By the MEPAG Mars Forward Lunar Objectives Science Analysis Group
David Beaty, (Mars Program Office, JPL/Caltech), Jennifer L. Heldmann (NASA Ames Research Center / SETI Institute), Lewis Peach (USRA), Noel Hinners (Consultant), Ben Clark (Lockheed Martin), Robert Easter (Jet Propulsion Laboratory), Robert Braun (Georgia Tech), Richard Mattingly (Jet Propulsion Laboratory), Chip Shearer (University of New Mexico)
September 16, 2006
Recommended bibliographic citation: MEPAG MFLO SAG (2006). Draft Findings of the Mars Forward Lunar Objectives Science Analysis Group, Unpublished white paper, 22 p, posted October, 2006 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag.jpl.nasa.gov/reports/index.html. or
Beaty, D.W.; Heldmann, J.L.; Peach, L.; Hinners, N.; Clark, B.; Easter, R.; Braun, R.; Mattingly, R.; Shearer, C.; (2006). Draft Findings of the Mars Forward Lunar Objectives Science Analysis Group, Unpublished white paper, 22 p, posted October, 2006 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag.jpl.nasa.gov/reports/index.html.
Comments are welcome, and should be directed to David W. Beaty (David.Beaty@jpl.nasa.gov, 818-354-7968), Jennifer L. Heldmann (email@example.com, 650-604-5530), or, Lewis Peach (firstname.lastname@example.org, 410-730-2656). Document Review reference number: CL#06-3374.
The Mars Exploration Program Analysis Group (MEPAG) has completed a preliminary analysis of the June, 2006 draft list of possible lunar objectives from the perspective of its relevance to preparation for human missions to Mars. MEPAG has reached eight preliminary findings.
1. Introduction and Background (from Jeff Volosin, NASA-HQ)
In late 2005, the NASA Administrator stated that in 2006, NASA would initiate a process to define a compelling story to address two questions: "Why are we returning to the Moon?" and "What are we going to do when we get there?" The Exploration Systems Mission Directorate (ESMD) initiated an effort, with participation from the Space Operations Mission Directorate (SOMD) and the Science Mission Directorate (SMD), to define and implement a process to address these questions. The initial stage of this process focused on the need to facilitate broad community involvement in addressing these questions, identifying key objectives for the lunar exploration program and thus contribute to the development of a more inclusive and comprehensive Global Exploration Strategy. Inputs were to be solicited from academia, international space agencies, and private sector organizations. By collecting and analyzing these data, NASA would then be in a better position to define the role that the United States should play in lunar exploration as well as begin to develop an understanding of potential opportunities for broad cooperation and collaboration in the exploration of space.
1.2 NASA Exploration Workshop
To initiate this process, NASA held an Exploration Strategy Workshop in Washington D.C. in April of 2006. Over 180 engineers, scientists, entrepreneurs, and other exploration experts from the international community attended this Workshop and provided NASA with some initial thoughts on the answers to the two questions posed above, that were captured in the form of Themes and Objectives:
1.3 Additional Inputs
In addition to this Workshop, NASA solicited independent recommendations for lunar objectives from the public through a Request For Information (RFI) that was open through early May 2006.
1.4 Synthesis and Vetting Process
The result of these two activities led to the identification of 85 proposed lunar themes and over 800 proposed lunar objectives. Since these submissions were provided by many different individuals, NASA next initiated an internal Synthesis Team activity to remove duplication and combine similar proposals. The result of this synthesis effort was the identification of six unique lunar themes and 85 lunar objectives. In an effort to ensure that this resulting set of themes and objectives was thorough and complete, NASA next initiated a series of vetting processes utilizing existing specific organizations that represented academic, international space agency and private sector scientific and exploration interests. These organizations included:
1.5 Resultant Product
The result of this process was the identification of an additional 100 lunar objectives and additional information that could be used to support the six themes identified earlier. As a result of the extensive engagement of the community in this assessment, more than 1,000 individuals had provided inputs to the process.
