Astronomy - Hohmann Transfer Orbit

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SUMMARY

The Hohmann Transfer Orbit, established by Wolfgang Hohmann in 1925, is the most efficient trajectory for spacecraft traveling from Earth to Mars. This method requires a spacecraft to escape Earth's gravitational influence, which orbits the Sun at 30 km/s, and then increase its velocity to ensure its aphelion grazes Mars' orbit at 1.524 AU. Key calculations involve determining the minimum and maximum distances from the Sun, the semi-major axis of the orbit, and using Kepler's 3rd law to calculate the orbital period, which provides the time required to reach Mars expressed in months.

PREREQUISITES
  • Understanding of orbital mechanics and Hohmann Transfer Orbits
  • Familiarity with Kepler's 3rd law of planetary motion
  • Basic knowledge of Newtonian physics
  • Ability to perform calculations involving astronomical units (AU)
NEXT STEPS
  • Research the mathematical derivation of Hohmann Transfer Orbits
  • Learn how to calculate orbital periods using Kepler's 3rd law
  • Explore the implications of gravitational assists in space travel
  • Study the dynamics of spacecraft propulsion systems for interplanetary travel
USEFUL FOR

Astronomers, aerospace engineers, students of astrophysics, and anyone interested in the mechanics of interplanetary travel will benefit from this discussion.

GPalm
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The most efficient way to reach Mars from Earth is following the Hohmann Transfer Orbit
(Wolfgang Hohmann, 1925). A spaceship must first get free of Earth (it still orbits the Sun
together with Earth, at 30 km/s, at a distance of 1 AU), then it adds speed so that its aphelion
(in its orbit around the Sun) just grazes the orbit of Mars, A = 1.524 AU (ignoring ellipticity).



(a) Draw the orbits of Earth and Mars, together with the Hohmann Transfer Orbit.


(b) What are the minimum and maximum separation from the Sun? What is the semi-major
axis of this orbit?


(c) Using the Newtonian derivation of Kepler's 3rd law once again, determine the orbital
period, and hence the time taken to reach Mars from Earth. Express your answer in
months.
 
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GPalm said:
The most efficient way to reach Mars from Earth is following the Hohmann Transfer Orbit
(Wolfgang Hohmann, 1925). A spaceship must first get free of Earth (it still orbits the Sun
together with Earth, at 30 km/s, at a distance of 1 AU), then it adds speed so that its aphelion
(in its orbit around the Sun) just grazes the orbit of Mars, A = 1.524 AU (ignoring ellipticity).



(a) Draw the orbits of Earth and Mars, together with the Hohmann Transfer Orbit.


(b) What are the minimum and maximum separation from the Sun? What is the semi-major
axis of this orbit?


(c) Using the Newtonian derivation of Kepler's 3rd law once again, determine the orbital
period, and hence the time taken to reach Mars from Earth. Express your answer in
months.
The posting template is there for a reason. You must show your own thoughts and efforts on the problem so we'll know how to help; no help can be given if you don't show effort.
 

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