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Team:Tokyo Tech/Approaches
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==Approaches== | ==Approaches== | ||
| - | + | As concrete approaches to realize the long-term plan of terra forming, we have five conceivable key components which would play an important role to adapt to and modify Martian environment. Those are 1)Iron-Oxidizing Baceria, 2) Microbial Consortium, 3) Anti-Freezing Protein (AFP), 4) Blackened Bacteria and 5) N2-Generating Bacteria. | |
| + | This year, we Tokyo Tech team focus on all of those components except N2-generating bacteria. | ||
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| + | <a href="https://2009.igem.org/Team:Tokyo_Tech/DarkercoloredEcoli"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/2/23/Tokyo_Tech_5.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/BlackenedEcoli">Blackened <i>E.coli</i></a></h3> | ||
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<td width="300" align="center"> | <td width="300" align="center"> | ||
<a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/2/2c/Tokyo_Tech_3.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria">Iron-oxidizing bacteria</a></h3> | <a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/2/2c/Tokyo_Tech_3.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria">Iron-oxidizing bacteria</a></h3> | ||
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<td width="300" align="center"> | <td width="300" align="center"> | ||
<a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/f/ff/Tokyo_Tech_Terra_Form.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium">Consortium</a></h3> | <a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/f/ff/Tokyo_Tech_Terra_Form.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium">Consortium</a></h3> | ||
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<td width="300" align="center"> | <td width="300" align="center"> | ||
<a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/1/10/Tokyo_Tech_4-2.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze">Antifreeze protein</a></h3> | <a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/1/10/Tokyo_Tech_4-2.gif"></a><h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze">Antifreeze protein</a></h3> | ||
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Latest revision as of 03:58, 22 October 2009
| Main | Team | Terraforming | Experiments | Parts | Safety |
Approaches
As concrete approaches to realize the long-term plan of terra forming, we have five conceivable key components which would play an important role to adapt to and modify Martian environment. Those are 1)Iron-Oxidizing Baceria, 2) Microbial Consortium, 3) Anti-Freezing Protein (AFP), 4) Blackened Bacteria and 5) N2-Generating Bacteria. This year, we Tokyo Tech team focus on all of those components except N2-generating bacteria.
 Blackened E.coli |
 Iron-oxidizing bacteria |
 Consortium |
 Antifreeze protein |