2. Basis for Assessment
2.1 MEPAG Goal IV Mars Human Precursor Study
A recent study was conducted by the MEPAG Mars Human Precursor Science Steering Group (MHP SSG) (Beaty et al., 2005) to analyze the priorities for precursor investigations, measurements, and technology/infrastructure demonstrations that would have a significant effect on the cost and risk of the first human mission to Mars. The purpose was to determine, in priority order, the ways in which the risk of a human mission to the martian surface can be reduced by means of robotic flight missions to Mars.
The scope of the MHP SSG study was to analyze the investigations of Mars by precursor robotic missions for the purpose of reducing mission risk/cost and increasing performance of a human mission to Mars. However, in order for a preparatory program to be complete, the following kinds of precursor investigations also need to be considered:
The MHP SSG considered ONLY robotic precursor missions to Mars. However, the current MFLO SAG study builds upon the work of the MHP SSG in terms of identifying the major risk/cost to a human Mars mission and also opportunities to cost-effectively increase performance. The MFLO study differs from the MHP SSG study in that the MHP SSG study considered robotic precursor missions to Mars as preparation for a human Mars mission whereas this MFLO SAG study considers robotic precursor missions to the Moon in preparation for a human Mars mission.
2.2 Purpose and Scope of MFLO Review
ESMD has recently prepared a draft set of themes and objectives for lunar exploration that have been synthesized from several activities, including the NASA Exploration Strategy Workshop and a Request for Information. NASA's formal statement of its strategic goal linking Mars and the Moon is to "establish a lunar return program having the maximum possible utility for later missions to Mars and other destinations". This topic is critically important and will influence the architecture for upcoming lunar exploration.
The purpose of the MFLO review is to evaluate the draft lunar planning from the perspective of eventual application to Mars. MEPAG was thus invited by NASA Headquarters to review the synthesis report and address the following questions:
2.3 MFLO Analysis Process
The MFLO analysis included the following steps:
The team further considered:
2.4 MEPAG Validation Process
The MFLO assessment was conducted on a time scale of two weeks by a small 'tiger-team' that had extensive involvement in the development of the recent analysis of MEPAG Goal IV. Because of the timing, it has not yet been possible to carry out MEPAG's normal vetting process, so this should be considered an interim assessment.
The MFLO study will be vetted with the Mars community, however, through the standard MEPAG procedures. The initial findings of the MFLO SAG will be presented to the community at the upcoming MEPAG meeting in Washington, D.C. (January 2007). Community members will then have the opportunity to comment on the MFLO findings. These comments will be evaluated and incorporated as appropriate by the MFLO study team. Once the findings reach a state of consensus then the white paper will be published as an official MEPAG document.
3. Comparison of Human Missions to the Moon and Mars
In order to analyze the ways in which the various aspects of the lunar exploration program might be beneficial to Mars, it is helpful first to compare and contrast the essential aspects of missions to the two destinations.
3.1 Primary similarities between crewed missions to the Moon and Mars
The primary similarities that provide a basis for designing lunar systems with maximum utility for eventual application to Mars human missions are discussed here. Such utility is two-fold: 1) physical systems designs, the basic elements of which can be applied with customization to Mars and 2) relevant operational experience.
A. The most obvious similarity is the mutual need for high reliability life support systems as neither environment has the requisite water, atmosphere or food to sustain a crew on the surface. Thus for both destinations life-support must be provided for the full mission duration which includes both round-trip transit and surface stay-time. For the Moon it is feasible and practical, relatively speaking, to use a "brute force" system of supply and resupply with attendant disposal of used resources. In theory such an approach is also possible for Mars. However, the cost of delivering mass to and from Mars is so much greater, and the mission opportunities, which are limited by orbital mechanics, are so infrequent, that it may be mission limiting if alternatives cannot be developed. Such alternatives include closed-loop or nearly-closed-loop life support systems and, eventually, ISRU (in situ resource utilization). Both of these techniques, while not essential, would enhance long-duration lunar outpost missions. It is doubtful that a Mars mission architecture which was dependent upon these technologies would ever be undertaken without having first demonstrated "proof of concept" for these techniques in a prior application (not necessarily on the Moon - some could be done on Earth and the International Space Station (ISS)).
