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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LIGHTHOUSE
LOCATION
The location of choice is the Tharsis region (0° 0‘N, 100°
0’W). Because of its many volcanos and lavatube sunlights
which can already be seen from satellites, it‘s most likely
that there are more lavatubes underground. Furthermore,
volcanic areas are prone to contain ice underground. The
region Tharsis has the highest possibility of finding water in
caves underground. This can help ensure the first human life
on Mars and will also be interesting for research purposes.
Lavatube roofs will be 10-90 meters thick, which is enough
to protect the population from the surface radiation,
galactic cosmic radiation, meteorite bombardment and
extreme temperatures.
It is important to say that lavatubes are not thoroughly
researched, because the procedure of scanning the
underground is quite complicated. While current research
by ESA focuses on scanning lavatubes, our concept also
includes scouting and research on site.
Chloe
Dena
Annie
Wendy
Arsia Mons. Jeanne Cave
Nikki
Abbey
Jeanne
Phase 5
Phase 4
~ 900 people reached
0 2090 2100 2110
expansion,
expansion,
expansion.
city completely self-sustainable
synodic cycle
97
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