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Of the remaining sequences, the 1 st , 3 rd , 4 th , <strong>and</strong> 7 th best known solutions from Table 20<br />

all remain in the <strong>design</strong> <strong>space</strong>.<br />

Next, the <strong>global</strong> <strong>optimization</strong> phase is applied to the reduced <strong>design</strong> <strong>space</strong>,<br />

beginning with ranking the remaining asteroid sequences by the normalized sum of the<br />

<strong>pruning</strong> metrics. Due to the GTOC2 objective function, which includes the overall time<br />

of flight, a slight modification was made in the calculation of the optimal two-impulse<br />

solutions, which are used to determine the upper bounds during the branch-<strong>and</strong>-bound<br />

process. When the optimal two-impulse solutions were initially being calculated, it was<br />

discovered that many of the optimal solutions were falling in the very low time of flight<br />

range. As the low-thrust optimal solutions were calculated, it became apparent that most<br />

of the asteroid sequences that yield very good impulsive solutions at low times of flight<br />

do not translate to good low-thrust solutions. While low times of flight are possible <strong>for</strong><br />

impulsive trajectories, low-thrust trajectories generally require longer times of flight to be<br />

feasible. There<strong>for</strong>e, a restriction was placed on the minimum time of flight when<br />

calculating the impulsive solutions. This change was initially made in order to better<br />

model the low-thrust trajectories. However, it also served to reduce the number of lowthrust<br />

<strong>optimization</strong>s that would be required, since the optimal impulsive objective<br />

function <strong>for</strong> many of the asteroid sequences was greatly reduced when applying the time<br />

of flight restriction. For this problem, this minimum allowable time of flight <strong>for</strong> the<br />

impulsive solutions was chosen at 7 years, which was estimated as the minimum realistic<br />

time of flight <strong>for</strong> the low-thrust trajectories. Figure 52 plots the optimal impulsive<br />

solutions <strong>for</strong> the asteroid sequences remaining after the <strong>pruning</strong> phase, with <strong>and</strong> without a<br />

time of flight restriction.<br />

122

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