B. Sustaining the health of crews is essential for survival and for effectively attaining mission goals. Operating for prolonged periods in low-gravity (~ 1/6 Earth gravity for the Moon and ~ 1/3 Earth gravity for Mars), exposure to cosmic and solar radiation and exposure to pervasive dust are environmental conditions common to both the Moon and Mars. They differ only in degree. The long-duration implications of lunar gravity are unknown, as are the implications of martian gravity. Human exploration of the Moon will provide the first good, long-duration, data point between micro-gravity (ISS) and 1 g (Earth) which will go a long way towards understanding the implications of Mars gravity and for developing any needed counter-measures to mitigate serious physiological de-conditioning issues and help assure human health for long duration missions to Mars. Radiation is another matter of serious concern for the human exploration of space. Techniques developed for constructing radiation shielding on the Moon, using native (regolith) materials, the attendant computer models and improved understanding of the biological effect of high-Z cosmic rays can be directly transferred to Mars missions. The effects of lunar vs. martian dust is more problematic as both the chemical and physical characteristics of the dust are grossly different in the two environments. However, lessons learned in ameliorating both mechanical and physiological effects of lunar dust will produce a cadre of engineers steeped in the discipline of developing seals, filters, cleansing techniques, and overall less-susceptible mechanical and electrical designs. Similarly, physiologists must understand the implications of the inevitable crew inhalation of micron and sub-micron dust particles, of irritation of eyes and mucous membranes and of possible chemical reactivity (probably more serious on Mars with its known highly oxidizing dust).
C. Potential health hazards go beyond those which may be induced by gravity, radiation and dust. Judged by some to be the most challenging for a Mars mission are the psychological factors induced by a two-to-three-year isolation from home, with no quick abort possible and, relative to lunar missions, a greater likelihood of medical emergencies. While no simulation or lunar mission can impose the reality of "no early return", long-duration lunar missions can aid in developing work/recreation/social interaction schemes designed to maintain a healthy mental outlook. And even in the lunar case, there could well arise medical emergencies which cannot be resolved with a three to four day abort to Earth. It, like launch vehicle losses, is simply a question of time.
D. Surface infrastructure and support requirements such as EVA (extravehicular activity) space suits, mobility systems and habitats are common elements of all Moon and Mars sortie and outpost missions. Again, designs will differ in detail yet the commonality of fundamental requirements for ease and flexibility of crew motion, reliable and repairable mobility systems and for highly functional yet homey, personalized habitats argues for high potential relevance.
E. Both Moon and Mars exploration programs need development of greater launch capacity and larger power systems than currently exist. While solar cells and fuel cells can in theory supply some of the needs, the development of nuclear surface power for lunar applications will be directly useful on Mars, especially if ISRU becomes practical; in fact, nuclear power may be enabling for ISRU, which in turn, is also likely enabling to long-term, sustainable human exploration.
F. Concerning scientific exploration per se, the basic techniques of geological and geophysical field research are well known and common to all planetary body explorations. They are fundamentally variants of what has been done on Earth and as was demonstrated on Apollo. New, however, is the potential for a significantly enhanced integrated robotic/human exploration. Long geophysical traverses, remote sampling and robotic assistants to do the drudge work and go into potentially hazardous locations are but a few examples of what can and ought to be done. Such an integrated approach will be valuable in lunar exploration but likely more so on Mars given the much higher cost per unit time of astronaut work.
A common theme runs through "primary similarities": to best prepare for eventual Mars human exploration, a constant awareness of and accommodation of the requirements for Mars must become part of the everyday thinking of lunar exploration. Even if some Mars "requirements" add incremental cost, the long-term payoff may well justify that investment. It is also likely that such investment will result in a more effective and productive lunar exploration.
3.2 Primary differences between crewed missions to the Moon and Mars
A. Both Mars and the Moon have very dry, rocky, dusty terrain and both have a lower gravity field than Earth. But the martian gravity level at its surface is more than twice that of the Moon, so that the relatively heavy portable life support systems (PLSS) built into spacesuits that were used in the Apollo missions would be far too heavy for use on Mars.
