Team:Brown-Stanford/PowerCell/Background

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(Difference between revisions)
(Photosynthesis on Mars)
(Photosynthesis on Mars)
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Photosynthesis on Earth represents an efficient way of converting solar to chemical energy on a large scale. However, photosynthetic output depends on variables such as atmospheric composition and amount of accessible sunlight. In this section we offer an estimate of the usefulness of photosynthesis on Mars by evaluating several environmental conditions.
Photosynthesis on Earth represents an efficient way of converting solar to chemical energy on a large scale. However, photosynthetic output depends on variables such as atmospheric composition and amount of accessible sunlight. In this section we offer an estimate of the usefulness of photosynthesis on Mars by evaluating several environmental conditions.
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=== '''Atmosphere''' ===
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== '''Atmosphere''' ==
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H2O Content:
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== '''H2O Content''' ==
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Dust particulate in the Martian Atmosphere:
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== '''Dust particulate in the Martian Atmosphere''' ==
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Solar irradiance:
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== '''Solar irradiance''' ==
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Estimating the extent of energy conversion:
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== '''Estimating the extent of energy conversion''' ==
{{:Team:Brown-Stanford/Templates/Foot}}
{{:Team:Brown-Stanford/Templates/Foot}}

Revision as of 16:57, 24 September 2011

Brown-Stanford
iGEM

Photosynthesis on Mars

Photosynthesis on Earth represents an efficient way of converting solar to chemical energy on a large scale. However, photosynthetic output depends on variables such as atmospheric composition and amount of accessible sunlight. In this section we offer an estimate of the usefulness of photosynthesis on Mars by evaluating several environmental conditions.

Atmosphere

H2O Content

Dust particulate in the Martian Atmosphere

Solar irradiance

Estimating the extent of energy conversion