Science
ACTUAL PROBLEMS OF AVIATION AND AEROSPACE SYSTEMS
Kazan Daytona Beach


VI-th Symposium on realistic near-term advanced scientific Space missions

review

Salvatore Santoli

INT - International Nanobiological Testbed Ltd., Italy-UK

 

This is the sixth edition of the symposium organized every two years in Aosta, Italy. This went on from July 6 to July 9, 2009, and like all its preceding ones it was organized by the IAA - International Academy of Astronautics and was devoted to advanced results concerning science and technology of missions to the outer solar system and beyond. Its proceedings have been published by the sponsors of the symposium, i.e. the Politecnico di Torino, the Regione Autonoma Valle di Aosta as the Assessorato Istruzione e Cultura, the Città di Aosta as the Assessorate Pubblica Instruzione, and by Hotel Europe which has been the hospiting venue. The proceedings have been edited by Prof. Giancarlo Genta, Chairman of the Organizing Committee. The Honorary Symposium Chairman was Dr. Leslie Shepherd, and the Chairman of the Scientific Committee was Dr. Giovanni Vulpetti. The Members of the Scientific Committee were

 

Jean-Michel Contant,

Giancarlo Genta,

Michael Gruntman,

Heiner Klinkrad,

Les Johnson,

Gregory Matloff,

Yoshinari Minami,

Eberhard Moebius,

Salvatore Santoli,

Leslie Shepherd,

Giovanni Vulpetti.

 

Twenty-four papers were presented. The following is a short review of all papers presented at the symposium. Seventeen out of the twenty-four papers were selected by the referees of the papers discussed at the symposium for proposal of publication in the journal Acta Astronautica.

 

Paul A.Gilster.

Interstellar Flight and the Public Imagination.

Here the problem is considered concerning the education of the public in interstellar travel issues as public involvement is considered to be an essential component of research, given the realities of straitened budgets and changing government strategies to respond to our society's vision of space exploration. It is remarked that no space agency can do the Europe Jupiter System Mission, for example, without a public sufficiently attuned to the interesting things that might be found among the Galilean satellites that justify the outlay. The role is examined of journalism and of the Web sites devoted to space, and it is advocated that researchers would master the new environment created by suitable reportage by learning to work with the writers and journalists whose job is to publicize their efforts, hoping that a fired public imagination will feed new sources of financial support.

 

Marco C.Bernasconi.

Space Exploration in the 21st Century: True Escapism or Deep Ethical Motives?

This paper discusses the fact that about fifty years ago some supporters of Astronautics got into a philosophical discussion as to whether space exploration represented a form of escapism. The Author's analysis concludes that beyond the philosophical considerations, we have to dream up systems for generating industrial power, for producing new wealth, and for keeping wealth. Astronautics realizations may provide both the material and social resources to make the respects of individuals' moral rights durative. Then deep space exploration will have freed itself of any suggestion of escapism.

 

Giancarlo Genta.

The Nuclear Renaissance: From the Power Industry to Space Exploration?

Space exploration seems to regain momentum, with the commitment by several space agencies to return to the Moon and the plans go beyond, at least to Mars, with human expeditions in a foreseeable future. True space exploration involves however a human presence in very deep space, beyond the orbit of Mars. While the vision of the space imperative does not impose a deadline, many supporters of the space option strongly support the idea that we have a time window to start our space faring civilization and a delay will cause our thrust outwards to stall, with the subsequent decline of our civilization. Is this vision correct, or we should now concentrate on developing enabling technologies to prepare a future in which human expansion in space, although slower, will lead to a civilization deeply influenced by its space faring character?

 

Tibor Pacher.

Unconventional Thinking in Interstellar Spaceflight Research: Practical Approaches.

Interstellar space flight and closely related topics, like a possible encounter with extraterrestrial life, are on the edge of interdisciplinary research. By their very nature these topics require unconventional thinking. Accordingly, two practical approaches that are expected to generate new ideas for practical interstellar flight involve the public and are not restricted to academics: the formulation, call and publication in a controlled way on the Web of Crazy Ideas, e.g. as the Crazy Ideas section at www.peregrinus-interstellar.net; and/or the formulation of a provocative but accountable prediction, e.g. cf. Interstellar Bet at www.longbets.org/395. Other possibilities are also explored for fostering ideas and unconventional thinking.

 

Nick Kanas.

From Earth's Orbit to the Outer Planets and Beyond: Psychological Issues in Space.

Current planning for the first interplanetary expedition to Mars in the early 2030s envisions a crew of six or seven people and a mission duration of around 2.5 years. However, this time frame is much less than that expected on expeditions to the outer solar system, where total mission durations of 10 or more years are likely. Although future technological breakthroughs in propulsion systems and space vehicle construction may sped up transit times, for now we must realistically consider the psychological impact of missions lasting for one or more decades. Strategies for dealing with psychological issues involving missions to the outer solar system are here considered and discussed, along with issues related to new technologies being considered for interstellar missions, such as putting the crew in suspended animation or creating giant self-contained generation ships of colonists who will not return to Earth.

