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IS COLONIZATION IN MARS
POSSIBLE?
CONTENTS
 What is Mission: Mars One?
 Difference from Earth
 Transportation and landing
 Equipments for colonization
 Possible locations for settlement
 Robotic Precursors and early Human
settlement
 Economy
What is Mission: Mars One?
Mars One is a non-profit organisation based in Netherland that plans to establish a
permanent human colony on Mars by 2025. The private spaceflight project is led
by Dutch entrepreneur Bas Lansdorp, who announced plans for the Mars One project in
May 2012.
Mars One's original concept included launching a robotic Lander and Orbiter as early as
2016 to be followed by a human crew of four in 2022.
According to their April 2013 schedule, the first crew of four astronauts would arrive on
Mars in 2025, after a seven-month journey from Earth. Additional teams would join the
settlement every two years, with the intention that by 2033 there would be over twenty
people living and working on Mars. The astronaut selection process began on 22 April
2013.
Mars is the focus of much speculation and scientific study about possible human
colonization. Its surface conditions and the likely availability of water make it arguably
the most hospitable of the planets, other than Earth.
Difference from Earth
EARTH
 1 solar day= 23 hours 56 minutes 4.0196
seconds
 Surface Area= S
 Radius= R
 Mass= M
 Axial tilt= 23.44˚
 1 revolution period= 365 days
 Average distance from Sun= 93 million
miles
 North pole facing Ursa Minor
 Surface gravity= g
 Mean Surface temperature= 15˚C
 Atmospheric Pressure= 1013 millibars
 Density of atmosphere= d
 Percentage of O2 = 21%
 Percentage of CO2 = 0.04%
MARS
 1 solar day= 24 hours 39 minutes 35.244
seconds
 Surface Area= 0.28S
 Radius= 0.5R
 Mass= 0.1M
 Axial tilt= 25.12˚
 1 revolution period= 686 days
 Average distance from Sun= 142 million
miles
 North pole facing Cygnus
 Surface gravity= 0.38g
 Mean Surface temperature=
-81˚C
 Atmospheric Pressure= 6 millibars
 Density of atmosphere= 0.006d
 Percentage of O2 = ~0.04%
 Percentage of CO2 = 95%
Transportation and landing
Mars requires less energy per unit mass (delta V) to reach from Earth than any planet except Venus.
Modified transfer trajectories that cut the travel time down to seven or six months in space are possible
with incrementally higher amounts of energy and fuel compared to a Hohmann transfer orbit.
Shortening the travel time below six months requires higher delta V and an exponentially increasing
amount of fuel. It might be feasible with advanced spacecraft propulsion technologies, some of which
have already been tested such as VASIMR, and nuclear rockets. In the former case, a trip time of 40
days could be attainable, and in the latter, a trip time down to about 2 weeks.
The effect of long term travel in interplanetary space is unknown, but scientists estimate an added risk
of 3.4% for men to die of cancer because of the radiation during the journey to Mars and back to Earth.
For women the probability is higher due to their larger glandular tissues.
Landing piloted missions on Mars will require braking and landing systems different from anything
used to land crewed spacecraft on the Moon or robotic missions on Mars. So if one assumes carbon
nano-tube construction material will be available with a strength of 130 GPa then a space
elevator could be built to land people and material on Mars.
Equipments for colonization
Types of equipments: To directly provide services to humans and to produce food,
propellant, water, energy and breathable oxygen (production equipments). Required
equipment will include:
 Habitats
 Storage facilities
 Shop workspaces
Resource extraction equipment, initially for water and
oxygen, later for a wider cross section of minerals,
building materials, etc.
 Energy production and storage equipment,
some solar and perhaps other forms
 Food production spaces and equipment
 Propellant production equipment, generally thought to be hydrogen and methane for fuel, with
oxygen oxidizer for chemical rocket engines.
