Robert Salkeld
Robert Salkeld To estimate a common-based comparison of asteroidal and lunar materials costs, both are here placed on the same program basis as assumed, for the lunar case (ref. 9). That is, Earth launches are assumed to begin in 1985 using the first generation space shuttle (capacity 60 flights/yr), phasing in 1987 to a shuttle -derivative heavy-lift vehicle (SD/HLV) for unmanned cargo (capacity - 80 flights/yr), and finally phasing in 1991 to a second generation passenger-cargo single stage-to-orbit (SSTO) shuttle. Program duration is 10 years (1985-1994), during which about 1 million tons of asteroid material (from the capture of two 1-million-ton asteroids) are returned to the space manufacturing facility (SMF), compared with about 2.4 million tons of lunar materials.
Capture of two asteroids in this time period is based on the estimate of a 5-year out-and-back mission time, and is consistent with the maximumpaced program assumed for the lunar case. Thus, the first generation shuttle launches the asteroid miner and mass driver in sections during 198586, contributing in the process all of its external tanks for mass-driver reaction mass. The SD/HVL then phases in to launch a second miner and mass driver, and all the remaining reaction mass for two asteroid expeditions as well as chemical orbital transfer vehicles (OTV) and their propellants for establishing the SMF, during 1987-89. The first expedition leaves low-Earth orbit (LEO) early in 1987 and returns in 1992. When it has successfully reached its target and is homeward bound 1989, the second leaves to return in 1994. The SD/HVL, SSTO and OTV establish the SMF in 1989-92 so that it is ready to process the first returning asteroid. The chemical OTV is used for SMF rather than a smaller mass driver, to avoid a second mass driver development program, and because the OTV is required in any case for SMF personnel transfer. Use of a mass driver for deploying SMF would reduce total program cost only slightly.
The results of preliminary costing of the asteroid and lunar programs are summarized in table 3. A possible requirement for an LEO station has been included as one consideration, to maintain as comparable basis as possible with the lunar case. Several observations may be made:
Asteroidal, 1.1X106 tons delivered to SMF |
Lunar, 2.4X106 tons to SMF |
|||
No | Yes | Yes | ||
Total program, $ billions |
RDT & E included |
27.7 | 31.2 | 57.0 |
RDT & E excluded |
11.9 | 12.6 | 37.0 | |
Per kg delivered, &/kg |
RDT & E included |
25.2 | 28.4 | 23.8 |
RDT & E excluded |
10.8 | 11.5 | 15.4 |
Curator: Al Globus If you find any errors on this page contact Al Globus. |
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