 

Les Johnson, Mark Whorton, Andy Heaton, Robin Pinson.

Nanosail-D: A Solar Sail Demonstration Mission.

The characteristics of the Nanosail-D mission that unfortunately due to the launch vehicle failure never had the opportunity to deploy are here described. The Nanosail-D would have been the first on-orbit solar sail deployment demonstration. Details concerning the planned deployment successive operations are given.

 

Roman Ya. Kezerashvili, Justin F.Vázquez-Poritz.

Deviations from Keplerian Orbits for Solar Sails.

During the last two decades, a number of solar probes have been designed to perform in-situ near-Sun measurements in a rather unusual and difficult environment like that met by a solar probe penetrating to a few solar radii as the region of less than 0.3 astronomical units. It is shown that the curvature of space time, a possible net electric charge on the sun, a small positive cosmological constant and the oblateness of the Sun, in conjunction with solar radiation pressure affect the bound orbital motion of solar sails and lead to deviations from Kepler's third law for heliocentric and non-Keplerian orbits. With regard to the Lense-Thirring effect, the solar radiation pressure increases the amount of precession per orbit for polar orbits. Non-Keplerian polar orbits exhibit an analogy of the Lense-Thirring effect in which the orbital plane precesses around the Sun.

 

C.Bruno, D.Simone.

Nuclear Electric Propulsion for Interstellar Precursor Missions.

Interstellar precursor missions are considered where the propulsion system is based on a fission power nuclear reactor. This preliminary study suggests that nuclear electric propulsion may become a viable propulsion system for probes and spacecraft capable of exploring the farthest reaches of the solar system and possibly beyond.

 

P.Janhunen.

Status Report of the Electric Sail - A Revolutionary Near-Term Propulsion Technique in the Solar System.

The electric sail is a new propulsion concept which uses charged tethers to extract momentum from the solar wind by Coulomb interaction. The status of this propulsion technique is given as of May 15, 2009. Progress is thus reported during the last two years in plasma physical thrust estimation, tether manufacture methods, navigability, test mission planning and applications. Using existing technology, it looks like being possible to build an electric sail of about 1 N thrust, about 100 kg mass and about 10 year lifetime. In terms of lifetime produced impulse per unit propulsion system mass, such a near-term and general-purpose device would be about 1000 times more efficient than a chemical rocket and about 100 times more efficient than a contemporary ion engine, a level of performance that is enough to enable many important applications, such as in situ measurements in interstellar space, sample return from most solar system targets, non-Keplerian orbit probes for space weather forecasting and helioseismology as well as economical utilization of asteroid resources.

 

A.A. Quarta, G. Mengali, P. Janhunen.

Optimal Interplanetary Rendezvous Combining Electric Sail and High Thrust Propulsion System.

The performance of an electric sail for minimum time missions towards planets in the solar system is quantified under the simplified assumption of circular planetary orbits. Tow possible mission scenarios are investigated: in the first case, the sailcraft reaches the target with zero hyperbolic excess velocity, thus performing a rendezvous mission. In the second mission scenario the final hyperbolic excess speed is zeroed through a suitable chemical propeller.

 

Giovanni Vulpetti.

Effects of the Total Solar Irradiance Fluctuations on Sailcraft Trajectories.

Strangely enough, in the last four or five decades of photon-solar sailing studies, he solar radiation pressure on the sail has been assumed always constant. In the fifties/sixties some conjectures and/or preliminary theories suggested that the solar radiant existence was not constant as claimed by Astrophysics. Indeed, from the standpoint of solar system evolution, such as planet climate, interplanetary plasma features and its interactions with the celestial bodies, photon irradiance etc., the Sun is remarkably variable. As solar radiation pressure is the primary source of momentum change of a photon sailcraft, this paper is the first one of a planned set of papers where total solar irradiance variations are explicitly included in a large high-precision computer code for sailcraft trajectory optimization. Mars - sailcraft rendezvous has been chosen to begin with studying such effects.

 

Roman Ya. Kezerashvili, Justin F. Vázquez-Poritz.

Escape Trajectories of Solar Sails and General Relativity.

General relativity can have a significant impact on the long-range escape trajectories of solar sails deployed near the Sun. Space-time curvature in the vicinity of the Sun can cause a solar sail travelling from 0.01 astronomical units (AU) to 2550 AU to be deflected by as much as one million kilometres, and should therefore be taken into account at the beginning of the mission. There are a number of smaller general relativistic effects, such as frame dragging due to the slow rotation of the Sun which can cause a deflection of more than one thousand kilometres.