 Fuels or other energy source for surface transportation. CO/O2 engines have been suggested for
early surface transportation use as both CO and O2 can be straight forwardly produced
by zirconia electrolysis from the Martian atmosphere
 Communications with Earth are relatively straightforward during the half-sol when Earth is above
the Martian horizon. NASA and ESA included communications relay equipment in several of the
Mars orbiters, so Mars already has communications satellites.
 The one-way communication delay due to the speed of light ranges from about 3 minutes at closest
approach (approximated by perihelion of Mars minus aphelion of Earth) to 22 minutes at the largest
possible superior conjunction (approximated by aphelion of Mars plus aphelion of Earth).
 Real-time communication is not possible.
 NASA has found that direct communication can be blocked for about 2 weeks every synodic period,
around the time of superior conjunction when the Sun is directly between Mars and Earth.
 A satellite at the L4 or L5 Earth–Sun Lagrangian point could serve as a relay during this period to
solve the problem but it itself has some problems too.
Possible locations for settlement
 Polar regions once attracted as great interest because seasonally-varying polar ice caps but lower
latitudes too showed availability of water. So less compelling.
 In equatorial region, Mars Odyssey found natural caves near the volcano Arsia Mons. It could
provide as a shelter to protect settlers from radiation and micrometeoroids. Geothermal energy is also
suspected in the equatorial regions.
 Valles Marineris, the "Grand Canyon" of Mars, is over 3,000 km long and averages 8 km deep.
Atmospheric pressure at the bottom would be some 25% higher than the surface average, 0.9 kPa vs
0.7 kPa. River channels lead to the canyon, indicating it was once flooded.
 Several lava tube on Mars have been located on the flanks of Arsia Mons. Earth based examples
indicate that some should have lengthy passages offering complete protection from radiation and be
relatively easy to seal using on-site materials, especially in small subsections.
 Landers like Phoenix, the Mars Exploration Rovers Spirit and Opportunity, and the Mars Science
Laboratory Rover Curiosity have encountered very different soil and rock characteristics. This
suggests that the Martian landscape is quite varied and the ideal location for a settlement would be
better determined when more data becomes available.
Robotic Precursors and early Human
settlement
Robotics systems could help locate resources, such as ground water or ice, that would help a colony
grow and thrive. The lifetimes of these systems would be measured in years and even decades, have a
reduced cost compared with early crewed operations, and have less political risk.
Wired systems might lay the groundwork for early crewed landings and bases.
Establishing power, communications, shelter, heating, and manufacturing basics can begin with
robotic systems, if only as a prelude to crewed operations.
Mars Surveyor 2001 Lander (Mars ISPP Precursor) was to demonstrate manufacture of oxygen
from the atmosphere of Mars, and test solar cell technologies and methods of mitigating the effect
of Martian dust on the power systems.
Before any people are transported to Mars in the 2030s, Mars Colonial Transporter envisioned
by SpaceX, a number of robotic cargo missions would be undertaken first in order to transport the
requisite equipment, habitats and supplies. Equipment that would be necessary would include
machines to produce fertilizer, CH4 and O2 from Mars' atmospheric N2 and CO2 and the planet's
subsurface water ice as well as construction materials to build transparent domes for initial
agricultural areas.
Economy
Economics would be a crucial aspect to a colony's success. The reduced gravity well of Mars and its position
in the Solar System may facilitate Mars–Earth trade and may provide an economic rationale for continued
settlement of the planet. A major economic problem is the enormous up-front investment required to establish
the colony and perhaps also terra-form the planet.
With a published price of US$56.5 million per launch of up to 13,150 kg (28,990 lb) payload to low Earth
orbit, SpaceX Falcon 9 rockets are already the "cheapest in the industry". Use of the SpaceX reusable
launch system development program. SpaceX' reusable plans include Falcon Heavy and future methane-
based launch vehicles including the Mars Colonial Transporter.
Alternative funding approaches might include
the creation of inducement prizes. For
example, the 2004, President's Commission
on Implementation of United States Space
Exploration Policy suggested that an
inducement prize contest should be established
for the achievement of space colonization.
