GREENING THE RED PLANET

 

Summary

 

        Man has been in quest of a new home on other planets out of necessities. The moderate climate on Mars and its Earth-like geophysical and geodynamical conditions as well as its proximity in space offer the best choice to set up our homes there . Initially, our homes will be built near the Martian poles that are believed to contain ice water. These homes will be basically designed as greenhouse modules that would provide ideal conditions for humans and plants to thrive. Although a lot of materials have to be initially carried from Earth, in course of time native resources from the planet can be harnessed and used to manufacture our day-to-day materials. This would eventually lead to a sustainable human society in the otherwise barren and desolated planet.

 

Major Highlights

 

·       Mars will be the ready choice in quest of our new homes for its many Earth like conditions and many favourable facors.

·       Human settlements on Mars would be located near its Poles because of easy availability of Water.

·       Human habitats on Mars will be designed into greenhouses for plants and animals to thrive in a sustainable environment.

  

Essay

 

Introduction

         Presently, our Earth has lost its glory caused by environmental degradations due to man’s interference with nature. Summer time temperature inching towards 45 degrees Celsius, worsening air conditions in national capital Delhi due to Smog and air pollutions, havocs of flood in Kerala and ravages of the  tropical cyclone like Fani in Odisha are some of the expressions of nature’s fury. If the present trend continues, a day will come when our beautiful planet will no longer be a habitable place to live on. In that case, we have to migrate to some other planet to settle our colony and propagate our human race.

          From the time life started on Earth, life has always migrated from its usual home to newer worlds of greater scopes.   We have heard about a fish called Eusthenepteron that was swimming in the murky water of the ancient seas some 385 million years ago which was totally a watery world for it. Fierce competition for food and shelter   forced it someday to leave its watery home and crawl onto the land with its muscular fins to discover an entire new world, a world of solids and gases. It took thousands of years for Eusthenepteron to to evolve into the most intelligent life form, the   man and master the land. That man on April 12, 1961 left his realm of solids and gases and flew to space and stayed 108 minutes there.  Life again migrated to a new world out of necessities!

          Since then, space has become the cradle of man and his ultimate destination in quest for   a new home in the event of a catastrophe making life uninhabitable on Earth. Our    nearest goal in this adventure should be obviously the red planet Mars.

Why Mars?

      Although many planets in the habitable zones of stars have been discovered, these are too far away from us to actually go and plan settlements there. The nearest of such  planets is Proxima Centauri b  that orbits  the star Proxima Centauri at nearly  4.3 light years  distance away from us. Kepler telescope has also  discovered many planets orbiting in the habitable zones of distant stars which are even farther away. Moreover, we don’t know much about the geophysical and geodynamical conditions of these planets because of the vast distance and our limitations in observation techniques. It would also be quite difficult for us to initially carry necessary materials to the planet from Earth to build our homes there. Hence, it is highly unlikely to make a voyage to these far-away planets in search of new homes.    

       Mars is singular in that it possesses most of the raw materials required to support not only life, but a new class of human civilization. Mars has elements like Carbon, Nitrogen, Hydrogen and Oxygen, all in biologically readily accessible forms such as Carbon dioxide gas, Nitrogen gas, Water ice and Permafrost.  According to an estimate, if Mars were planes and all its ice and permafrost melted into liquid water, the entire planet would be covered with an ocean up to 100 meters deep. Moreover, on Mars, hydrologic and volcanic processes have occurred in past like Earth that are likely to have consolidated various elements into local concentrations of high grade mineral ore. The geological history of Mars can be best compared to that of Africa with very optimistic inferences on the availability of most of its mineral resources in the red planet.    


        In this backdrop, the planet Mars offers the most convenient place to plan our settlements. With the fastest mode of transport available today, it would take 9 months time to travel to Mars and another 9 months time to return to Earth which is quite tolerable to plan for our annual work schedule. Given the travel time, it will be easier for humans to initially shuttle many times between Mars and the Earth carrying necessary man and materials before we actually settle down finally there. Also, Mars requires less energy per unit mass (delta-v to reach from Earth than any planet other than Venus  It is very important that our settlement in the alien planet is sustainable, as space travel is very expensive to carry each and every material from Earth.

 Mars has several key favorable conditions for supporting life which are outlined below:

It has frozen water trapped at the Poles.
It has a thin atmosphere that contains mostly Carbon dioxide gas which can be utilized for photosynthesis by the plants.

It has a range of temperatures with moderate climatic conditions where a man can thrive.

