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ESA Document - Emits - ESA

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3.3.3.2 Assumptions<br />

HMM<br />

Assessment Study<br />

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

February 2004<br />

page 168 of 422<br />

• Incidental thermal fluxes are the result of the vehicle attitude against the relative location of<br />

the different heat sources (the Sun or a planet). A conservative approach is to consider<br />

envelopes through worst-case scenarios:<br />

• maximization of the absorbed radiative energy (normal incidence) for hot cases,<br />

minimisation of the absorbed radiative energy (maximization of the Sun angle) for the<br />

cold case<br />

• Environmental heat loads values are shown in Table 3-21:<br />

Solar flux [W/m 2 ] Planet albedo Planet IR [W/m 2 ]<br />

Hot case (Earth LEO, WS, 1 AU) 1423 0.33 241<br />

Hot case (Venus swing-by, 0.7 AU) 1 2904 negligible negligible<br />

Hot case (Mars orbit, perihelion, 1.38 AU) 2 717 0.29 (subsolar) 470 (subsolar) to 30<br />

Cold case (Mars orbit, aphelion, 1.66 AU) 3 493 0.29 (subsolar) 315 (subsolar) to 30<br />

Table 3-21: Thermal cases definition<br />

Note that the Venus swing-by is an option. That with respect to Mars arrival and departure dates,<br />

the vehicle passes aphelion and perihelion. That for the hot case with Mars, and cold cases<br />

around Mars depend in a certain extent on the orbit of the spacecraft (and thermal characteristics<br />

of the underneath regions). The worst cold case is sought with long eclipse duration: 500 km<br />

circular orbit and a coplanar Sun (beta 0) give a 13.6 mn eclipse out of a 40.2 mn orbit.<br />

• Thermal design shall manage all internal heat loads resulting from the human activities and<br />

various dissipating equipments:<br />

• Total mean heat load of 12.3kW during LEO<br />

• Heat load turndown ratio of 1.2<br />

• Metabolic dissipation is estimated to be 110W (steady activity) or 295W (active state) per<br />

crew.<br />

3.3.3.3 Baseline thermal design<br />

The design block proposed is based on the exploitation of existing heritage: space stations on one<br />

hand (ISS, Skylab), and visiting/orbiting vehicles on the other hand (STS, Apollo, Soyuz).<br />

Undergoing or foreseen technological developments, and in general non-qualified hardware, are<br />

excluded.<br />

The thermal control philosophy adopted for such vehicle is standard and relies on the following<br />

approach:<br />

• simplification of the heat transfer with maximal use of thermal decoupling when possible<br />

• use of thermal regulated bus to recuperate and transfer internal heat to heat sinks<br />

• use of switch capability to modulate this transfer and balance the heat inputs from the<br />

outputs, and thus maintain temperatures within a certain bandwidth.

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