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1.INTRODUCTIONThe Hubble Space Telescope (HST) has for decades provided some of the most valuable insights into the science of astronomy and astrophysics. Similarly the other great astronomical observatories of the past, Chandra, Spitzer, and Compton have contributed immensely to advancing science and our general knowledge of the universe. These large observatories are the some of the most productive “science machines” ever built. This tradition is expected to continue with the James Webb Space Telescope (JWST) when it is launched in 2018. Astrophysics, whether space based or ground based, is continuously driven to larger and larger apertures in order to explore the distant universe or study faint nearby objects such as exoplanets. Unfortunately but not unexpectedly, these great observatories have also been some of the most costly observatories built by NASA. All of these observatories were threatened with cancellation during development due to cost and schedule overruns, a risk also run by NASA flagship missions outside of astrophysics. The on-orbit performance of HST and the performance expectations for JWST have also clearly established the value, scientific and otherwise, of a new and much larger space observatory covering at least the spectral region from the ultraviolet (UV) through the visible (VIS) to the near infrared (NIR). But the future great observatories will have to be built at a time when, for the foreseeable future, NASA budgets are almost certain to be flat or declining. There have been a number of studies of the mission concepts and technologies for larger space observatories, identified as the Advanced Technology Large Aperture Space Telescope (ATLAST)1,2 and the Modular Assembled Space Telescope (MAST)3. These studies have established the technical feasibility of a number of sizes and designs, and the science utility will be discussed in a few paragraphs. Costing factors have been addressed in other studies4,5. The general conclusion of these studies is the fiscal incompatibility of the required large space telescope designs with the expected NASA budgets referred to in the preceding paragraph. An independent, and more detailed, analysis of this same conundrum, reaching the same conclusions regarding the incompatibility of the fiscal and the technical can be found in Arenberg et al6 in paper 9143-36 at this conference. It is therefore essential to identify and implement a new development concept for large space telescopes that increases their affordability while, over time, providing the much improved resolution and light collecting power required to do the forefront science. It is our contention that, partly due to the annual funding cycle that NASA must employ, the root cause of the cancellation or delay risks run by a Flagship class mission is due to the annual cost of the mission. When this cost consumes too great a percentage of the yearly NASA budget it threatens all other missions, even those that are operating successfully and may offer an extended lifetime of great scientific merit. With multiple missions of all sizes threatened, the science community and NASA begin to consider draconic measures to reduce the annual cost of the Flagship mission: i.e., cancellation or program down-sizing and/or extension. Potentially, it may be possible to overcome most of these programmatic risks by implementing some of their characteristics immediately in the initial stages of the program, effectively trading longer time to ultimate completion for greater affordability. Specifically, design, construction, and launch of the space telescope will be conducted in a number of stages, each producing a complete telescope fully capable of valuable scientific observations. Stage 1 will form the core of the observatory and will provide selected improvements upon systems operating at the planned launch date. Succeeding Stages will build upon the Stage 1 observatory in several year increments (nominally about 5 years between launches), and will add mirrors, structures, and instruments to the Stage 1 telescope. A full Flagship capability† will be achieved by Stage 3 (details of one possible approach are provided in the Reference Concept section below). Future, even more capable Stages are, of course, possible, but are not addressed in this paper. This is the concept for the Evolvable Space Telescope (EST). 2.EST PROGRAMMATICSAs noted above, the development and deployment of EST will be conducted in a number of Stages, each of increasing capability, culminating in the full capability of an ATLAST observatory. Programmatically, this strategy will succeed if and only if the annual budget for each Stage is constrained below a reasonable fraction‡ of the NASA astrophysics budget, and that fraction is well known to the astrophysics community. Thus, the EST programmatic strategy is, to a large extent, a design-to-annual-cost strategy combined with a “science-as-you go” strategy that is coupled with the requirements established by the principal science drivers. The annual cost target, still to be developed, will need to be based upon two principal factors: sufficiency for EST to achieve scientific viability with early flight stages so that the community will have continuing access to essential observational data, but low enough in cost to enable significant progress in astrophysics missions in other science regions. The program will be structured with a modest cost, extended development in mind, enabling steady progress while capitalizing upon economies of scale as possible. Perhaps most importantly, maintaining a conservative but steady expenditure rate will protect EST from the effects of downsizing, which include inefficient use of personnel and equipment and increased expenditures in later program stages. As an illustrative example, if all three Stages can be acquired and deployed within a planned period of 15 years and the annual spend rate maintained at approximately $400M (current year dollars), a full ATLAST capability will be deployed for a total cost of ~$8B. Assuming that the total available for NASA astrophysics remains at about $1,200M as it has for most of the past decade, this will still leave financial room for other, extensive astrophysics systems development. It should also be noted that the only costs that will be addressed in the proposed EST study will be those to be financed directly and managed by NASA. This rule is intended primarily to reduce program turbulence over its long lifetime. Other organizations, national or international, public or private, may be able to make major contributions to EST once it enters development, but a central management will be essential to maintaining the viability of the program. 3.SCIENCE DRIVERSA fundamental design rule for EST will be the requirement that each Stage, beginning with Stage 1 itself, will be designed to contribute significant science beyond that which constitutes the then current state-of-knowledge in important sub-fields of astronomy. The specifics of this requirement will be detailed in the design studies for the separate Stages but, as a minimum, will be based upon the science drivers used in the ATLAST studies by Green, Postman and others1,7,8,9 and a few examples are shown in Figure 1. It will be necessary to derive intermediate science requirements that contribute to the attainment of these goals using the lesser capabilities of the intermediate stages of EST. These science drivers, at all levels of the EST program, will address multiple questions, many of which are organized around three topics which are paraphrased here and may be reviewed in detail in the cited references for ATLAST and MAST.
