06.02.2013 Views

ESA Document - Emits - ESA

ESA Document - Emits - ESA

ESA Document - Emits - ESA

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

s<br />

Figure 4-54: Solar irradiance on the Martian surface during one Martian year<br />

Figure 4-55: Periods for which landing cannot be performed based on solar-cell design<br />

HMM<br />

Assessment Study<br />

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

February 2004<br />

page 307 of 422<br />

For the designs without solar cells, this operations limitation simply disappears.<br />

For example, the design based on primary fuel cells is not dependent the landing date nor the<br />

latitude of the landing site.<br />

4.3.5.5.2 Fuel storage for FC<br />

Hydrogen and oxygen can be stored either in gaseous or in liquid form.<br />

For the gaseous forms, high-pressure storage is necessary to limit the volume, especially for the<br />

hydrogen that has a low density. Therefore, hydrogen is assumed to be stored at 700 bars.<br />

The storage in a liquid state without losses due to boil-off can only be performed by cooling the<br />

tanks to 20° K for H2 and 90° K for O2. Therefore, the corresponding power requested for this<br />

thermal regulation has permanently to be supplied by the TV until the separation of the MEV.<br />

On the Martian surface itself, with the tanks protected by the structure, the boil-off has been<br />

estimated only around 1% per month. Consequently, the cooling of the tanks doesn’t need to be<br />

continued during this phase.<br />

4.3.5.5.3 PCDU<br />

At this stage of definition, the power conditioning and distribution has not been analysed in<br />

details. Indeed, this module is not as critical as the power generation and storage modules for all<br />

aspects: mass, volume, technology, cost.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!