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Modular Laser Launch Architecture: 
Analysis and Beam Module Design 
NIAC Phase I Fellows Meeting 
24 March 2004 
Jordin T. Kare 
Kare Technical Consulting 
908 15th Ave. East 
Seattle, WA 98112 
206-323-0795 
jtkare@attglobal.net 
Revised 3/23/04 
Kare Technical Consulting 3/23/04 1
The Laser Launch Concept 
Leave The Hard Parts 
On The Ground! 
Launch many small payloads 
on demand -- up to 10 per hour Leave The Hard Parts 
! 
On The Ground! 
Laser and Beam Projector 
• Big 
• Heavy 
• Expensive 
• STATIONARY 
Vehicle 
• Small 
• Simple 
• Cheap 
• Inert 
30,000 launches per year x 100 kg 
= 3000 Metric tons per year!! 
Rule of Thumb: 
1 kg of payload 
per MWof laser 
Kare Technical Consulting 3/23/04 2
Why Laser Launch? 
• Massive launch capacity 
– A 100-kg launcher can put 3000 tons per year in LEO 
• Very low marginal cost to orbit 
– Electricity, vehicle, and propellant easily <$100/lb 
• Potentially low total cost to orbit 
– If the system is cheap enough to buy and run, and… 
– If there are enough payloads to launch 
• Maximum safety -- no stored energy on vehicles 
– Enables all-azimuth launch from any site 
• High reliability, easy to maintain 
– The hard parts stay on the ground 
– Vehicles are simple, mass-produced, and testable 
• Ultimate launch-on-demand -- FedEx to space 
Kare Technical Consulting 3/23/04 3
Pulsed Laser Propulsion Works... 
Kare Technical Consulting 3/23/04 4
… But Has The Same Problems As Everything Else 
• Development cost 
– Even at $10/watt, $1 Billion for 100 MW 
• Technical risk 
– You don’t know if it will work at all without spending $$$ 
• In this case, for a multi-megawatt test laser 
• Programmatic risk 
– You don’t know what it will actually cost until you’ve built it 
• Big lasers have had cost/schedule/performance problems for 40 
years! 
– Reality is always different from theory; operational systems 
are always different from prototypes 
Kare Technical Consulting 3/23/04 5
The Heat Exchanger Thruster 
Primary (H2) Propellant Tank 
Pump 
(optional) 
Lightweight 
Heat Exchanger 
Secondary 
(Dense) 
Propellant 
Nozzle(s) 
Laser 
Beam 
Dense propellant 
injection trades lower Isp 
for higher thrust, 
matches exhaust velocity 
to vehicle velocity 
• Exhaust Temperature ~1000 C 
• Specific Impulse ~600 seconds 
Kare Technical Consulting 3/23/04 6
Heat Exchanger Thruster Advantages 
• Works with any laser wavelength and pulse format 
• Nearly 100% efficient 
– high absorption, negligible reradiation 
• Simple to design 
– Steady flow 
– Simple propellant properties (especially for H2) 
• Simple to build 
– Electroplating technique demonstrated at LLNL 
– Modular design scales easily to any area 
• Simple to test 
– Works with any radiant source; doesn’t even need a laser 
Kare Technical Consulting 3/23/04 7
Current 100 MW Vehicle Concept 
Dense propellant tanks Avionics 
! 
Drop tank 
Stage 2 tank 
Total H2 tank volume ~25 m3 Payload 
Aeroshell 
Pressurant tank 
Drop tank 
! 
~6 meters 
! 
Heat exchanger 
(25 m2) 
Kare Technical Consulting 3/23/04 8
What Do We Do About The #%&@ Laser? 
• Lasers cost too much 
– Absolute cheapest high power laser is $20-50/watt 
• CO2 electric discharge, with very poor beam quality 
• Should scale to 100 MW, but not easily or cheaply 
– Stay-on-all-day lasers above ~10 kW don’t exist 
• AVLIS copper vapor lasers were 10 kW total, at a cost of 
>>$1000/watt 
• No one will pay to develop a large laser 
– Too many bad memories: CO2, HF/DF, Excimer, FEL… 
– “There are liars, damn liars, and laser builders” 
Kare Technical Consulting 3/23/04 9
Laser Diode Arrays 
• >50% efficient DC to Light at ~800 nm 
• 10,000 hour lifetime (60,000 launches!) CW operation 
• Run on DC current; water cooled 
• Commercially available from multiple vendors 
• $4 - $10/watt NOW 
• $2/watt in a few years in 
100 MW quantities 
• BUT -- not coherent; not 
high enough radiance to 
beam 500 km 
A 1200 Watt CW “stack” 
from Nuvonyx, Inc. -- 
a catalog item! 
