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The Great Leap Out of the Cradle: The Human Exploration of Our Solar System

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Abstract

Moving human space exploration beyond the Moon is the next challenge. Mars, the most Earth-like planet in the solar system, is the next target. Table 4.1 summarises the main physical characteristics of the Earth and Mars.

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Notes

  1. 1.

    The pressure at the ground is less than one-hundredth of the atmospheric pressure on Earth and has much variability with altitude and latitude. It varies from around 0.3 millibars on Olympus Mons to over 11.6 millibars in the depths of Hellas Planitia. It has a mean surface level pressure of 6.36 millibars, ranging from 4.0 to 8.7 millibars depending on the season.

  2. 2.

    Mission proposals include among others: (i) Project Empire, a study commissioned by the Marshal Space Flight Center and awarded to General Dynamics and Lockheed (1959); (ii) von Braun’s Mars Project (1969); (iii) The Martian Expeditionary Complex of the Soviet Union (1969); (iv) the NASA Space Exploration Initiative (1989); (v) Mars Direct by R. Zubrin and D. A. Baker (early 1990s); (vi) the NASA Design Reference Mission (early 1990s and 2000); (vii) the Mars Piloted Orbital Mission of the Russian Space Agency (2000/2005); (viii) the Aurora Programme of ESA (2001); the ESA–Russian Plan (2002); and the Vision for Space Exploration of the United States (2004).

  3. 3.

    See G. Gugliotta (2008).

  4. 4.

    A recent study compared Mars’s atmospheric concentrations of water to heavy water. It discovered that the concentration of deuterium over Mars’s polar ice caps is now much higher than in Earth’s oceans. See Villanueva G. L. et al. (2015).

  5. 5.

    Mars has a weak magnetic field, present over large areas of the planet, but that does not extend over the entire surface. Hence, Mars is not protected as Earth is from cosmic radiation. We do not have good information on ultraviolet radiation that reaches the Martian surface. Consequently, a more detailed understanding of the radiation environment is needed. Present robotic exploration should be collecting the information necessary to assess the effects of radiation on astronauts and future colonists.

  6. 6.

    ESA’s Mars Express mission identified this crater.

  7. 7.

    Adobe is the Spanish word for mud brick, made from natural building materials such as sand, clay, water, and fibrous or organic material.

  8. 8.

    While it is possible for humans to breathe pure oxygen, such an atmosphere is dangerous as demonstrated by the fire in the Apollo 1 capsule. So the Mars habitat may need additional gases. One possibility is to take nitrogen and argon from Mars’s atmosphere. Separating nitrogen from argon is difficult. It is suggested that the Mars habitat uses 40 % argon, 40 % nitrogen, and 20 % oxygen. Thanks to modern technology, Mars’s atmosphere could be compressed and adjusted to form a breathable mixture for humans. But the effects of breathing gaseous argon are unknown. Ongoing experiments are being conducted to monitor the health and activities of different animals while breathing a gas mixture that includes argon.

  9. 9.

    The liquid metal is a sodium potassium mixture, which is used to transfer heat from the reactor to a generator.

  10. 10.

    SP-100 (Space Reactor Prototype) is a US research programme for nuclear-fission reactors in space. A significant part of the SP-100 Project is aimed at identifying plausible missions and determining their requirements. Preliminary results indicate significant benefits of nuclear-reactor power systems.

  11. 11.

    Radioisotope power systems provide electricity and heat, enabling spaceships to undertake missions to environments beyond the capabilities of solar power, chemical batteries, and fuel cells. These technologies are capable of producing electricity and heat for decades under the harsh conditions of deep space without refuelling.

  12. 12.

    Nano-capacitors store electrical charge on two metal-electrode surfaces separated by insulating material. Their storage capacity is directly proportional to the electrodes’ surface area. Electrodes work in the same way as in conventional capacitors, but, instead of being flat, they are tubular and located deep inside the nanopores.

  13. 13.

