Team:Tokyo Tech/Ibuki test

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==Introduction==
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<div align=center>
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Modifying planet’s environment (※1) to more habitable one for human beings on earth.
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<img src="https://static.igem.org/mediawiki/2009/8/89/Tokyotech.png" height="200">
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Mars is the most earth-like of all the other planets in our solar system.  
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<img src="https://static.igem.org/mediawiki/2009/b/bc/IGEM-1-1.jpg" height="200">
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</div>
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In long term,
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*1. Start Point of Terra Forming.
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*2. Microorganisms I (for adaptation).
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*3. Microorganisms II (for habitat manipulation).
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*4. Cyanobacteria / Plants.
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*5. Animals,
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*6. Human Beings
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<ul id="Tokyo_Tech_menu">
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In short term or in those steps, our approach is shown below.
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<li class="menu" onmouseover="this.className='menuOn'" onmouseout="this.className='menu'">
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*Heat Energy Injection.
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<a href="https://2009.igem.org/Team:Tokyo_Tech">Main</a>
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*Heat Energy Production.
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<ul></ul></li>
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*Atmosphere Generation.
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*Organic Matters Accumulation.
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*Water Accumulation.
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(Introduction/ideas/story about terraforming)
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<li class="menu" onmouseover="this.className='menuOn'" onmouseout="this.className='menu'">
 
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Team">Team</a>
 
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<ul></ul></li>
 
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<li class="menu" onmouseover="this.className='menuOn'" onmouseout="this.className='menu'">
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==Approaches==
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Project">Project</a>
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Actually we have four ideas to terraform the Mars.
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  <ul>
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  (Overlook of the four ideas)
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing">Iron-oxidizing bacteria</a></li>
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[[Image:Tokyo_Tech_3.jpg|150px|link=Team:Tokyo_Tech/Iron-oxidizing_bacteria]]
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium">Microbial consortium</a></li>
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[[Image:Tokyo_Tech_2.jpg|150px|link=Team:Tokyo_Tech/Consortium]]
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze">Antifreeze protein</a></li>
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[[Image:Tokyo_Tech_4-2.jpg|150px|link=Team:Tokyo_Tech/Antifreeze]]
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Idea4">Idea 4</a></li>
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[[Image:Tokyo_Tech_5.jpg|150px|link=Team:Tokyo_Tech/DarkercoloredEcoli]]
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Idea5">Idea 5</a></li>
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<body>
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<ul></ul></li>
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<h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria">Iron-oxidizing　bacteria</a></h3>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing_bacteria"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/e/e2/Tokyo_Tech_3.jpg"></a>
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<li class="menu" onmouseover="this.className='menuOn'" onmouseout="this.className='menu'">
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<h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium">Consortium</a></h3>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Conclusion">Conclusion</a>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/1/1f/Tokyo_Tech_2.jpg"></a>
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<ul></ul></li>
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<li class="menu" onmouseover="this.className='menuOn'" onmouseout="this.className='menu'">
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<h3><a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze">Antifreeze protein</a></h3>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Links">Links</a>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze"><img width="150" height="150" src="https://static.igem.org/mediawiki/2009/0/0c/Tokyo_Tech_4-2.jpg"></a>
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<ul></ul></li>
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<h3><a href="https://2009.igem.org/Team:Tokyo_Tech/DarkercoloredEcoli">Darker colored E.coli</a></h3>
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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/e/ea/Tokyo_Tech_5.jpg"></a>
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</ul>
 
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(Abstract/link of each idea)
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*アルベドと温度の関係について
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According to　Stefan-Boltzmann law,
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blackbody emit per surface in unit time is calculated as
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<!--<math>\sigma T^4</math>,-->
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&sigma;<i>T</i><sup>4</sup>,
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where T is the temperature of the black body and <math>\sigma=5.67*10^{-8} (W/m^2K^4)</math> is constant value.
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The total energy that comes from the sun is calculated as
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<!--<math>S(1-A)\pi r^2</math>,-->
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<i>S</i>(1 &minus; <i>A</i>)&pi;<i>r</i><sup>2</sup>,
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where <math>S=597 (W/m^2)</math>is the energy which actually reaches the mars from the sun,
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A is the albedo of the Mars and <math>r=3.3972*10^6 (m)</math> is the radius of the Mars.
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Regarding the Mars as blackbody, the radiative equilibrium temperature of the Mars is estimated as
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<math>T=\sqrt[4]{\frac{S(1-A)}{4\lambda}}</math>.
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According to Yurij Shkuratov and Larissa Starukhina, albedo A can be calculated as
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<math>A=\frac{1+\rho_b^2-\rho_f^2}{2\rho_b}-\sqrt{(\frac{1+\rho_b^2-\rho_f^2}{2\rho_b})^2-1}</math>,
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where <math>\rho_b</math> and <math>\rho_f</math> are the one-dimensional indicatrix back and forward.
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If we succeeded in decreasing the albedo by making the Mars black,
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the temperature will change as the graph shows.
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x axis is year and y axis is temperature.
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[[File:Temp.png|300px|thumb|temperature estimation]]
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If we could change the albedo from 0.15 to 0.05, the temperature of the Mars would increase by about 6 Celsius degree.
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==Related works==
 +
(write down some related works)

Revision as of 18:19, 19 October 2009

Tokyo Tech toplogo.png
Main Team Terraforming Experiments Parts Safety

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.

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

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. 

(Overlook of the four ideas)

Tokyo Tech 3.jpg Tokyo Tech 2.jpg Tokyo Tech 4-2.jpg Tokyo Tech 5.jpg 

(Abstract/link of each idea)

Related works

(write down some related works)
Retrieved from "http://2009.igem.org/Team:Tokyo_Tech/Ibuki_test"