A 1200 Watt CW “stack” 
from Nuvonyx, Inc. -- 
a catalog item! 
1 cm 
Kare Technical Consulting 3/23/04 10
The Beam Module Concept 
• DON’T build one big laser and beam director 
• Build MANY small “Beam Modules” 
– Completely independent laser and beam director 
– Minimal common services, ideally only power and water 
“This division of the laser source among many apertures was initially 
regarded only as a necessary evil, required by the low radiance of 
noncoherent [laser diode] arrays. However, we have recently realized that 
the fact that the laser and optical aperture can be subdivided into small 
independent “beam modules” is a fundamental advantage of laser 
propulsion over other advanced propulsion systems, and may well be the 
key to making laser launch the best option for a future launch architecture” 
-- J. Kare 7/03 
“This division of the laser source among many apertures was initially 
regarded only as a necessary evil, required by the low radiance of 
noncoherent [laser diode] arrays. However, we have recently realized that 
the fact that the laser and optical aperture can be subdivided into small 
independent “beam modules” is a fundamental advantage of laser 
propulsion over other advanced propulsion systems, and may well be the 
key to making laser launch the best option for a future launch architecture” 
-- J. Kare 7/03 
Kare Technical Consulting 3/23/04 11
Advantages of Beam Modules 
• Scalability 
– System grows smoothly by adding beam modules 
• Reliability and maintainability 
– Failed modules have no effect on launch (even in progress) 
– Beam modules can be replaced as units 
• Cost 
– Everything in the system is mass-produced 
– Plausible cost goal: comparable to a modern automobile 
(excluding laser) 
• Development 
– All the technical risk is in the first few units: $M, not $B 
– No failure costs very much -- you can’t “crash the prototype” 
Kare Technical Consulting 3/23/04 12
Conceptual Beam Module (as of last year) 
Optics module 
• 6 kW* diode array 
• Stacking optics 
• Tip-tilt mirror 
• Tracking sensor 
Support module 
• Diode power supply (16 kW* DC) 
• Diode temperature controller 
• Cooling water pump/regulator 
• Tracking sensor controller 
• Mount controller and drivers 
• Tip/tilt controller and drivers 
Telescope 
• 3-m replica primary 
• Secondary 
• 2-axis alt-az mount 
(possibly alt-alt to avoid 
zenith singularity) 
A 100 MW launch 
system might have 
~20,000 of these* -- 
But you can build ONE 
A 100 MW launch 
system might have 
~20,000 of these* -- 
But you can build ONE 
to start with 
to start with 
*Based on 2x1013 radiance and 500 km range; 
better radiance or shorter range would increase 
unit power and decrease number required 
Kare Technical Consulting 3/23/04 13
At Least Three Solutions 
• Fiber Lasers 
• Spectral Beam Combining 
• Diode Pumped Alkali Laser (DPAL) 
All made breakthroughs within the last year! 
Kare Technical Consulting 3/23/04 14
Fiber Lasers 
See www.spiphotonics.com 
• Converts non-coherent diode array light to single-mode laser 
output with up to 90% efficiency; 75% is routine 
• Demonstrated at 1 kW; 10 kW projected within 1-2 years 
• Simple and mass-produceable; already in commercial production 
Kare Technical Consulting 3/23/04 15
Spectral Beam Combining (SBC) 
lmax 
lmin 
Diffraction 
Grating 
Diode bars 
Field lens 
2-D Microlenses 
• Diodes operate independently in external cavity 
Output 
Coupler 
– Antireflection coating on laser diode output facets 
– Each diode automatically operates at the “correct” wavelength 
• Demonstrated* with ~700 diodes in 7 bars (26 watt output) 
– >1000-fold stacking should be feasible 
• SBC efficiency ~50% (power out compared to raw diode bars) 
•AcuLight, Inc., Bothell, WA, 2004 
Kare Technical Consulting 3/23/04 16
Diode Pumped Alkali Laser (DPAL) 
4 kW 795 nm Rb laser concept 
• Diode array pump 6.08 kW @ 780 nm 
• 66% light-to-light efficiency 
• New concept (2003) developed by W. Krupke et al. (ex-LLNL) 
• Rb (785 nm) or Cs (895 nm) vapor in He buffer gas 
– Absorption line pressure-broadened to match diode linewidth 
– High efficiency requires tight control of diode wavelength, spectrum 
• Demonstrated at ~30 W level 
– Performance predicted accurately with no free parameters 
Kare Technical Consulting 3/23/04 17
Laser Subsystem: Alternatives 
DPAL 
Rubidium vapor cell 
795 nm 
Baseline Fiber Laser SBC Diodes 
8 x 125 W diode bars 
805 - 810 nm 
Yb-doped double-core 
fiber 
Lasing medium 
Wavelength 1.08 mm 
Module output power 50 kW 10 kW 50 kW 
10 kW 
6 
1.2 
1.1 x 1016 
54% 
18.5 kW 
50% 
27% 
222 kW 
162 kW 
~300 liter/min* 
Unit laser power 10 kW 600 W 
# of lasers/module 6 20 
2 
2.3 x 1014 
60% SBC eff. 