    We assumed that the mission launch plane is inclined by 28.5 degree to the Earth’s equator, but 23.5 degree to the ecliptic plane. The plane change is thus 5 degree. Allowing a window within which to make the burn, the plane change is closer to 7 degree.

  14. 14.

    The spaceship needs a specific velocity to orbit Mars. This velocity is less than the one needed to continue to orbit the Sun in the transfer orbit. Hence the spaceship has to decelerate to be captured by Mars’s gravity.

  15. 15.

    See Zubrin R. et al. (1990); George L.E. et al. (1998); and Landau D.F. et al. (2006).

  16. 16.

    An instrument aboard the Curiosity Mars rover during its 253-day cruise to Mars calculated that the spaceship received around 660 millisieverts. The average yearly radiation dose received by a person on Earth is 3 millisieverts. It takes 250 millisieverts to cause any noticeable change in blood chemistry, and 750 millisieverts before any signs of illness occur. But at that level, recovery is likely; beyond that level, serious medical problems arise, so protection against radiation hazards on manned missions to Mars is a must.

  17. 17.

    A physics experiment on the International Space Station will help in these measurements. The Alpha Magnetic Spectrometer will be attached outside the station and will search for different cosmic rays, measuring their long-term variation over a wide energy range, and for nuclei from protons of iron.

  18. 18.

    Secondary radiation comes from the shielding material itself. When particles of space radiation smash into atoms within the shield, they trigger tiny nuclear reactions, which produce a shower of nuclear by-products—neutrons and other particles—that then enter the spaceship.

  19. 19.

    See R.H. Levy et al. (1964); and F.W. French et al. (1968).

  20. 20.

    See Horneck, G. et al. (2003).

  21. 21.

    Attitude control is the control of the orientation of an object with respect to an inertial frame of reference or another entity.

  22. 22.

    This idea is not new. In April 2008, the Russian space agency proposed building an orbital construction yard (OPSEK) for spacecraft too heavy to launch from Earth. See http://www.parabolicarc.com/2009/06/29/roskosmos-administrator-perminov-speaks-present-future-iss-cooperation/#sthash.sKlb544Z.dpuf.

  23. 23.

    A good example is the European Organization for Nuclear Research (CERN), which operates the world’s largest particle-physics laboratory. The large investment needed to build this laboratory induced 12 European nations to share the costs. The number of member countries subsequently grew to 28. CERN’s main role is to provide the particle accelerators needed for high-energy physics research. As a result, many experiments at CERN involve international collaboration.

  24. 24.

    Principally the Mars Foundation. Other organisations are simulating technologies and equipment needed to build the Mars base. Simulations are conducted in zones with temperatures close to those on Mars, such as in the Antarctic and northern Canada.

  25. 25.

    The idea of a rotating wheel to emulate Earth’s gravity has been around since the start of the twentieth century. Wernher von Braun envisioned one version, where the wheel is changed so that the pods where people live are tilted downward. This enables the wheel to add more gravity to the existing Martian gravity. The downward angle of the pods and the wheel speed can be adjusted to provide a 1 g net gravity.

  26. 26.

    See L. M. Weistein (2003).

  27. 27.

    Who will be the future colonists? A first group will be individuals who place high value in individual freedom, personal control, and self-realisation. They will be the modern version of frontier men and women. A second group will be individuals who place high value on the search for new opportunities or simply desire adventure and exploration. They are the modern version of Homer’s Ulysses. Today, as yesterday, personal values are diversified among the human population. A recent survey shows that the likely candidates constitute around 25 % of the population in advanced industrial countries; see Klinenberg E. (2012). The required skills will be mainly technical, geological, bio/geochemical, agronomical, and medical. Other skills, such as administrative, organisational, legal and logistics, should be assigned to individuals on the basis of their cross-training.

  28. 28.

    In English common law, dominions were autonomous political systems nominally under the British Crown. They had specific forms of fully responsible government (not to be confused with the nature of representative government). These institutions were able to legislate on every matter, except in the fields of foreign affairs, defence, and international trade. These powers remained under the control of the United Kingdom’s Parliament.

  29. 29.