B. Mars also has a sensible atmosphere, which profoundly affects the engineering challenges of safe entry, descent and landing (EDL) as well as operations on the surface. The EDL phase of landed missions for Mars requires an aeroentry heat shield with thermal protection of the aft-body. All Mars missions to date have also used a large disk-gap band parachute deployed at supersonic velocities to further reduce the entry velocity. Retrorockets have been used for terminal propulsion, augmented by crushable legs or air bags. In many areas of Mars, the population of angular rocks is very high. On Mars, high near-surface winds must be accounted for in this terminal descent system.
C. The presence of an atmosphere and further distance from the Sun moderates temperature swings on Mars. On the Moon, peak daytime temperature of soil can reach +120 deg C or more, i.e., higher than the boiling point of H2O. On Mars, excursions above the freezing point of H2O are brief, restricted in both location and season. The day-night temperature swings on the Moon are about 300 deg C in amplitude, whereas on Mars diurnal cycles vary by 60 to 100 deg C.
D. Lunar dust sticks to cloth because of the Velcro-like action [NW1]of glass blebs on the surfaces of grains created by relentless bombardment by hypervelocity micrometeoroids. Small meteoroids encountering Mars are ablated and slowed in the martian atmosphere before reaching the surface. On the other hand, the martian dust is a far finer grain size than lunar regolith, presumably because of being created by a combination of physical and chemical weathering. Dust devils are common in many places on Mars, but absent on the Moon. Methods of filtration and cleaning to mitigate dust may be somewhat different, but could also have important similarities. Rovers on Mars have gotten bogged in low bearing-strength soils which so far have not been encountered on the Moon.
E. The Moon is much closer to Earth in distance and in travel time (although there is not a proportionate reduction in 'propulsion energy requirements' because lunar missions do not benefit from aeroentry, or atmospheric drag, which reduces descent delta-velocity requirements for Mars missions, whereas lunar missions require all-propulsive maneuvers). Aborting from a lunar mission for reasons of crew safety is quite feasible, as Apollo 13 demonstrated, but aborting a Mars mission is almost out of the question after the first week or so in space, with the exception of forgoing a landing for a long, slow, free return abort. Communications latency to the Moon requires about three seconds in an optimum case, and is not significantly more difficult than delays using geosynchronous satellite links. For Mars, roundtrip light travel time is up to forty minutes, and dips to eight minutes for only a short portion of mission time. Teleoperation of rovers on Mars has proven to be a distinctly different operation mode from the "joysticking" that is possible for rovers on the Moon. For this reason, it is often thought that martian astronauts must have far greater operational autonomy than lunar astronauts have ever been afforded. The long time in space and inaccessibility for resupply for a Mars mission will likely demand closed-loop regenerative processing of life support commodities such as air and water. Such has not been found necessary for Moon, shuttle and space station operations because of their more limited duration missions and reasonably frequent ability to resupply from Earth.
F. In situ resource utilization (ISRU) at Mars is far different because of the availability of a key ingredient, carbon dioxide, in the atmosphere. Also, water is present in almost all martian soils and ice deposits are likely within a few meters of the surface at many mid and high latitudes on Mars. Neither CO2 nor H2O are present at these high levels on the Moon, except possibly in permanently shadowed polar traps. Extraction of lunar oxygen will be from regolith minerals, whereas on Mars it can be from the atmosphere or soil water. The specific engineering systems will be different, but gaining experience in operability of systems requiring access and processing of surface materials at the Moon could demonstrate generic feasibility (or difficulty) of such systems for Mars (see Section 4.4 for a detailed discussion of the special case of ISRU).
G. Another key difference is the requirement for planetary protection, which is serious for forward contamination of Mars but with even more serious safeguards needed to assure protection against back contamination. Although the Apollo program had some measures in place to achieve these, it was quickly decided that they were not necessary and will not be required in future missions. Because the Moon is sterile, it can provide a useful testing ground, to assess the effectiveness of forward contamination preventative measures. should the lunar program be willing to develop its habitats and spacesuits with this as an engineering requirement.