Other topics, such as solar system physics (planetary and small body) may be addressed by EST as well. Indeed, EST can be expected to follow the path of almost all early astronomical observatories, uncovering and resolving new issues that cannot be foreseen at this time and generating needs for more and different observations from still newer observatories over time. 4.MISSION CONCEPTThe preceding introductory sections defined the Evolvable Space Telescope (EST), outlined its value, rationale, and timeliness (scientific and otherwise), and sketched the approach and expected products of the feasibility study needed as the first step towards an EST. This section will outline important aspects of the programmatic approach and environment, while later sections will present more details of the trade space accessible to the general concept, outline near term studies needed to begin assessment of the concept, provide an example of a generic design to suggest the sort of detailed study that will be needed, and describe the in-space servicing capabilities and technologies expected to be available at least through Stage 1 of EST. 4.1OrbitEST is envisioned as a Sun-Earth L2 (SEL2) based observatory. This location offers an excellent observation environment, will be well understood from years of JWST performance at SEL2, and has relatively low delta-V requirements if we need to move the observatory to a convenient nearer Earth location or easier access from Earth than other possible orbits, if the servicing is to be done at SEL2. 4.2Measures of MeritAs a very large space telescope, ultimately similar in capability to ATLAST, EST will be subject to a large number of measures of merit, most notably in terms of performance and affordability. These will be addressed in detail over the extended study, but there are three that particularly distinguish the EST mission concept: evolvability, adaptability, and serviceability.
4.3Budget FactorsAs noted in the previous section, it will be essential for EST to be adaptable under changing budget conditions, since the budget environment is and will remain highly volatile and adjustable on a short-term basis (generally annually). The study will employ several assumptions:
In addition, a small number of budgetary requirements will be imposed on the output of the study to control the affordability and therefore the feasibility of EST: 4.4Launch CadenceBased upon a 5 meter interior diameter launch shroud, the first Stage is baselined to employ a ~4 meter unit cell (flat-to-flat hexagon). The unit cell can be larger if a larger shroud is available, or smaller if budget conditions worsen. There are several families of possible launch vehicles: ULA (principally Atlas V and Delta IV), the Space-X Falcon 9, and the Ariane 5, for example. The baseline program will consist of Stages 2 and 3 to build on the Stage 1 telescope. These have not as yet been designed, but the goal is a final Stage 3 aperture in the 16 to 20 meter range, with launches occurring at approximately 5- year intervals. Stages beyond 3 are possible, but early concept development will not actively pursue these levels, but will take no actions that will preclude missions as long as 50 to 60 years. 4.5Instrument SuitesEST instruments, beginning with Stage 1, will be mounted in a manner that will enable either a simple replacement of the entire suite or individual instrument replacement. By the time EST is launched we are assuming that the ongoing revolution in astrophysics instruments will continue, particularly in the area of Integral Field Spectrographs and other similar imagery/spectroscopy instruments, and that it is likely that this type of instrument would comprise the “core” general use instrument for EST. In addition we would expect specialized instruments such as starlight suppression systems (starshades or coronagraphs - EST will be starshade compatible) and likely other focused application instruments for specific science goals. These instruments would be selected through a Science Mission Directorate (SMD) competitive process based upon both the prioritized science drivers and the technological maturity of the relevant instruments at the time of the mission. For the purpose of this study we are simply assuming that there will be a core instrument suite for EST with ancillary “specialized” instruments. 4.6OutreachJust as with the HST and JWST, EST will be a key element in NASA astrophysics outreach, both directly to the public and educational establishments and to senior government officials. It will be the prominent space telescope that is most readily understood by all members of the public, and will therefore provide key support for other science missions. They will watch it be launched and evolve, and watch the science return become ever more spectacular. Since EST, and some of its possible support elements, can provide significant support to both human exploration and planetary science missions, it will be essential to establish a firm working relationship at least with the Planetary Sciences Division of SMD and with the Human Exploration and Operations Mission Directorate (HEOMD). 5.EST TRADE SPACEThe preliminary concept study will need to make a large number of technical tradeoffs in order to define a basic reference design for future in-depth study. Although a totally complete set cannot be established in the early stages, these tradeoffs will necessarily include those listed in the following table. Some tradeoffs that would be included in a totally bottoms-up study have already been made, and their results are included in the assumptions. Two of these are:
Note that this table does not address tradeoffs among instruments, which will have to be considered in later work once the telescope (and spacecraft) designs are more settled for each Stage. These analyses will be largely based upon detailed considerations of the primary science drivers, with allowances made for the flexibility needed to address unexpected scientific questions and opportunities.