THANK YOU

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Mars one - Colonization in Mars

  • 1. IS COLONIZATION IN MARS POSSIBLE?
  • 2. CONTENTS  What is Mission: Mars One?  Difference from Earth  Transportation and landing  Equipments for colonization  Possible locations for settlement  Robotic Precursors and early Human settlement  Economy
  • 3.
  • 4. What is Mission: Mars One? Mars One is a non-profit organisation based in Netherland that plans to establish a permanent human colony on Mars by 2025. The private spaceflight project is led by Dutch entrepreneur Bas Lansdorp, who announced plans for the Mars One project in May 2012. Mars One's original concept included launching a robotic Lander and Orbiter as early as 2016 to be followed by a human crew of four in 2022. According to their April 2013 schedule, the first crew of four astronauts would arrive on Mars in 2025, after a seven-month journey from Earth. Additional teams would join the settlement every two years, with the intention that by 2033 there would be over twenty people living and working on Mars. The astronaut selection process began on 22 April 2013. Mars is the focus of much speculation and scientific study about possible human colonization. Its surface conditions and the likely availability of water make it arguably the most hospitable of the planets, other than Earth.
  • 5. Difference from Earth EARTH  1 solar day= 23 hours 56 minutes 4.0196 seconds  Surface Area= S  Radius= R  Mass= M  Axial tilt= 23.44˚  1 revolution period= 365 days  Average distance from Sun= 93 million miles  North pole facing Ursa Minor  Surface gravity= g  Mean Surface temperature= 15˚C  Atmospheric Pressure= 1013 millibars  Density of atmosphere= d  Percentage of O2 = 21%  Percentage of CO2 = 0.04% MARS  1 solar day= 24 hours 39 minutes 35.244 seconds  Surface Area= 0.28S  Radius= 0.5R  Mass= 0.1M  Axial tilt= 25.12˚  1 revolution period= 686 days  Average distance from Sun= 142 million miles  North pole facing Cygnus  Surface gravity= 0.38g  Mean Surface temperature= -81˚C  Atmospheric Pressure= 6 millibars  Density of atmosphere= 0.006d  Percentage of O2 = ~0.04%  Percentage of CO2 = 95%
  • 6. Transportation and landing Mars requires less energy per unit mass (delta V) to reach from Earth than any planet except Venus. Modified transfer trajectories that cut the travel time down to seven or six months in space are possible with incrementally higher amounts of energy and fuel compared to a Hohmann transfer orbit. Shortening the travel time below six months requires higher delta V and an exponentially increasing amount of fuel. It might be feasible with advanced spacecraft propulsion technologies, some of which have already been tested such as VASIMR, and nuclear rockets. In the former case, a trip time of 40 days could be attainable, and in the latter, a trip time down to about 2 weeks. The effect of long term travel in interplanetary space is unknown, but scientists estimate an added risk of 3.4% for men to die of cancer because of the radiation during the journey to Mars and back to Earth. For women the probability is higher due to their larger glandular tissues. Landing piloted missions on Mars will require braking and landing systems different from anything used to land crewed spacecraft on the Moon or robotic missions on Mars. So if one assumes carbon nano-tube construction material will be available with a strength of 130 GPa then a space elevator could be built to land people and material on Mars.
  • 7. Equipments for colonization Types of equipments: To directly provide services to humans and to produce food, propellant, water, energy and breathable oxygen (production equipments). Required equipment will include:  Habitats  Storage facilities  Shop workspaces Resource extraction equipment, initially for water and oxygen, later for a wider cross section of minerals, building materials, etc.  Energy production and storage equipment, some solar and perhaps other forms  Food production spaces and equipment  Propellant production equipment, generally thought to be hydrogen and methane for fuel, with oxygen oxidizer for chemical rocket engines.
