Mars Science City – Space Architecture Design Studio 2020
The Mars Science City design studio topic fits into the long-term vision to build a human settlement on Mars. The students were first asked to look far into the future and imagine what a city on Mars would be like. How do they think people would live in about 100 years on another planet? What would they take with them from Earth, and what would they want to see totally different? The student teams have developed a conceptual vision of this city. In parallel they researched and worked on the environmental, technical and social challenges of getting to and being on Mars. Each team was asked to identify three major challenges and / or characteristics, based on their vision. What would be needed to start the settlement in order to become the city they have imagined? This was the most challenging part for the student’s teams, and became the starting point for the individual architectural solutions of the near-term project on Mars. Design Task S. 6 Teaching Team S. 16 The Students S. 24 Projects DUNE S. 30 Moving Mars S. 42 Terra Mars S. 54 AB-ORIGO S. 66 Protocity S. 76 Dune Haranea S. 86 Lighthouse S. 94 Arcadia City S. 104 Apoikia S. 114 Adventus S. 122 Ice Age S. 138 Teaching Team: Sandra Häuplik-Meusburger (Studio Director), Alexander S., Bannova O., Bier H., Bishop S., Ciardullo C., Esfand M., Farmwald L., Frischauf N., Gourlis B., Grömer G., Kahr F., Lamborelle O., Makaya A., Nixon D., Perino M., Russ C., Schechtner K., Schwehm G., Wong D.; Students: Binder D., Brajic A., Gojkovic B., Brückler A., Hamzic E., Kaprinayova E., Stauber B., Vorraber J., Podwalski K., Adnan M., Trinca E., Ahr S., Bula M., Ivanonva M., Stoyanova S., Graf J., Kugic A., Neumerkel R., Vecerdi M., Glinac M., Ramovic A., Schneider G., Ajdari S., Mujedini X., Gündar J.
The Mars Science City design studio topic fits into the long-term vision to build a human settlement on Mars. The students were first asked to look far into the future and imagine what a city on Mars would be like. How do they think people would live in about 100 years on another planet? What would they take with them from Earth, and what would they want to see totally different? The student teams have developed a conceptual vision of this city. In parallel they researched and worked on the environmental, technical and social challenges of getting to and being on Mars. Each team was asked to identify three major challenges and / or characteristics, based on their vision. What would be needed to start the settlement in order to become the city they have imagined? This was the most challenging part for the student’s teams, and became the starting point for the individual architectural solutions of the near-term project on Mars.
Design Task S. 6
Teaching Team S. 16
The Students S. 24
Projects
DUNE S. 30
Moving Mars S. 42
Terra Mars S. 54
AB-ORIGO S. 66
Protocity S. 76
Dune Haranea S. 86
Lighthouse S. 94
Arcadia City S. 104
Apoikia S. 114
Adventus S. 122
Ice Age S. 138
Teaching Team: Sandra Häuplik-Meusburger (Studio Director), Alexander S., Bannova O., Bier H., Bishop S., Ciardullo C., Esfand M., Farmwald L., Frischauf N., Gourlis B., Grömer G., Kahr F., Lamborelle O., Makaya A., Nixon D., Perino M., Russ C., Schechtner K., Schwehm G., Wong D.;
Students: Binder D., Brajic A., Gojkovic B., Brückler A., Hamzic E., Kaprinayova E., Stauber B., Vorraber J., Podwalski K., Adnan M., Trinca E., Ahr S., Bula M., Ivanonva M., Stoyanova S., Graf J., Kugic A., Neumerkel R., Vecerdi M., Glinac M., Ramovic A., Schneider G., Ajdari S., Mujedini X., Gündar J.
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kilometers
DUNE
0 3 6 12 18
Nili Paterae
8.9N, 67E
70km diameter
Elevation 100m
Barchan Dunes
LOCATION
ation, easier access to light and a thinner and faster structure.
It should be possible to manufacture high density polyethylene
polymers on Mars using carbon dioxide from the atmosphere
and hydrogen from water in the soil. With 3D printing technology
we will be able to build a structure that minimizes construction
and maximizes light and space. Dune can begin as a small
infrastructure or gradually grow to house an entire Martian city.
The concept relies heavily on the natural characteristics of
the Martian surface. Nili Patera Dune Field complements
our concept of imitating sand dunes and using the deposition
of Martian Regolith on top of our habitat as protection
from the Galactic Cosmic Rays and other radiation.
The location consists of Barchant Dunes that are found within a crater
in Nili Patera. The dunes lie on top of solidified lava beds which
indicate a location with rich minerals such as basalt rocks and molten
silver. The soil is also reliable for food production as impact glass
has been found beneath the surface. The location is also abundant
with water , about 4% in mass in the first meter of ground is water.
The Barchant Dunes are a result of one-directional wind due to
which sand accumulates and forms dunes. The Aerodynamic
shape of the dunes allows for wind to naturally flow and for
soil to deposit; this would be the core of our design concept.
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