Project engineers and scientists are going full-bore ahead. The funding is in the federal budget. Pretty much a done deal.
I want to know about this dark planet that Art Bell's recent guests/callers keep talking about.
The use of parametric cost estimation is helping engineers at NASA's Marshall Space Flight Center (MSFC) make early cost estimates for a proposed mission to Pluto. Cost estimates are critical in the early phases of projects in order to obtain budgetary approval and evaluate various approaches early in the life of the proposed program when they can have the most impact on its cost. MSFC uses a cost model developed by the government especially for aerospace program costs but it works at a very high level so it often isn't very useful for comparing alternative approaches at the subsystem level and below. In recent years, MSFC has supplemented these estimates with those provided by a commercial software package that offers the ability to create a model that is as detailed as desired and provides an extensive database that quickly generates system, subsystem and component cost estimates based on real-world experience. This approach proved very useful in providing early estimates of the cost of making the first flyby of the last unexplored planet as well as the Kuiper Belt, which lies beyond it and hasn't changed much since the solar system was created.
Pluto is the only planet in our Solar System not yet viewed close-up by spacecraft, and given its great distance and tiny size, study of the planet continues to challenge and extend the skills of planetary astronomers. Most of what we know about Pluto we have learned since the late 1970s. Many of the key questions about Pluto and its satellite Charon await the close-up observation of a space flight mission. Beyond Pluto lies the recently-discovered Kuiper Belt of "ice dwarfs" or minor planets. NASA originally planned to launch the Pluto-Kuiper Express in 2004 to conduct the first reconnaissance of Pluto and its large moon Charon with low mass flyby spacecraft, using advanced technologies to serve as a pathfinder for low cost exploration of the outer Solar System. The scientific goals of the mission were to 1) characterize the global geology and geomorphology of Pluto and Charon, imaging both sides of each 2) map the surface composition and 3) characterize Pluto's neutral atmosphere, including composition, thermal structure, and aerosol particles.
Need for a lower cost approach
Missions to the outer Solar System are by nature complex and expensive and it soon became clear that the funding was inadequate to launch the series of missions NASA had hoped for during the next decade. Last fall, NASA Headquarters announced that - because both the Pluto-Kuiper Express Mission and the Europa Orbiter mission to follow it were now certain to cost almost twice as much as the Jet Propulsion Laboratory had first suggested - the 2004 Pluto mission would be cancelled, to ensure that there were enough funds to launch the Europa mission in 2007. Europa is the subject of great scientific interest because of the possibility that it may hold life, but the Pluto cancellation nevertheless disappointed the planetary science community. They pointed out that if the 2004 launch opportunity is missed there can be no gravity-assist flyby of Jupiter to catapult them out to Pluto and that the Europa mission, on the other hand, could tolerate a launch delay without any loss of science. As a result, NASA Headquarters began soliciting proposals for a simpler, less expensive Pluto-Kuiper Belt mission, ideally one that could be flown for under $500 million.
As the request for proposals put it: "Every aspect of the investigation must reflect a commitment to mission success while keeping total costs as low as possible. Consequently, the investigation should be designed to emphasize mission success within the specified cost and schedule constraints by incorporating sufficient cost, schedule, and design margins, reserves, and content resiliency." MSFC with partners Teledyne Brown Engineering (TBE), Los Alamos National Laboratory (LANL), and NASA Glenn Research Center (GRC) put together a team of engineers from the disciplines involved, including structural, thermal control, propulsion, and avionics, in an effort to meet this challenge. These engineers developed rough order of magnitude subsystem level design specifications, in many cases developing multiple alternative designs. The MSFC/TBE/LANL/GRC design efforts resulted in a Pluto Orbiter which far surpassed the original specification for a flyby mission. Their work was turned over to the engineering cost group, the group that is responsible for developing cost estimates of various proposals for accomplishing this mission. NASA has used parametric costing methods for about three decades. One tool that they used on this project is the NASA/Air Force Cost Model (NAFCOM96) which is an innovative tool for developing a high level estimate of aerospace program costs.
SEER-H has approximately 40 knowledge bases for electronic elements and for mechanical. While SEER-H is primarily focused on the development process, it also includes manufacturing cost estimation capabilities for low volume production. The program is sensitive to the difference between mechanical and electrical elements and between labor and materials costs. It also bases the price of individual PCBs on their number of components rather than their weight, an approach that usually provides more realistic results. SEER-H allows the user to choose the probability level of estimates, and set different levels for each portion of the project. It also provides detailed sensitivity analysis features that make it possible to determine the impact of adjusting specific project factors. This feature, for instance, makes it possible to quickly estimate the impact on cost if a project schedule is compressed by two months. This software package reduces the learning curve by avoiding the use of less-than-obvious adjustments in order to present the estimating objective more clearly.