3.3 Preparation for Mars Exploration
Preparing to send humans to Mars within acceptable risk standards will require a variety of precursor development work. We can organize this development work into four distinct portions according to venue: activities done at Mars, at the Moon, in Earth orbit, and on the Earth. As pointed out by Hinners et al. (2005), there is a well-defined progression in cost across this sequence-doing things at Mars is much more expensive than doing them on the Earth. This derives from the obvious but all-to-frequently unstated fact that as one moves away from Earth, the amount of data and the flexibility of experiment design, testing and re-test progressively decrease and the cost escalates dramatically. We cannot justify acquiring information at Mars if information of acceptable quality and utility can be acquired less expensively on Earth. As an example, experimenting with and developing a closed-loop space-qualified life support system is easier and cheaper to do on Earth followed by first flight demonstration on ISS.
It is becoming increasingly clear that a plan describing the full spectrum of activity required to prepare for the conduct of safe human missions to Mars is essential. Even though such a plan would need to be carried out over an extended period of time, and the work would certainly be sponsored by a variety of funding entities (on an international basis), without this we don't have a clear means of knowing how the pieces all fit together, how they relate to each other, and whether there are gaps that are not being worked at all. In particular, this would help us to understand the importance of the various R&D activities taking place on Earth at Mars analog field sites, in laboratories, in engineering test facilities, and by means of computer simulations.
4. Analysis of Priority of Draft Lunar Objectives to Mars
4.1 Prioritization Scale
In assessing the relevance of the lunar objectives to Mars exploration and science, the MFLO SAG felt that a simple binary response was inadequate and that it is more useful to indicate the degree of relevance to Mars; Therefore, a prioritization scale, consisting of the following definitions, was developed and used to rate the degrees of relevancy.
Essential Precursor Requirement => An activity that must be performed on the Moon, as a precondition to human exploration of Mars, which is considered enabling and therefore is a firm requirement that must be met, and one that might only be achieved through the lunar exploration program.
High Relevance => An activity that, given the lunar program, could be performed on the Moon as a precursor to Mars exploration, which is considered of sufficient value and priority that it warrants a marginal investment to assure maximum relevance to Mars (i.e., there is a high correspondence between the activity at the Moon and the fidelity of a representative capability that is needed at Mars, and this is seen as a cost effective, and timely means to achieve this goal).
Medium Relevance => An activity that, while it could be performed on the Moon, might be more effectively accomplished by other means - Earth analogs, space station, robotics precursors, etc. (i.e., there is a less compelling rationale that these activities need to be demonstrated on the Moon, and/or, there may be more efficient (lower costs) or more relevant means (higher fidelity) to achieve these goals).
Low Relevance => An activity that is of low priority for the 'Mars Human Precursor-Lunar Program' (MHP-LP) that would be better demonstrated by other means. (i.e., demonstrating this on the Moon is of sufficiently low value that this should not be a part of the MHP-LP).
(No score, or 'X') => n/a - An activity, which while possibly serving other needs, is not seen as relevant to the MHP-LP.
4.2 General Relevance of Lunar Program to Preparation for Mars
The MEPAG MFLO SAG examined the draft lunar objectives from two perspectives including 1) relevance to preparation for Mars human missions and 2) relevance to better understanding Mars scientifically. MFLO study results indicate that a significant fraction of the lunar objectives have some (variable) degree of relevance to Mars. The qualifier is significant in that no objective was considered absolutely essential (i.e., absolutely required before one could conduct Mars human exploration). In other words, one could proceed today with preparation for Mars human exploration without an intervening lunar program. Notably, no Mars-relevant objectives were deemed missing from the lunar objectives. Neither of these observations negates the potential utility of lunar exploration in preparing for Mars; the lunar exploration program offers many opportunities to better prepare for Mars. In that spirit, the MFLO SAG examined the individual objectives and suggested modifications that could improve the relevance to Mars. Additionally, as mentioned in the previous section, a priority ranking was assigned to each objective, rather than simply checking the box of relevant or non-relevant. The lunar program has not yet incorporated this prioritization approach; we recommend that this be done as the total set of lunar objectives is further refined.