  • 8.  Fuels or other energy source for surface transportation. CO/O2 engines have been suggested for early surface transportation use as both CO and O2 can be straight forwardly produced by zirconia electrolysis from the Martian atmosphere  Communications with Earth are relatively straightforward during the half-sol when Earth is above the Martian horizon. NASA and ESA included communications relay equipment in several of the Mars orbiters, so Mars already has communications satellites.  The one-way communication delay due to the speed of light ranges from about 3 minutes at closest approach (approximated by perihelion of Mars minus aphelion of Earth) to 22 minutes at the largest possible superior conjunction (approximated by aphelion of Mars plus aphelion of Earth).  Real-time communication is not possible.  NASA has found that direct communication can be blocked for about 2 weeks every synodic period, around the time of superior conjunction when the Sun is directly between Mars and Earth.  A satellite at the L4 or L5 Earth–Sun Lagrangian point could serve as a relay during this period to solve the problem but it itself has some problems too.
  • 9. Possible locations for settlement  Polar regions once attracted as great interest because seasonally-varying polar ice caps but lower latitudes too showed availability of water. So less compelling.  In equatorial region, Mars Odyssey found natural caves near the volcano Arsia Mons. It could provide as a shelter to protect settlers from radiation and micrometeoroids. Geothermal energy is also suspected in the equatorial regions.  Valles Marineris, the "Grand Canyon" of Mars, is over 3,000 km long and averages 8 km deep. Atmospheric pressure at the bottom would be some 25% higher than the surface average, 0.9 kPa vs 0.7 kPa. River channels lead to the canyon, indicating it was once flooded.  Several lava tube on Mars have been located on the flanks of Arsia Mons. Earth based examples indicate that some should have lengthy passages offering complete protection from radiation and be relatively easy to seal using on-site materials, especially in small subsections.  Landers like Phoenix, the Mars Exploration Rovers Spirit and Opportunity, and the Mars Science Laboratory Rover Curiosity have encountered very different soil and rock characteristics. This suggests that the Martian landscape is quite varied and the ideal location for a settlement would be better determined when more data becomes available.
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  • 11. Robotic Precursors and early Human settlement Robotics systems could help locate resources, such as ground water or ice, that would help a colony grow and thrive. The lifetimes of these systems would be measured in years and even decades, have a reduced cost compared with early crewed operations, and have less political risk. Wired systems might lay the groundwork for early crewed landings and bases. Establishing power, communications, shelter, heating, and manufacturing basics can begin with robotic systems, if only as a prelude to crewed operations. Mars Surveyor 2001 Lander (Mars ISPP Precursor) was to demonstrate manufacture of oxygen from the atmosphere of Mars, and test solar cell technologies and methods of mitigating the effect of Martian dust on the power systems. Before any people are transported to Mars in the 2030s, Mars Colonial Transporter envisioned by SpaceX, a number of robotic cargo missions would be undertaken first in order to transport the requisite equipment, habitats and supplies. Equipment that would be necessary would include machines to produce fertilizer, CH4 and O2 from Mars' atmospheric N2 and CO2 and the planet's subsurface water ice as well as construction materials to build transparent domes for initial agricultural areas.
  • 12. Economy Economics would be a crucial aspect to a colony's success. The reduced gravity well of Mars and its position in the Solar System may facilitate Mars–Earth trade and may provide an economic rationale for continued settlement of the planet. A major economic problem is the enormous up-front investment required to establish the colony and perhaps also terra-form the planet. With a published price of US$56.5 million per launch of up to 13,150 kg (28,990 lb) payload to low Earth orbit, SpaceX Falcon 9 rockets are already the "cheapest in the industry". Use of the SpaceX reusable launch system development program. SpaceX' reusable plans include Falcon Heavy and future methane- based launch vehicles including the Mars Colonial Transporter. Alternative funding approaches might include the creation of inducement prizes. For example, the 2004, President's Commission on Implementation of United States Space Exploration Policy suggested that an inducement prize contest should be established for the achievement of space colonization.