    King James I granted a charter to the Virginia Company in 1606. He appointed the board of the corporation and endorsed the colony. Members of the English aristocracy who had wealth, power, and family connections were the leading members. In 1609, the king revised the charter and the colony’s governing constitution. The London board appointed a governor, who selected members of the council governing the colony; see Craven W. F. (1957); Bemiss F. M. (1957).

  30. 30.

    See D. Acemoglu et al. (2001).

  31. 31.

    Several low-mass metal liners form a thick blanket surrounding the target plasmoid and compress it to fusion conditions. The radiant, neutron, and particle energy from the plasma is absorbed by the encapsulating metal blanket. This energy is adequate to vaporise and ionise the metal blanket. This hot, ionised metal propellant expands through a magnetically insulated nozzle producing high thrust at the optimal specific impulse.

  32. 32.

    In this propulsion, only 20 % of the energy produced becomes kinetic energy. A significant fraction, around 70 %, is lost as electromagnetic radiation, mainly X-rays. This energy could be recovered, for example to make an auxiliary laser engine. In this way, exhaust velocities may reach between one-hundredth and one-tenth of the speed of light.

  33. 33.

    Annibale de Gasparis discovered 16 Psych in 1852. Since then, it has been the target of several astronomical observations. Many believe that it has an exposed metallic core different from its bigger parent’s body.

  34. 34.

    The physical mechanism that makes possible the oxygen’s presence starts from the dissociation of water molecules in the ice surface caused by the bombardment of cosmic rays. Oxygen molecules then spread into the liquid water through cracks in the ice caused by tidal motions.

  35. 35.

    Data from Voyager 1 and 2 suggest the presence of hydrocarbons in Titan’s seas and a thick atmosphere with approximately the correct temperature and to support them. Data from Hubble and other observations suggest the existence of liquid methane on Titan either in disconnected pockets or in wide oceans as on Earth.

  36. 36.

    See R. M. Zubrin et al. (1997); L. Bessone et al. (2004).

  37. 37.

    The comparative advantage of americium 242 over isotopes of uranium or plutonium lies in its chemical properties. Due to its lower critical mass, it can be produced as thin sheets of less than 1 micron. This enables fission products to ionise and escape the fuel easily. Carlo Rubbia and Giovanni Bignami proved that it takes the fission of a small quantity of americium 242 to produce a large amount of energy. Such ability to pack a big punch in a light and compact fuel allows for a smaller and lighter nuclear generator. Utilising such a generator in nuclear-thermal propulsion will allow for greater weight allocation to the payload, significantly improving the efficiency.

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Appendix: Various Propulsion Systems Proposed for a Manned Mars Mission

Appendix: Various Propulsion Systems Proposed for a Manned Mars Mission

4.1.1 Chemical Propulsion

Several proposalsFootnote 36 are under consideration for manned Mars missions based on liquid-propellant rockets. The most efficient fuel is liquid hydrogen, while combustion of hydrogen and oxygen is effective, which allows for a high specific impulse (around 450 s) compared to other propellant types, a technology that is already mastered. The Apollo missions used this technology for the trans-lunar injection. There are three challenges in using this cryogenic propulsion for a manned Mars mission:

  • Keeping a spaceship’s initial mass low. If used for the mission’s primary propulsion phases, the total mass in low Earth orbit is around 1000 tonnes, assuming a crew of six astronauts. To reduce the initial mass, propellant for the return trip must be produced on Mars. Alternatively, fuel must be sent in advance and stationed in Mars orbit.

  • Mastering the propellant’s evaporation. Today we can store liquid hydrogen and oxygen in a spaceship for a few weeks. But several months of storage are needed for a Mars mission. Space agencies (NASA, CNES) are working to improve the tank’s insulation and active cooling systems.

  • Primary rockets are lost after every launch. If plans entail several missions to Mars, non-reusable rockets affect overall costs and are an inefficient solution.

In summary, chemical propulsion consumes large amounts of fuel and has low-cost efficiency. Other technologies are being looked at, such as nuclear fission that uses 50 % less propellant than the best chemical engine.

