Problem 5.155
One option when traveling to Mars from the Earth is to use a Hohmann transfer
orbit like that described in Probs. 5.148–5.152. Assuming that the Sun is the
primary gravitational influence and ignoring the gravitational influence of
Earth and Mars (since the Sun accounts for 99.8% of the mass of the solar
system), determine the change in speed required at the Earth
ve
(perihelion
in the transfer orbit) and the required change in speed at Mars
vm
(aphelion
in the transfer orbit) to accomplish the mission to Mars using a Hohmann
transfer. In addition, determine the amount of time
⌧
it would take for orbital
transfer. Use
1:989⇥1030 kg
for the mass of the Sun, assume that the orbits
of Earth and Mars are circular, and assume that the changes in speed are
impulsive, that is, they occur instantaneously. In addition, use
150⇥106km
for the radius of Earth’s orbit and
228⇥106km
for the radius of Mars’s orbit.
Solution
We start with determining the circular orbit speed (see Eq. (5.82) on p. 388 of the textbook) and the elliptical
orbit speed (see Eq. (5.105) on p. 391 of the textbook) at aphelion corresponding to a distance from the Sun
Finally, we determine the time needed for the orbital transfer. This time is half of the full elliptical orbit
period. Hence, using Eq. (5.97) on p. 390 of the textbook, we have
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