4.3 Relationship of Lunar Program to MEPAG Goal IV: Prepare for Human Exploration
MEPAG has conducted an analysis of the robotic science measurements and engineering/technology developments that could accomplish significant risk-reduction for Mars human exploration (MEPAG, 2006). The Goal IV study pertaining to "Prepare for Human Exploration" had two major objectives A: Obtain knowledge of Mars sufficient to design and implement a human mission with acceptable cost, risk and performance and B: Conduct risk and/or cost reduction technology and infrastructure demonstrations in transit to, at, or on the surface of Mars.
When Goal IV was developed, it was assumed that any work that could be done somewhere other than Mars (e.g. on Earth, in Earth orbit, on the ISS, or on the Moon) would be done in these alternative locations. Nevertheless, as a sanity check, the MFLO SAG examined Goal IV to re-assess whether any of its objectives could instead be accomplished on the Moon. The finding is "No", reinforcing that some objectives must be carried out at or on Mars well before one can conduct a human exploration mission. Our reassessment had an ancillary positive benefit of helping determine where selected lunar objectives could be made more relevant to Mars preparation. Our proposed re-writes of selected lunar objectives reflects that perspective.
4.4 A Special Case: ISRU Moon/Mars Linkages
Elements of ISRU (in situ resource utilization) constitute many of the objectives of the lunar exploration program. It is recognized as a potentially valuable technique to significantly reduce the mass carried to the Moon and thus reduce the cost of lunar exploration and to be relevant to Mars. Indeed, similar objectives have been stated for future Mars human exploration and MEPAG Goal IV addressed the Mars-unique aspects of ISRU. Given the greater cost of carrying mass to Mars, its application at Mars takes on greater importance; some believe that ISRU may be, along with other mass-saving approaches, enabling of a human Mars mission. That said, for both the Moon and Mars, the potential of ISRU is subject to major uncertainties regarding the nature of the resources present, their accessibility, future supply/demand relationships, and technical/economic factors involved in extraction, production, storage and utilization processes. Developing and proving out certain basic ISRU capabilities on the Moon has direct relevance to its application to Mars. However, there are significant, non-trivial differences. On the Moon, regolith silicates and ilmenite are a known widely available resource. They each require extensive energy to extract oxygen and have unique processing requirements. The possibility that exploitable hydrogen exists in permanently shadowed polar regions gives hope that an easily extractable source of fuel will be available. For Mars, atmospheric CO2 and hydrogen (most likely as water) are widely present and likely obviate the need to use silicates.
The ultimate value of lunar ISRU experience to future Mars application depends to a significant degree on resolution of many details concerning both the Moon and Mars. This uncertain but potentially important relationship between use of lunar ISRU and martian ISRU needs further study to enhance the potential of Mars ISRU.
4.5 Science Linkages between the Moon and Mars
Lunar planetary science investigations are not required to prepare for human exploration of Mars. However, one of NASA's goals pertaining to the lunar program is to ensure "maximum possible utility for later missions to Mars". Based on this goal, there are important scientific concepts that could be developed on the Moon that will provide valuable insights into understanding Mars as a planet. The scientific linkages between the Moon and Mars were most recently examined in the MEPAG white paper "Findings of the Moon_Mars Science Linkage Science Steering Group" (Shearer et al., 2004). This analysis group reviewed this document and concluded that the basic scientific linkages were still valid.
The Moon_Mars Science Linkage Steering Group (2004) and the Exploration Strategy Workshop (2006) identified fundamental science themes that are relevant to understanding both the Moon and Mars. The science themes are cross-referenced in this discussion.
