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AAWSAP DIRD, Laser Lightcraft Nanosatellites, November 2010

U.S. Department of War · 2010-11-01 · 77 pages · text from the file's own layer

This Defense Intelligence Reference Document (DIA-08-1011-001), dated 1 November 2010, was prepared by the Defense Intelligence Agency's Defense Warning Office under the Advanced Aerospace Weapon System Applications program. It covers nanosatellite technologies, laser Lightcraft propulsion, a weapon mission selection study and a multi-megawatt laser study. The author recommends that the Department of Defense, working with NASA, bring laser Lightcraft propulsion research back to the United States and restart the Air Force X-50LR test flight program.

From the source:Release of 2026-09-18 Incident: 11/1/10, Las Vegas, Nevada. Released with redactions. This document is a Defense Intelligence Reference Document (DIRD), a technical reference format used by the Defense Intelligence Agency (DIA) to capture baseline knowledge on a specific topic for later analytic use. DIRDs are best understood as reference and synthesis products rather than as original research. It is one of 38 DIRDs produced under the Advanced Aerospace Weapon System Applications Program (AAWSAP) between 2009 and 2011. Because AAWSAP’s scope permitted a broad range of supporting topics, not every DIRD in the series directly concerns aerospace systems or future threat assessment. The following summary reflects the DIRD’s scope and framing at the time of writing and should not be read as implying current validation of the concepts discussed. This DIRD examines laser-propelled “Lightcraft” as a possible low-cost method to launch very small satellites into low Earth orbit by using a remote high-energy laser to supply most of the propulsion energy rather than relying entirely on onboard energy sources. The report combines a survey of nanosatellite trends with a review of “Lightcraft” propulsion concepts, vehicle design, beam-control requirements, and mission studies, and argues that the most promising application is the launch of nano- or pico-satellites, especially Earth- and space-observing payloads of a few kilograms or less. It presents the concept as potentially much cheaper than conventional multistage rockets for very small payloads, while also noting significant practical constraints including strict beam-riding geometry, atmospheric losses, demanding pointing and adaptive-optics requirements, and heavy dependence on large ground-, sea-, or air-based laser infrastructure. Overall, the document presents laser “Lightcraft” as a technically plausible launch concept whose attractiveness depends on whether the supporting laser and beam-control system can be made reliable and economical at operational scale.

  • p. 8 …The sensor must be capable of detecting Earth over a range of orbital radii with a…
  • p. 17 …For the purpose of this report, we envision a Lightcraft Earth-to-Orbit (ETO) transportation system…
  • p. 23 …kg, and 1.0 kg into low Earth orbit (LEO). And preliminary life-cycle cost estimates…
  • p. 34 …not only placing nanosats into LEO at low cost (Figure 14 ), but also for performing much…
  • p. 42 …Each picosat is gravity gradient stable, has a dipole array facing Earth, and a broader beam…
  • p. 43 …orrlCIAE USE 014Lf pushbroom scanning mode for complete Earth coverage rather than only sampling coverage. The…
  • p. 72 …The system is single-stage-to-orbit and completely reusable with no onboard propellant required (the…
  • p. 75 …J., et al. (1991), "System Requirements for Low-Earth-Orbit Launch Using Laser Propulsion," in Proc…
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These array functions can be made coherent over very great distances. RF antennas
with sizes of hundreds of kilometers and optical telescopes of hundreds of meters
diameter can be formed. These systems can enable new capabilities not possible with
single spacecraft either acting alone, as a proliferated but non-coherent constellation,
or as relays for each other. Formed of nanosats and picosats, such swarms will contain
so many spacecraft that the economics of true mass production will come into play in
space for the first time, greatly reducing the cost of producing the system. In addition,
these systems feature the advantages of truly distributed satellite systems, including
fault tolerance, robustness, survivability, reconfigurability by software, and the ability
to be incrementally emplaced and upgraded as budgets are available.
These swarms can be implemented in a cost effective manner using laser propulsion for
both launch and orbital insertion. However, the system designs described in the
following sections are flexible enough to allow for the use of alternative conventional
launch vehicle technologies. The technologies to produce these swarms and their
constituent nanosats or picosats probably can be demonstrated by 2015 and deployed
in space by 2020.
The following concepts were provided via the voluminous research notes, lectures, and
briefings provided courtesy of I. Bekey.
ROTATING PICOSAT SWARM ARRAY RADIO FREQUENCY COLLECTOR
An unconventional, large sparse antenna array RF collector spacecraft with a small
surface footprint even when deployed in geosynchronous Earth orbit (GEO) separates
different sources in proximity and also detects weak signals. Its implementation would
result in a highly desirable, long dwell RF emitter detection capability.
At the heart of this system is a large antenna that is formed by a swarm of tiny
elements that make up the lens of a space-fed array with no structure. The antenna is
a sparse, self-cohering array formed from a large number of picosats rotating (in
relative coordinates) in a plane around a central orbital point in GEO. The picosats are
self-contained repeater spacecraft. Each one receives the ground signal, delays it, and
retransmits the signal so that it arrives at the feeds at the same time as a direct ray
through the center of the array. The time delay of each picosat is self computed based
on its location in the swarm, as measured by a local differential global positioning
system (DGPS)-like navigation signal, to compensate for its deviation from its assigned
ideal location. Each picosat digitizes, delays, frequency shifts, and retransmits its
received signals independently, causing an in-phase composite signal from the ground
to be received at the feeds.
The relative positions of these picosat elements change slowly, and only small and
infrequent propulsive maneuvers are needed for constellation maintenance. A tether
along the local vertical at the central point holds the receivers and DGPS-like reference
at the focus against a counterweight. A pseudorandom distribution of the picosats
suppresses the antenna grating lobes, and intensive computation greatly reduces much
of the remaining sidelobes, creates multiple beams, and steers the ensemble of the
individual beams anywhere on Earth. The antenna system will function with far fewer
elements as a more sparse array, though with limited sensitivity. This system can be
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Official release, from the pursue collection. The PDF is mirrored here; the original link is above. 77 pages are in the text index: search them above, or from the library's search.