6.THE INITIAL EST STUDYAs with any study of a new mission concept, the first step must be to decide precisely what to study in detail and how to proceed with those detailed assessments. There is a natural flow down, possibly involving one or more iterative cycles as later steps encounter flaws in earlier conclusions that this study will follow.
As the EST Mission Concept Study develops, it should provide a source of information and insight that will help to both build community interest (including the scientific, government, and public communities) and as a construct for all of these communities to discuss, debate, and refine. Much of the discussion can be expected to revolve around evolving Design Reference Concepts. A simplified, preliminary concept is outlined in the following section. 7.DESIGN REFERENCE CONCEPTThis paper is not intended to provide an extensive list of design concepts that could be used to implement the Evolvable Space Telescope architectural philosophy. However, the authors believe that comprehension of this design philosophy will be assisted through discussion of at least one elementary example as a reference. The details of the assembly of the EST Primary Mirror Assembly (PMA) are represented in Figure 2. For comparative purposes, this paper assumes that all the hexagonal segments shown are ~4 meters flat-to-flat, or approximately 4.5 meters point-to-point, although these dimensions are purely illustrative. The EST approach can accommodate any segment size, but the telescope aperture at each stage will of course scale with the segment size. Figure 2 is intended to represent only the underlying approach to be employed in EST, and not a specific implementation of that approach. The details of possible implementations will be worked out in detailed studies to follow this initial work, but some specifics are included to provide a relatively intuitive insight into the EST concept. This discussion is based upon Figure 2, which represents one possible configuration of the primary mirror in each of the three Stages:
8.SERVICING CONSIDERATIONSAs implied under the discussion of the principle measures of merit in the Mission Concept section, serviceability will be a key to the success of the Evolvable Space Telescope, particularly given the extended operational lifetime expected of the observatory. Two principal technologies are developing rapidly that will enable this critical capability: robotics/telerobotics and multiple space platforms that can form the basis for servicing operations of all types. 8.1Robotics/TeleroboticsThe capability of human/machine and autonomous machine systems to perform a wide variety of mechanical functions is one of the most conspicuous features of current technology. This is true in space as well as within the biosphere, despite the arduous conditions faced there, as most visibly demonstrated at the International Space Station (ISS) and on the surface of Mars, among others. These capabilities provide the foundation needed to enable the assembly and servicing of systems such as EST, regardless of their specific locations. Performance of these functions can be expected to become increasingly the responsibility of autonomous robots but, with the availability of an increasing variety of manned systems, human presence will continue to provide support both to reduce temporal latency and to assume control when unforeseeable circumstances arise. 8.2Service PlatformsImplementation of an effective in-space infrastructure is in its early stages, but is proceeding with increasing rapidity, driven by the ISS and the variety of deep space missions being planned and evaluated. Systems range in size from the ISS down to electronic chip size, and are in all stages of development. A complete discussion is well out of scope of this paper, but a few relevant points are outlined in the following:
9.SUMMARY9.1Summary of Specific ObservationsIn the process of developing this paper, several specific conclusions have become apparent to the authors. Some of these are presented in the body of the text, but they are summarized in the following:
9.2Continuing ActivitiesThe principal remaining activity for 2014 will be to finish (by November) the mission concept study reported in this paper. In particular, by the completion of this phase of the study, we plan to have:
9.3General SummaryThe study team has developed a preliminary concept for an Evolvable Space Telescope (EST) architecture that can enable the development and operation of very large (> 14 meters) space observatories in an era of flat budgets. The architecture is characterized by:
ACKNOWLEDGEMENTSThe authors would like to acknowledge strong support and internal funding from Northrop Grumman Aerospace Systems and very helpful comments, suggestions, and criticisms from a variety of people, including Jonathan Arenberg, Alberto Conti, Lee Feinberg, Marc Postman, Theodore Swanson, and Harley Thronson. REFERENCES, “National Aeronautics and Space Administration, ATLAST Mission Concept Study,”
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