4.1.2 Nuclear Propulsion

Nuclear-fission propulsion is a broad topic that includes several engine designs, which range from the thermal-nuclear engine to nuclear-electric engines and more advanced designs such as the Rubbia engine.

Thermal-Nuclear Propulsion

In thermal-nuclear propulsion, a nuclear reactor heats a coolant to high temperatures and expels it out through a nozzle. The most common type is the NERVA (Nuclear Engine for Rocket Vehicle Application), developed and tested in the 1960s. Their specific impulse is around 900 s, double that of chemical engines.

The main advantage of thermal-nuclear propulsion is its advanced stage of development (TRL). The United States and the then Soviet Union tested thermal-nuclear propulsion between 1960 and 1971. A few engines have operated for up to one hour with a thrust of 330 kN. Nuclear-thermal propulsion is still considered to be one of the key technologies by NASA and several related research activities within NASA and the DOE laboratories are ongoing. The Russians built and ground-tested several nuclear-thermal engines, which operated on a variety of propellants, including hydrogen, ammonia, and alcohol. Although their work continued until the mid-1980s, no evidence exists to confirm whether the Russians flight-tested any of these engines.

Nuclear-thermal propulsion offers other advantages: (i) shorter mission time (mission time to Mars is around 300 days, around half the time using chemical propulsion, due to the increased thrust); (ii) lower operating costs because of reduced propellant requirement; and (iii) efficiency of operations because the spaceship could be used in several missions to Mars, contrary to spaceships powered by chemicals.

The main challenges associated with the use of nuclear-thermal propulsion are:

  • Radiation, which a nuclear engine gives off in large amounts. Before considering these engines, effective shielding mechanisms must be developed. The goal is to limit the crew’s exposure to 10 REM. By comparison, the limit for civilians is 150 REM, and for military personnel 500 REM. The bad news is that this radiation shielding adds to the spaceship’s mass.

  • Testing a nuclear-thermal propulsion device is like testing a nuclear-power plant with the primary circuit open. Today, nuclear systems must have at least three confinement barriers: fuel cladding, a primary circuit envelope, and a confinement building for the reactor. Nuclear-thermal propulsion has a single confinement barrier: fuel cladding separating the uranium and fission products from the environment. To provide an environmentally safe system is thus a complex problem. Complexity could constitute a barrier to the development of these engines if not handled properly.

Nuclear-Electric Propulsion

Nuclear-electric propulsion is composed of two main parts: a fission-based power-generation unit and an electric propulsion module. A variety of thrusters use the electricity generated by the nuclear reactor. Ion thrusters use electric fields to accelerate ions to high velocities. In principle, the only limit on the specific impulse achievable with ion thrusters is the operating voltage and the power supply. Hall thrusters use magnetic fields to ionise the propellant gas and to create a net axial-electric field accelerating ions in the thrust direction. MPD thrusters use either steady-state or pulsed-electromagnetic fields to accelerate plasma in the thrust direction. To get a high thrust density, ion thrusters use xenon, while Hall and MPD thrusters can work well with argon or hydrogen.

One advantage of electric-propulsion technology is its steady development since the 1950s. Ion and Hall-thruster technologies have matured to the point that they are now being used on commercial and military satellites with photo-voltaic power sources. Magnetic Plasma Dynamcs (MPD)-thruster technology is still under development. Another advantage is the higher specific impulses of the electric propulsion. In contrast to a chemical rocket or a nuclear-thermal rocket, they can work continuously for days, weeks, and even months. The main problem is that they have a low power-to-weight ratio and a low thrust density. This makes nuclear electric propulsion infeasible for missions where high accelerations are required. Nuclear-electric propulsion is well suited for unmanned cargo missions between the Earth, Moon, and the other planets.

