Engineering topics
Cutts, James
Publications and source records attributed to Cutts, James.
Guidance, Navigation, and Control Technology Assessment for Future Planetary Science Missions
Future planetary explorations envisioned by the National Research Council's (NRC's) report titled Vision and Voyages for Planetary Science in the Decade 2013-2022, developed for NASA Science Mission Directorate (SMD) Planetary Science Division (PSD), seek to reach targets of broad scientific interest across the solar system. This goal requires new capabilities such as innovative interplanetary trajectories, precision landing, operation in close proximity to targets, precision pointing, multiple collaborating spacecraft, multiple target tours, and advanced robotic surface exploration. Advancements in Guidance, Navigation, and Control (GN&C) and Mission Design in the areas of software, algorithm development and sensors will be necessary to accomplish these future missions. This paper summarizes the key GN&C and mission design capabilities and technologies needed for future missions pursuing SMD PSD's scientific goals.
Rapid Cost Assessment of Space Mission Concepts through Application of Complexity Indices
In 2005, the Solar System Exploration Strategic Roadmap Conmrittee (chartered by NASA to develop the roadmap for Solar System Exploration Missions for the coming decades) found itself posed with the difficult problem of sorting through several mission concepts and determining their relative costs. While detailed mission studies are the normal approach to costing, neither the budget nor schedule allotted to the conmrittee could support such studies. Members of the Jet Propulsion Laboratory (JPL) supporting the conmrittee were given the challenge of developing a semi-quantitative approach that could provide the relative costs of these missions, without requiring an in depth study of the missions. In response to this challenge, a rapid cost assessment methodology based on a set of mission cost/complexity indexes was developed. This methodology also underwent two separate validations, one comparing its results when applied to historical missions, and another comparing its estimates against those of veteran space mission managers. Remarkably good agreement was achieved, suggesting that this approach provides an effective early indication of space mission costs.
Rapid Cost Assessment of Space Mission Concepts Through Application of Complexity-Based Cost Indices
This slide presentation reviews the development of a rapid cost assessment models for evaluation of exploration missions through the application of complexity based cost indices. In Fall of 2004, NASA began developing 13 documents, known as "strategic roadmaps," intended to outline a strategy for space exploration over the next 30 years. The Third Strategic Roadmap, The Strategic Roadmap for Solar System Exploration, focused on strategy for robotic exploration of the Solar System. Development of the Strategic Roadmap for Solar System Exploration led to the investigation of a large variety of missions. However, the necessity of planning around scientific inquiry and budgetary constraints made it necessary for the roadmap development team to evaluate potential missions not only for scientific return but also cost. Performing detailed cost studies for each of the large number of missions was impractical given the time constraints involved and lack of detailed mission studies; so a method of rapid cost assessment was developed by us to allow preliminary analysis. It has been noted that there is a strong correlation between complexity and cost and schedule of planetary missions. While these correlations were made after missions had been built and flown (successfully or otherwise), it seemed likely that a similar approach could provide at least some relative cost ranking. Cost estimation relationships (CERs) have been developed based on subsystem design choices. These CERs required more detailed information than available, forcing the team to adopt a more high level approach. Costing by analogy has been developed for small satellites, however, planetary exploration missions provide such varying spacecraft requirements that there is a lack of adequately comparable missions that can be used for analogy.
Planning for planetary protection and contamination control : challenges beyond Mars
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Venus Exploration opportunities within NASA's Solar System Exploration roadmap
Science goals to understand the origin, history and environment of Venus have been driving international space exploration missions for over 40 years. Past missions include the Magellan and Pioneer-Venus missions by the US; the Venera program by the USSR; and the Vega missions through international cooperation. Furthermore, the US National Research Council (NRC), in the 2003 Solar System Exploration (SSE) Decadal Survey, identified Venus as a high priority target, thus demonstrating a continuing interest in Earth's sister planet. In response to the NRC recommendation, the 2005 NASA SSE Roadmap included a number of potential Venus missions arching through all mission classes from small Discovery, to medium New Frontiers and to large Flagship class missions. While missions in all of these classes could be designed as orbiters with remote sensing capabilities, the desire for scientific advancements beyond our current knowledge - including what we expect to learn from the ongoing ESA Venus Express mission - point to in-situ exploration of Venus.
(abstract) Searching for Ice and Ocean Biogenic Activity on Europa and Earth
One of the more likely places in the solar system for the existence of extraterrestrial life forms is the jovian moon Europa. It has been postulated that a volcanically heated ocean exists underneath Europa's icy surface. In order to make quantitative measurements of the Europan environment, a lander spacecraft capable of penetrating the surface ice layer by melting through it is proposed. This vehicle, dubbed a
(abstract) Through the Europan Ice: Advanced Lander Mission Options
A variety of options for missions to visit Europa and study it in depth are being discussed. A first reconaissance may be made with an orbiter only. However, detailed examination of any water-ice ocean, particularily to determine the possible existence of biochemical materials, will require landing on and perhaps melting down through the ice itself to directly explore the Europan ocean. A first mission to Europa will attempt to determine whether or not this liquid water exists. Assuming this first mission determined it likely that liquid water did indeed exist, a more sophisticated lander package would be appropriate. This paper will describe strawman designs of this advanced lander as well and will discuss the many opportunities and challences in creating such spacecraft. Work in progress at both Leicester and JPL to further determine cryobot feasibility through numerical modeling and mechanical prototyping will be described.
Workshop proceedings: Information Systems for Space Astrophysics in the 21st Century, volume 1
The Astrophysical Information Systems Workshop was one of the three Integrated Technology Planning workshops. Its objectives were to develop an understanding of future mission requirements for information systems, the potential role of technology in meeting these requirements, and the areas in which NASA investment might have the greatest impact. Workshop participants were briefed on the astrophysical mission set with an emphasis on those missions that drive information systems technology, the existing NASA space-science operations infrastructure, and the ongoing and planned NASA information systems technology programs. Program plans and recommendations were prepared in five technical areas: Mission Planning and Operations; Space-Borne Data Processing; Space-to-Earth Communications; Science Data Systems; and Data Analysis, Integration, and Visualization.
Technology for submillimeter wave remote sensing
NASA's sub-mm wave technology development program addresses emerging possibilities in spaceborne sensor design for what is one of the few unexplored regions of the spectrum, from 1.0 to 0.1 mm wavelengths. Astrophysics, earth atmosphere research and solar system exploration can all benefit from the development of such sensor capabilities. Technology status evaluations are presented for Shottky-diode and SIS mixers, solid state and backward wave oscillators, intermodulation frequency amplifiers, and digital autocorrelator and acoustooptic spectrometers.