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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DUNE HARENAE
LOCATION
The structure is located in one of Hellas Planitia lava
The tubes. structure Hellas Planitia is located is in a vast one of plain Hellas within Planitia a circular lava
tubes. impact Hellas basin, Planitia located is on a the vast southern plain within hemisphere. a circular
impact basin, located on the southern hemisphere.
LANDING - Its
LANDING - Its flat surface makes it ideal for landing
WATER - There are glaciers of water ice lying
WATER - There are glaciers of water ice lying
beneath beneath
the the
surface, surface,
making making
it it
one one
of of
the the
„wettest“
„wettest“
places of of Mars. Mars. Also, Also, the the atmospheric atmospheric pressure pressure is
is
situated above the the triple triple point point of of water, water, suggesting
suggesting
that the liquid phase of water could be present under
certain conditions of of temperature, pressure, pressure, and
and
dissolved salt content.
RADIATION - Because the basin is is 7km 7km deep, deep, 50%
50%
less radiation reaches the the basin basin floor o than it would at a
higher elevation elevation regions regions of Mars. of Mars.
PROTECTION - Lava tubes southwest to Hadriacus
PROTECTION Lava tubes southwest to Hadriacus
Mons could reduce the radiation exposure down to
61.64 Mons
usv/ could
day reduce
while also the radiation
providing exposure
extra protection
down to
from 61.64 regolith’s usv/ day perchlorates, while also providing extreme temperature
extra protection
fluctuations from regolith’s and from perchlorates, micrometeorites.
extreme temperature
-36.961°87.841°E - - Candidate lava tube in in Hellas Planitia
COMPLEX OF DUNES
2085
100
VILLAGE
bring nothing
89
SEducationalVersion
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