Advanced Nuclear Propulsion

Advanced nuclear propulsion is under study both in the United States and in Europe. The Idaho National Engineering Laboratory and the Lawrence Livermore National Laboratory advanced one proposal for a fission-fragment engine, which is an engine design that directly harnesses hot nuclear-fission products for thrust as opposed to using a separate fluid as the working mass. In a conventional nuclear reactor, the high kinetic energy of the fission fragments is dissipated by collisions to generate heat, which is then converted to electrical power with efficiencies of only 50 %. Alternatively, the fission fragments produced in the plasma reactor can be used directly for providing thrust. This design can, in theory, produce high specific impulses, while still being well within the abilities of current technologies. In Fig. 4.2, A are the fission fragments ejected for propulsion; B is the reactor; C are the fission fragments decelerated for power generation; d is the moderator, either beryllium or lithium; e is the containment field generator; and f is the induction coil.

Fig. 4.2
figure 2

Fission-fragment plasma-bed reactor (Source: Credit:http://en.wikipedia.org/wiki/File:Dusty_plasma_bed_reactor.svg)

In this engine, fuel is placed into several very thin carbon bundles, each one sub-critical. Bundles are collected and arranged like spokes on a wheel, and several wheels are stacked on a common shaft to produce a single large cylinder. The entire cylinder rotates so that several bundles are always in the reactor core where the additional surrounding fuel make the bundles go critical. Fission fragments at the bundles’ surface break free and are channelled for thrust. Lower-temperature unreacted fuel rotates out of the core to cool. The engine thus automatically selects the most energetic fuel to become the working mass. The engine’s efficiency is high; specific impulses greater than 100,000 s are possible using existing materials. But the reactor-core’s mass makes the overall performance of these engines lower.

In Europe, Rubbia designed an advanced nuclear engine between 1998 and 2002. This engine is powered by americium 242,Footnote 37 a fissionable material hungry for neutrons and capable of absorbing them when bombarded by neutrons. The fissionable material is coated in a thin layer (less than a micron) on the inner walls of a hollow cylinder. This tube is filled with normal gas (hydrogen) at pressures of one atmosphere. Thanks to this geometry, when fission occurs, a high probability exists that one fission fragment flies into the gas and deposits its kinetic energy there. In the nozzle, a small miracle of physics happens. Inside the tube, the super-heated gas moves in all directions with a chaotic motion. In the nozzle, the gas moves in one direction and pushes in the opposite direction. Newton is vindicated. The spaceship, anchored to the engine, moves in the opposite direction of the gas (Fig. 4.3).

Fig. 4.3
figure 3

Scheme of The Rubbia engine (Source: Bignami et al. 2011)

Temperature in the gas’s central region can reach around 10,000 °C. With this heating method, a large saving of fissionable material is possible. The spaceship needs just a few pounds of plutonium or americium for a round trip to Mars. This mass is equivalent to two large cups (1 litre of plutonium weighs around 20 pounds). The specific impulse is estimated at 4000 s. Average exhaust speed is estimated at 40 kilometres per second. But a few unsolved problems remain. The first one concerns the material that can withstand the high temperatures of the super-heated gas. Research is ongoing to develop materials that can do this. The second problem concerns the dissipation of the heat generated, which can be done by equipping the spaceship with large heat-exchange surfaces facing the void of space. Because the temperature of space is around 2.7 degree above absolute zero, it has an infinite capacity to absorb heat.

In summary, nuclear propulsion is the best near-term method for powering spaceships directed at Mars. It offers lower costs and shorter travel times. Among possible nuclear engines, we have chosen the more advanced nuclear propulsion, called the Rubbia engine. It enables a shorter time of travel, less use of propellant, and more payload compared to other nuclear-propulsion systems. The major drawback of advanced propulsion is that they are today only at the concept stage. They need extensive engineering work and testing before spaceships powered by them are ready to fly. But our scenario foresees an exploratory Mars mission in the course of the 2040s. This timetable provides sufficient time for the development and testing of advanced nuclear engines.

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Bignami, G., Sommariva, A. (2016). The Great Leap Out of the Cradle: The Human Exploration of Our Solar System. In: The Future of Human Space Exploration. Palgrave Macmillan, London. https://doi.org/10.1057/978-1-137-52658-8_4

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