 

Giovanni Vulpetti.

Reaching Extra solar System Targets via Large Post-Perihelion Lightness-Jumping Sailcraft.

The fast solar sailing theory, formulated after the preliminary study of a photonic propulsion spacecraft featuring an ultra light monolayer solar sail with a reflective membrane of carbon nanotubes obtained by a novel technology for carbon nanotube membranes, allowing cruise speeds up to some thousandths the speed of light (Giovanni Vulpetti, Salvatore Santoli and Gabriele Mocci, Preliminary Investigation on Carbon Nanotube Membranes for Photon Solar Sails, JBIS, Vol. 61, No. 8, pp. 284-289, ISSN 0007-084X) is here applied for the first time to a multi-target mission sailcraft with maximum lightness number significantly greater than 1. The farthest target is the solar gravitational lens zone. The high speed of this solar sail allows distances of 550 astronomical units to be reached 17.5 years after the departure from the Earth-Moon system. The astrodynamical concept of large post-perihelion lightness-jumping is discussed and all details of the sailcraft structure and engineering design are illustrated.

 

Claudio Maccone.

Focal Mission to 550 Thru 1000 AU: Status Review 2009.

A review is presented of a 2009 status of the FOCAL space mission, that has been studied by the author and others since 1992 and was formally proposed to ESA for consideration after the year 2000, and whose objective is the realization of a probe to reach distances between 550 and 1000 astronomical units (AU) to exploit the huge radio magnification provided there by the gravitational lens of the Sun, as predicted by the general theory of relativity. It is stressed that the present status FOCAL technologies mainly consist in the use of a relativistic interstellar flight profile called "hyperbolic motion" to reach 1000 AU in the smallest amount of time and the relevant propulsion problems, and in the utilization of the relativistic Karhunen Loève Transform (KLT) instead of the classical FFT to insure optimal telecommunications with the Earth during such relativistic flight.

 

Arturo Graziano Grappone.

Assembly-Level Anticipatory Programming in Space Missions.

With a view to developing an efficient software an a remarkable reduction of hardware in space missions, and with a strong reduction of payload and considerable savings for launchers, the principles of the emerging mathematics for anticipatory systems are illustrated and then a direct implementation of the anticipatory mathematics iterative algorithm is proposed by low-level programming, i.e. by a reformulation of the Assembly language.

 

Greg L. Matloff, Monika Wilga.

NEOs as Stepping Stones to Mars and Main-Belt Asteroids.

Human interplanetary ambitions are constrained by the problem of astronaut exposure to galactic radiation. I survey is here presented of the existing on-line Near Earth Object (NEO) database in an attempt to identify NEOs that cross both Earth's and Mars's orbits and could be used as cosmic-rays shields by interplanetary voyagers. The search concentrated on low-inclination Mars-crossing NEOs that approach Earth, Mars and main-belt asteroids in the time frame 20020-2100. Both outbound and return transfers were searched for. Several candidate NEOs for Earth-Mars, Mars-Earth and Earth-Vesta transfers have been found from the very incomplete existing database of about 5,000 NEOs. Kinematics of Earth-NEO transfer is also considered.

 

F. De Tiberis, L. Simone, D. Gelfusa, P. Simone, R. Viola, A. Santoni, O. Cocciolillo, M.Ziarelli, F. Barletta, N. Salerno, M. Maffei, V. Nanni.

The X/X/KA-Band Deep Space Transponder For the BepiColombo Mission to Mercury.

A detailed overview and the architectural design of the Deep Space Transponder equipment that has been developed by Thales Alenia Space, Italy, for the European Space Agency (ESA) BepiColombo mission to Mercury, whose scientific goals were aimed at estimating the rotational dynamics of Mercury, thus allowing to accurately infer the internal structure; the global structure of the gravity field of Mercury, thus allowing to accurately infer the internal structure; the local gravitational anomalies of Mercury, thus allowing to accurately infer the structure of the mantle and the crust-mantel interface; the orbit of Mercury around the Sun and the propagation of electromagnetic waves between the Earth and Mercury, in order to improve the determination of the post-Newtonian parameters and test the General Theory of Relativity to an unprecedented level of accuracy.

 

Giancarlo Genta, Alessandro Genta.

A Small Robotic Rover for Titan Exploration. Part 1: General Layout.

Titan is a very interesting target in deep space exploration. With its solid surface on which a rover can easily travel and its methane lakes which can be sailed it is the ideal target for a deep space mission which includes a mobile platform. If the Huygens lander of the Cassini mission had a device of this type, the scientific returns of that already most successful mission would have been much larger. The general layout of a rover for a mission to Titan is studied. The results apply not only to a future mission to Titan, but also to other missions that in the future will be designed for reaching satellites of the outer planets of size comparable with that of Titan and the largest Kuiper belt objects like Pluto and 136472 Makemake. The simple configuration studied in this paper for a small rover allows the rover to move on the surface of Titan both on solid and liquid surfaces. A radioisotope thermoelectric or thermal generator is suggested as the power source, and a set of wheels was designed that could be used as paddle wheels for sailing the methane lakes with a methane-tight vehicle shaped as a boat by raising the wheels above the liquid level.

