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ESA Document - Emits - ESA

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s<br />

HMM<br />

Assessment Study<br />

Report: CDF-20(A)<br />

February 2004<br />

page 53 of 422<br />

duration around Mars, and also the highest ratio, increasing the exploration opportunities. This<br />

opportunity also minimises the time spent in deep space.<br />

The following shows an example of difference in energy requirements for the different dates:<br />

TMI+MOI+TEI max = 8593 m/s in 2037<br />

TMI+MOI+TEI min = 7721 m/s in 2041<br />

Difference = 872 m/s<br />

TMI max = 4005 m/s in 2037<br />

TMI min = 3619 m/s in 2041<br />

Difference = 386 m/s<br />

MOI max = 2613 m/s in 2031<br />

MOI min = 2010 m/s in 2041<br />

Difference = 603 m/s<br />

TEI max = 2595 m/s in 2035<br />

TEI min = 1955 m/s in 2043<br />

Difference = 640 m/s<br />

∆V (m/s)<br />

∆V (m/s)<br />

10000<br />

9000<br />

8000<br />

7000<br />

6000<br />

5000<br />

4000<br />

3000<br />

2000<br />

1000<br />

0<br />

4500<br />

4000<br />

3500<br />

3000<br />

2500<br />

2000<br />

1500<br />

1000<br />

500<br />

0<br />

7892<br />

Mission<br />

2028<br />

Mission<br />

2028<br />

TMI+MOI+TEI<br />

8299 8383 8388 8593<br />

Mission<br />

2031<br />

Mission<br />

2031<br />

Mission<br />

2033<br />

Mission<br />

2033<br />

Mission<br />

2035<br />

Mission<br />

2035<br />

Mission<br />

2037<br />

Mission<br />

2037<br />

8014 7721 7753<br />

Mission<br />

2039<br />

Mission<br />

2039<br />

Figure 2-21: Energy requirements<br />

The difference during the cycle is slight, around 10%. Therefore, any of the trip opportunities is<br />

representative enough for the mission case.<br />

Concerning the entry velocity at Earth arrival the differences are:<br />

V entry max = 12515 m/s in 2028<br />

V entry min = 11472 m/s in 2037<br />

Difference = 1043 m/s<br />

Apollo Entry Velocity = 11200 m/s<br />

Mission<br />

2041<br />

Mission<br />

2041<br />

Mission<br />

2043<br />

TMI<br />

MOI<br />

TEI<br />

Mission<br />

2043

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