A. Early Planetary Evolution and Planetary Structure: The Moon has been and will continue to be the scientific foundation for our understanding of the early evolution of the terrestrial planets. The detailed geologic record of these early events has long since vanished from the Earth and has been at least partially erased from Mars. The Moon contains the remnants of one of the basic mechanisms of early planetary differentiation: magma ocean. These remnants are in the form of a primary planetary crust and subsequent crustal additions that were products of melting of magma-ocean products in the lunar mantle. Clearly, the differences in size and formation between the Moon and Mars have affected the style of differentiation and early magmatism. However, the Moon provides a valuable and nearly complete end-member model for a style of planetary differentiation and early planetary magmatism. Understanding the internal structure and mantle dynamics of a second planetary body (the Earth being the first) will provide invaluable insights into the dynamical history of the martian mantle and core, the history of the martian magnetic field, and the evolution and structure of primary planetary crusts. The Moon presents the best opportunity to geochemically characterize early fundamental processes of a planetary body of substantial size, including the early differentiation into component parts, the production of an early crust, and the genesis of basalts from various mantle depths. Much of the first billion years of planetary geochemical evolution is not available on Earth. In this regard the Moon and Earth represent end-member bodies in that the Moon reveals early geochemical processes, whereas the Earth is a continually active planet. Mars probably represents an intermediate case.
B. Evolution of Planetary Surfaces: Some surface modification processes will be very similar for the Moon and Mars, and others will differ due to the presence of fluid erosion and chemical weathering on Mars. The Moon retains the history of the early impact environment of the inner solar system, at the time when life may have first arisen on the Earth and perhaps Mars. Understanding the character of the impact history of the inner solar system from 4.5-3.8 Ga is fundamental to reconstructing the planetary surface environments under which life arose, especially determining whether or not there was a "late cataclysm" or spike in impact cratering at 3.9 Ga. Further, the early impact history played a role in the early atmosphere, early tectonics, and the delivery of volatiles. All of these are tied to the important Mars theme of "follow the water". Also, impact history may have a role in planetary asymmetry that is relevant to understanding both the Moon and Mars.
Establishing a well-defined impact flux for the Earth-Moon system for the last 3.8 Ga is a step in better understanding the impact flux on Mars. Such an understanding will help to construct timelines for erosional, depositional, and volcanic features on Mars. Further, minor spikes in impact flux that have been suggested for the Earth-Moon system during this period of time may have been experienced by Mars. This clearly had an influence on evolution of life in the Earth-Moon system. Is it relevant for Mars?
C. Record of Volatile Evolution and Behavior: As Mars and the Moon are at nearly opposite ends of the volatile spectrum for rocky planets, most of the volatile science studies to be conducted on Mars are not possible on the Moon. There are several special cases where the study of lunar volatiles may be relevant to Mars. One example is "energetic particles", whose composition and interaction have been well studied on the Moon and whose study on Mars will probably be limited to determination of near-surface exposure histories. The characterization and exploitation of possible water ice at the lunar poles may be important as a resource for human exploration. In addition, it provides insight into the transport of volatiles on airless planetary bodies. Another special case is the nature of lunar endogenic volatiles that provide insights into the nature of volatile reservoirs in early planetary mantles.
D. Astrobiology: Astrobiology is the quest to understand how habitable planets form and how inhabited worlds evolve, as well as the prospects for life beyond the Earth. Therefore, astrobiology research questions provide many linkages between lunar exploration and Mars science goals. Historically, the Moon preserves unique information about events and processes that have affected the habitability of the entire inner Solar System, including early Mars. Such events include impact chronology (especially during the first billion years), the composition of large impactors and interplanetary dust particle (IDP) flux, the delivery of exogenous volatiles and organics molecules, history of solar activity (solar wind; flares) and the occurrence of nearby supernovae and gamma ray burst (GRB) events. The record of such events is obscured on Earth. Although it is somewhat better preserved on Mars, the lunar record is much more accessible. Hence, the Moon is the ideal place to improve our understanding of some of these events.
Fulfilling many of the scientific goals associated with these Moon-Mars linkages requires the development and utilization of instrumentation that is much more technologically complex than used by Apollo or current Mars exploration missions. Deploying (either robotically or by humans) and maintaining a long-lived and highly sensitive geophysical network on the Moon is relevant to deploying such a network on Mars. The sampling of diverse and environmentally hostile terrains on both the Moon and Mars is important for all themes listed above. Development of sample collection strategies that extend the capabilities of humans through robotics is critical. The development of deep drilling technologies provides 1) access to regions that are unexplored by surface studies and 2) links between the surface and the deep planetary interior.
The MFLO-SAG was not able to identify any significant gaps in the form of objectives of importance to Mars that are not present in the draft list of lunar objectives.