 

Giancarlo Genta.

A Small Robotic Rover for Titan Exploration. Part 2: Strategies for Trajectory Control.

In the configuration study for a small robotic rover for Titan exploration described in Part 1, a four-wheel configuration with trajectory control based on slip steering was chosen. Here this solution is compared with the more conventional strategy based on steering wheels. A method for the trajectory design based on the potential approach is assumed and an ideal trajectory is obtained for a few typical cases. The actual trajectory followed by the rover is then simulated using the ideal trajectory for both slip steering and conventional steering control, for different vehicle speeds. In the second case both kinematics and dynamic steering were assumed. As a result the simulated trajectories are shown to state the adequateness of slip steering.

 

Salvatore Santoli.

Devising an Unconventional Formal Logic for Bioinspired Spacefaring Automata.

The field of robotics is increasingly moving from robots confined to factory floors and assembly lines and bound to perform the same tasks over and over in an uncertainty-free, well foreseeable environment, to robots designed for operating in highly dynamic and uncertain domains, like those of interest in space exploration. According to an idea of a "new system of formal logic less rigid than past and present formal logic" advocated by J. von Neumann for building a powerful theory of automata, such system should be "closer to another discipline which has been little linked in the past with logic, i.e. thermodynamics, primarily in the form it was received by Boltzmann". Following that idea, which is particularly interesting now with the emerging computational nanosciences, it is stressed here that a full set of isomorphisms can be established between the fundamental logical principles and the information flows, Hamiltonian or dissipative, in phase space. This form of logic, dubbed here kinetic logic, takes standard formal logic out of the field of combinatory and into the field of the Boltzmannian form of thermodynamics, i.e. kinetics.

 

J. Poncy, V. Martinot, J. Fontdecaba-Baix, F. Feresin.

A Preliminary Assessment of an Orbiter in the Haumean System: How Quickly Can a Planetary Orbiter Reach Such a Distant Target?

With the recent discoveries of planetary objects beyond Neptune and Pluto, the vast majority of all sizeable Solar System planetary objects lie now beyond Uranus, where insertion into orbit after a reasonably short travel is still not within the current capabilities of our spacecraft. Being able to go and stop at a transneptunian dwarf planet would represent a stepping-stone for ambitious long-term goals such as Solar System colonization or interstellar travel, both in term of technology and logistics. Thales Alenia Space has carried out a preliminary assessment of a mission with a challenging target of such kind: in orbiter in the Haumean system. The main parameters of the mission design are presented, and a review is supplied of the technological options and challenges. The performance is inferred for high-specific-impulse propulsion and power generation as a function of launch mass and allowed cruise duration. An optimum specific impulse of about 10,000 was identified. It is concluded that carrying out such a mission within a reasonable duration compatible with scientists' careers would demand progress beyond the current state of the art, mainly for mass of power generators.

 

Nikolay Slyunyayev, Alexander Degtyarev, Oleg Ventskovsky.

Concept of Creation of the Orbital Stages for Deep Space Missions.

A concept of creation of the orbital stages of the rocket-space systems capable to deliver payloads to the far borders of the Solar System is discussed. The concept assumes that the rocket starts from the Earth using off-the-shelf chemical fuel engines with specific impulse in the range of 300 - 600 s. For further flight of the orbital stage the energy sources employed were the gravitational fields of the Earth and planets, the magnetic fields of the Earth and planets, and solar radiation energy, with options of the orbital stage design characteristics for collection of the dangerous asteroids.

 

Claudio Maccone.

The Living Drake Equation of the Tau Zero Foundation.

The Living Drake Equation is the statistical generalization developed in this paper of the well known Drake equation such that it can take into account any number of factors. The new result opens up the possibility to enrich the original equation by inserting more new factors as long as the scientific learning increases. The qualifier Living refers just to this envisage able continuous enrichment of the Drake equation and is the goal of a new research project that the Tau Zero Foundation has entrusted to the author of this paper as the discoverer of the Statistical Drake Equation described here. The original Drake equation is in the form of a simple product of seven positive numbers, and such equation is here transformed into the product of seven positive random numbers. The mathematical consequences of this transformation consist in giving the Drake equation a more scientific character as the original purely arbitrary deterministic parameters are substituted with statistical estimates whose accuracy will increase as the advancement of knowledge as relative will increase. Moreover, this development makes the original arbitrary Drake equation the characteristic scientific feature of being falsifiable.



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