 Similarities of Mars to Earth

         Although the Earth  is similar to Venus size and surface gravity, Mars similarities to Earth are more compelling when considering conditions for thriving of life. Firstly, the Martian day (or Sol) is very close in duration to an Earth day. A Solar day on Mars is 24 hours, 39 minutes and 35.244 seconds in contrast to Earth which is 24 hours 56 minutes and 4.1 seconds. Second, Mars has a surface area which is 28.4% of Earth, which is slightly less than the amount of total dry land on Earth (which is 29.2% of Earth's surface). Third, Mars has an axial tilt of 25.19° similar to Earth's 23.44°. As a result, Mars undergoes  seasonal cycle much like the  Earth, though an average season on Mars is nearly twice longer than that on Earth because the Martian year is about 1.88 times the  Earth year. Fourth, Mars has an atmosphere which, like our Earth, is a mixture of various gases although the atmosphere is much thinner. Fifth, recent observations by NASA's Mars Reconnaissance Orbiter and Phoenix Lander spacecrafts and ESA's Mars Express spacecraft confirm the presence of water ice on Mars.

     Dissimilarities from Earth

          In spite of these similarities, Mars has many striking dissimilarities from Earth which should be taken care of while planning our settlements there.  First, the surface gravity of Mars  is only 38% that of Earth. Although microgravity is known to cause many health problems like muscle loss and bone demineralization,  it is not known if Martian gravity would have a similar effect on humans. Second, Mars is much colder than Earth with mean surface temperatures varying between −87 °C and −5 °C (depending on position).  The lowest temperature ever recorded on Earth was −89.2 °C in Antarctica. Third, because Mars is about 52% farther from the Sun, the amount of solar energy entering its upper atmosphere per unit area (the Solar Constant) is only around 43.3% of what reaches the Earth's upper atmosphere.  However, due to the much thinner atmosphere, a higher fraction of the solar energy reaches the Mars surface.  The maximum solar irradiance on Mars is about 590 W/m2 as compared to about 1000 W/m2 at the Earth's surface. Fourth, dust storms are common throughout the year and cover the entire planet for weeks, blocking sunlight from reaching the surface.   Fifth, due to the lack of a Magnetosphere, Solar particles   and cosmic rays can easily reach the Martian surface. Sixth, the atmospheric pressure  on Mars is far below the Armstrong limit at which people can survive without pressure suits. Since terraforming  (deliberately changing of the climate by geoengineering to make the planetary conditions suitable for life)  cannot be expected as a near term solution, habitable structures on Mars would need to be constructed with pressure vessels similar to spacecraft capable of maintaining a pressure between 30 and 100 kPa. Seventh, the Martian atmosphere is toxic with 95% Carbon dioxide , 3% Nitrogen, 1.6% Argon and traces of other gases including Oxygen totaling less than 0.4%. Eighth, the thin atmosphere does not cut off ultraviolet radiation coming from the Sun, and hence, life cannot survive in the open. Ninth, due to the thin atmosphere, the temperature difference between day and night times is much longer than on Earth, typically around 70 °C. 

 

Generating Power on Mars

 

       We can generate power on Mars by deploying large solar panels.  But if we wish to manufacture solar panels so as to create a self-sustaining power base, Mars holds an enormous possibility, as only Mars possesses the large supplies of carbon and hydrogen needed to produce pure silicon required for manufacturing photovoltaic panels and other electronic equipments. . As Mars has no rain and virtually no cloud, it is permanently sunny which means solar panels can always operate at maximum efficiency on dust-free days like dust storms.

 

        In addition, Mars has the potential for wind-generated power. But both solar and wind offer relatively modest power potential. However, to create a vibrant civilization, we need a richer power base and, in this respect, Mars has both in the short and medium term opportunities in the form of its geothermal power resources which offer potential for large numbers of locally created electricity generating stations in the 10 MW class. In the long-term, Mars will enjoy a power-rich economy based upon exploitation of its large domestic resources of deuterium fuel for fusion reactors. Deuterium is five times more common on Mars than on Earth and tens of thousands of times more common on Mars than on the Moon.


Greening the Red Planet

 

        The first step to build a home is to choose the location that offers the best chance of survival. For Mars, our first choice would be the planet’s poles which contain ice deposits that have been built up over thousands of years. These deposits are thought to contain large amounts of water ice which could potentially be extracted and turned into liquid water. The poles also harbour other natural resources like Carbon dioxide, Iron, Aluminum, Silicon and Sulfur which could be used to make things like glass, brick and plastic for daily use.


               Our home will be basically designed into a greenhouse which will be useful for raising crops and providing accommodation to farmers.  The greenhouse would produce the necessary warming and an artificial environment for the people to live in.  It is believed that the first visitors to the red planet would be the farmers who would cultivate crops and keep the conditions ready for incoming astronomers.  Because Mars has soil very poor in fertility (especially in organic matter) and extremely low atmospheric pressure (only one-tenth of the Earth’s atmospheric pressure), plants cannot survive in the open, and hence, need an artificial environment like greenhouse.

