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Phase II Final Report - NASA's Institute for Advanced Concepts

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Chapter 3.0 Vehicle Design<br />

3.6 Power System<br />

The latitude (φ) and Earth's declination angle (δ) vary with the day of the year (d). This day<br />

number (d) is based on the vernal equinox.<br />

δ = δ max sin(2 π d / d t ) Equation 3-64<br />

The hour angle (a) is given by the following expression, where i is the instantaneous time of day<br />

in hours.<br />

a = 2 π i / h l Equation 3-65<br />

SI o = SI om ( r m 2 / r 2 ) Equation 3-66<br />

The distance from the flight planet to the sun (r) varies throughout the year. The planet's orbital<br />

radius is based on the mean radius (r m ) and is represented by Equations 3-67 and 3-68, where the<br />

day number (d p ) is based on the date of perihelion.<br />

r = r m (1 - e 2 ) / (1 + e cos(θ)) Equation 3-67<br />

θ = 2 π d p / d t<br />

Equation 3-68<br />

Based on the equations given above, power-available curves were generated. The curves represent<br />

the available power at different times of the year and different latitudes. Four times of year<br />

were plotted: vernal equinox, summer solstice, autumnal equinox, and winter solstice. These<br />

dates represent the maximum and minimum points <strong>for</strong> the year as well as the times of equal day<br />

and night cycle lengths. Figures 3-173 through 3-177 show the power available on Mars.<br />

60<br />

0° Latitude<br />

50<br />

40<br />

Vernal Equinox (Day 1)<br />

Summer Solsitce (Day 167)<br />

Autimal Equinox (Day 333)<br />

Winter Solstice (Day 500)<br />

30<br />

20<br />

10<br />

0<br />

0 5 10 15 20<br />

Time (hours)<br />

Figure 3-173: Mars: Available Power Throughout the Day at 0 o Latitude<br />

213

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