4.7 Mars as a Core Theme for the Lunar Program
The MFLO team considered several different programmatic options to achieve the goal of keeping Mars exploration in the forefront of the lunar program. Since the lunar program will serve as a precursor to Mars exploration, it is important that the lunar program architecture be consistent with achieving the needs of a Mars precursor program.
The options considered for keeping Mars as a signpost out in front of the lunar program included:
The MFLO SAG consensus regarding the best way to ensure that the lunar program is designed for maximum relevancy to Mars exploration is to leave Mars as a core theme within the lunar program. Considering Mars as a core theme within the lunar program helps to keep the relevancy of the lunar objectives over a broad range of topics consistent with the notion of utilizing the lunar program as a precursor for Mars exploration. Additionally, using Mars exploration as a prioritization criterion for the lunar objectives will also help ensure the maximum utility of the lunar program for future Mars exploration.
Beaty, D.W., Snook, K., Allen, C.C., Eppler, D., Farrell, W.M., Heldmann, J., Metzger, P., Peach, L., Wagner, S.A., and Zeitlin, C., (2005). An Analysis of the Precursor Measurements of Mars Needed to Reduce the Risk of the First Human Missions to Mars. Unpublished white paper, 77 p, posted June, 2005 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag.jpl.nasa.gov/reports/index.html.
Hinners, N.W., Braun, R.D., Joosten, K.B., Kohlhase, C.E., and Powell, R.W., (2005), Report of the MEPAG Mars Human Precursor Science Steering Group Technology Demonstration and Infrastructure Emplacement (TI) Sub-Group, 24 p. document posted July, 2005 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag.jpl.nasa.gov/reports/index.html.
MEPAG (2006). Mars Scientific Goals, Objectives, Investigations, and Priorities: 2006, J. Grant, ed., 31 p. white paper posted February, 2006 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag.jpl.nasa.gov/reports/index.html.
Shearer, C., Beaty, D.W., Anbar, A.D., Banerdt, B., Bogard, D., Campbell, B.A., Duke, M., Gaddis, L., Jolliff, B., Lentz, R.C.F., McKay, D., Neumann, G., Papanastassiou, D., Phillips, R., Plescia, J., and Wadhwa, M. (2004). Findings of the Moon_Mars Science Linkage Science Steering Group. Unpublished white paper, 29 p, posted October, 2004 by the Mars Exploration Program Analysis Group (MEPAG) at http://mepag/reports/index.html.
Space Studies Board (2002). Safe on Mars: Precursor Measurements Necessary to Support Human Operations on the Martian Surface. National Research Council, National Academy Press, Washington, DC.
Appendix 1 and Appendix 2 list specific lunar objectives with a perceived relevance to Mars exploration in terms of preparation for humans and science linkages, respectively. The charts also indicate the relevance assessments regarding Mars for each lunar objective. Note that these charts only contain those lunar objectives with a perceived relevance to Mars exploration and other lunar objectives with no perceived relevance to Mars are not listed here.
The information contained within the charts (Appendix 1 and Appendix 2) is as follows. The "Objective ID Number" references the specific objective originally listed in the draft lunar objectives. The "Name" column describes this objective in more detail. Within the "Name" category, cells in green represent the original text describing the lunar objective while cells in blue were rewritten by the MFLO SAG to provide more relevance to Mars. The "Prepare for Mars Priority" (Appendix 1) and "Relevance to Understanding Mars" (Appendix 2) columns indicate a high (H), medium (M), or (L) relevance to Mars exploration (see detailed explanation of ranking definitions in Section 4.1). The "Discussion" column captures the rationale of the MLFO SAG regarding the assessment of each lunar objective.
Appendix 3 is a list of acronyms used in this paper.
SpaceRef Note: Download Appendix 1 and 2 as a PDF file
APPENDIX 1: Lunar objectives with relevance to preparation for human Mars exploration.
APPENDIX 2: Lunar objectives with relevance to understanding Mars
APPENDIX 3. Acronym list
[NW1]need to check this statement; Velcro is a system of hooks and barbs. Has someone done studies on lunar dust to understand this 'stickiness'? ??
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