 

        Satellite or balloon-borne large mirrors can be deployed in the Martian sky to direct solar heat radiations onto the ice-cap to melt ice. Mars atmosphere has been successfully used for aero-braking of spacecrafts and is believed capable of producing enough buoyancy to support large balloons. The liquid water can be delivered through underground pipes into the greenhouse to irrigate crops as well as for human use.

 

             The green-house on Mars may not be inflated to full atmospheric pressure, because maintaining full atmospheric pressure on another planet would be difficult and as plants only need one-tenth of the atmospheric pressure to function. The liquid water will also be split into Oxygen and Hydrogen by electrolytic dissociation using electricity generated from large Photo-voltaic panels deployed outside the greenhouse. While Oxygen will be utilized to provide life support system inside the Green-house (Respiration), Hydrogen will be used as fuel in Fuel cells to provide energy for the operation of the Green-house. Hydrogen can also be used as a domestic fuel for cooking our foods. Carbon dioxide will be sucked into the greenhouse directly from the Mars atmosphere by pumps for producing necessary warming as well as for serving as a raw material for photosynthesis by plants. Since Mars soil is poor in fertility, plants can be initially grown without soil hydroponically in the nutrient medium. As plants grow and decay, they will leave organic matter into the soil gradually enriching the soil with organic matter which will sustain more plants and the cycle will continue. Once sufficient number of plants is established inside the greenhouse, they would give out adequate quantity of Oxygen for humans to breathe in which, in turn, would give enough Carbon dioxide for the plants to make photosynthesis and the cycle would continue. Our Martian greenhouse will be able to raise crops like peas, beans and many fresh vegetables to be used as food for farmers and astronauts.

 

Greenhouse Design

 

    Our greenhouses will be basically dome-shaped and made up of thin-walled inflatable plastic sheets with UV-resistant film lining capable of quick deployment anywhere. Such domes up to 50 meters in diameter are light enough to be transported from Earth initially, and later on, these can be manufactured on Mars itself out of indigenous materials. Because all the resources to make plastic exist on Mars, networks of such 50 to 100 meter domes could be rapidly manufactured and deployed, thus opening up large areas of the surface for both human habitation and agriculture.

        Each dome would consist of three units: a central core, three surrounding capsules and a massive over-arching dome. The central core would stretch 41 feet high and 16 feet in diameter and would house sufficient living space for accommodating the crew. The three capsules surrounding the central core would function as airlocks, passages that connect the core and the Martian surface and minimize changes in air pressure between the two domains. Finally, an enormous polyethylene fiber dome would encapsulate the entire base camp which would serve as a giant radiation shield and help further regulate the air pressure. The antenna for establishing communication with Earth and the rocket launch pad for transportation with Earth should be located outside the green house as frequent dependence on Earth will be necessary during the initial period before our establishment becomes sustainable on the alien planet. 

Conservation is the Key to Survival


          As Mars has limited resources, conserving the resources in our Martian homes will be the key to our survival. We should never allow a single drop of water to go waste as water is very scarce on Mars. The water, after use, can be sent to special recycling plants set up inside our homes where it can be purified to make fit for human use again. Even the water that is used in toilets should not be wasted and, after special treatments, should be used again either for toilet or for watering plants. The channels that would carry water should be meticulously covered so as to prevent loss of water due to evaporation. We should also follow practices of how to save electricity in our Martian homes.  We should use high efficient LED lamps in our homes and switch off different gadgets when not in use.  The waste vegetable matter should not be thrown away, rather be allowed to biodegrade to yield useful elements into the soil for the plants to absorb. Similarly, the decayed plant matter should be allowed composting by burying them in pits which can be later used to increase the fertility of the soil. Even human wastes should be either used to biodegrade for yielding manures or for providing energy by some innovative methods. All our approaches should be eco-friendly and environmentally sustainable.

 

Future Plans

 

     It will eventually be possible for humans to substantially thicken Mars atmosphere by forcing the regolith to outgas its contents through a deliberate program of artificially induced global warming. Once that has been accomplished, the habitation domes could be virtually of any size, as they would not have to sustain a pressure differential between their interior and exterior. In that event, it will be possible for humans to freely roam outside and raise specially bred crops in the open. We may also look forward to take help of other terraforming techniques by which the planet’s environment could be deliberately changed to make conditions suitable for life although it would take a longer period to practically implement it. Once that has been done, our home on Mars will be much safer and smoother and our stay on the alien planet will be enjoyable.

  

Conclusion:

 

      The essay describes some original ideas on how to set up our homes on a new planet taking care of the fact that the entire project is self-sustainable. In this context, I have chosen Mars as my destination due to several favourable factors.




                                                                                        

                                                                                        Nikunja Bihari  Sahu

                                                                                        Regional Science Centre

                                                                                        Bhopal

                                                                                        

 

 

 

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