Team:Tokyo Tech/Project

From 2009.igem.org

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|[[Image:Tokyo_Tech_Intro_Mars.gif|200px|thumb|Mars]]
|[[Image:Tokyo_Tech_Intro_Mars.gif|200px|thumb|Mars]]
|[[Image:Tokyo_Tech_Intro_Surface.gif|200px|thumb|Water on Mars]]
|[[Image:Tokyo_Tech_Intro_Surface.gif|200px|thumb|Water on Mars]]
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|}
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{|style="color:black;text-align:center;font-size:small;position:relative;table-layout:fixed;" border="1"
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|-
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|
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|Earth
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|Mars
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|-
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|Atmosphere
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|N<sub>2</sub>(78%)
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O<sub>2</sub>(20%)
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|CO<sub>2</sub>(95%)
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N<sub>2</sub>(2%)
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|-
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|Pressure at Surface [atm]
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|1
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|0.007
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|-
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|Temperature at Surface [K]
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|280 ± 20
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|180 ± 30
|}
|}

Revision as of 12:43, 20 October 2009

Tokyo Tech toplogo.png
Main Team Terraforming Experiments [http://partsregistry.org/cgi/partsdb/pgroup.cgi?pgroup=iGEM2009&group=Tokyo_Tech Parts] Safety


Contents

Introduction

Modifying planet’s environment (※1) to more habitable one for human beings on earth. Mars is the most earth-like of all the other planets in our solar system.

Mars
Water on Mars
Earth Mars
Atmosphere N2(78%)

O2(20%)

CO2(95%)

N2(2%)

Pressure at Surface [atm] 1 0.007
Temperature at Surface [K] 280 ± 20 180 ± 30
Long term

In long term,

  • 1. Start Point of Terra Forming.
  • 2. Microorganisms I (for adaptation).
  • 3. Microorganisms II (for habitat manipulation).
  • 4. Cyanobacteria / Plants.
  • 5. Animals,
  • 6. Human Beings


Short term

In short term or in those steps, our approach is shown below.

  • Heat Energy Injection.
  • Heat Energy Production.
  • Atmosphere Generation.
  • Organic Matters Accumulation.
  • Water Accumulation. 


(Introduction/ideas/story about terraforming)


Approaches

Actually we have four ideas to terraform the Mars.


Iron-oxidizing　bacteria

Consortium

Antifreeze protein

Darker colored E.coli

Cph

(Abstract/link of each idea)

Related works

(write down some related works)
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