion.

haxxorboi
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Homework Statement


A. NASA sends a satellite to another planet by placing the satellite in a Keplerian orbit such that the perihelion is at the radius of the Earth's orbit (1 AU) and the aphelion is at the radius of the planet's orbit. The gravitational effects may be neglected. Suppose a new planet were to appear in a circular orbit of radius 7.30 AU around the Sun. Calculate the time it would take a NASA satellite to travel from Earth to this planet. Express the result in years.

B. A Global Positioning System (GPS) satellite is placed in a high circular orbit around the earth. The period of revolution is 12 hours. Calculate the radius r of the orbit.

Homework Equations


A. Kepler's third law

B. T^2=(4*pi^2*r^3)/GM

The Attempt at a Solution


A.
1^2 yr x^2 yr
------- = --------
1^3 au 7.03^3 au

X would be 18.639 years but this seems to be incorrect.

B. I think T needs to be in seconds as that's what the other units are in. Thus:
43200^2=(4*pi^2*x^3)/(6.674E-11*5.9742E24) Thus, X=2.6613E7 m but again no luck.
Any help on either would be greatly appreciated! Thanks!
 
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"SEMI" -major axis of this orbit is HOW far?

by the way, they only want the trip time OUT, not the entire orbit time.
 
You'll have to bear with me because I'm not too great with these types of problems. I have a problem conceptualizing them or something. Anyways...

I got the satellite-to-planet one. That was really stupid (wasn't halving it at the end and was using 7.3/2 instead of 8.3/2. Final answer came out to be 4.277 AU.

Thank you very much for the help on that one.

Now for the other one which I'm sure I'm just being stupid about again. It seems like it should be really easy with how short it is but I'm just not able to understand what I'm messing up.
 

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