1000 W 
50% 
30% 
40 kW 
28 kW 
~50 liter/min* 
Beam quality (M2) 1.5 
Radiance (P / l2 (M2)2) 3.8 x 1015 W/m2-sr 
Laser Efficiency (P 80% out / Pdiode) 
Pump Power per laser 12.5 kW 
Diode Efficiency 50% 
DC efficiency (P 40% out / PDC) 
DC Power (module) 150 kW 
Cooling Requirement 90 kW 
Water flow ~100 liter/min 
Kare Technical Consulting 3/23/04 18
10 
9 
8 
7 
6 
5 
4 
3 
2 
1 
0 
How Much Will They Cost? Diode Arrays 
Current 
Price 
Range 
Diamond Optical est. 
$4/W @ 1000 bars, 
~20% drop per 10X qty 
95% learning curve 
90% learning curve 
Likely price range 
@ 200 MW quantity ~$2 - 3.50/W 
0.1 1.0 10.0 100.0 1000.0 
Total power (MW) 
$10/W 
$6/W 
$/Watt 
$/W 
Kare Technical Consulting 3/23/04 19
Laser Diode Cost Trends 
– Substantial reductions in bar cost 
• $100/bar, 100 W bars in 1-2 years (F. Way, Diamond Optical) 
• $10/bar (50 W bars?) “to stay competitive” (a major manufacturer) 
– Substantial reductions in packaging cost 
• LLNL, Oriel, others developing low-cost packaging 
– Oriel “TO-220” package aimed at 50% of late-’03 price; available in mid 2004 
• Diamond Optical willing to quote ~50 cents/watt 
– Unpredictable gains in performance 
• Bars have been stuck at 60 W for several years (100 W Real Soon Now) 
• Major improvement may require radical approach (e.g., VCSEL arrays) 
– But...Current market does not support large investments in improved 
processing/packaging 
• ~$100M/year for all high power arrays, vs. $4B/year for discrete diodes at 
peak of telecomm market 
• ~$1B market for launch system would drive industry 
Kare Technical Consulting 3/23/04 20
How Much Will They Cost? Complete Lasers 
• Current commercial fiber lasers are $500/watt* -- Too Much. 
BUT 
– Relatively low unit power: 100 W 
– Based on discrete packaged diodes @ $100 - 150/watt, not bars 
– Semi-custom production: typically ~10 units 
• Best prediction for high-volume, multi-kW lasers: $7 - 10/W 
– 3 - 4X diode cost 
– Best estimate of component cost in quantity 
– Consistent with projected cost of fiber ($2K / 1 kW) 
– Consistent with ~85% learning curve for complex assemblies 
• Other laser options in same range 
Kare Technical Consulting 3/23/04 21
Telescope Requirements 
• Total Area 
– Set by laser radiance (W/m2-sr) and vehicle flux requirement 
• e.g., fiber laser @ 3.8 x 1015 W/m2 sr requires ~330 m2 of optics 
– Secondary limits from mirror heating, thermal blooming 
• Still need to double check blooming 
• Mirror size and quality 
– Diffraction: Dmirror > f l R / d 
• R / d ~ 105 (500 km / 5 m) f ~ 2 (2.44 for classical limit) 
• ~ 16 cm @ 0.8 mm, 22 cm @ 1.08 mm 
– Wavefront error: Slope < 0.5 x 10-6 
• ~5 waves per meter (vs. 1/10 wave for astronomical telescope) 
• Pointing and tracking 
– Pointing range (nominal) +/- 80° along track, +/- 45° crosstrack 
– Closed loop tracking to <<10 mrad; open loop pointing to ~1 mrad 
Kare Technical Consulting 3/23/04 22
Optics Options 
Cassegrain 
• Simple optics 
• Compact mount 
• Obscuration losses (few %) 
Off-axis Cassegrain 
• Low loss 
• Asymmetric optics 
• Bulky 
Diffractive primary 
• Potentially low cost primary 
• Potentially light weight 
• No obscuration 
• No current technology 
• Chromatic aberration 
Stationary telescope 
with tracking flat 
• All hardware is stationary 
• Minimum moving mass 
• Cheap primary 
• Additional large optic (flat) 
• Field rotation 
Multiple small telescopes 
on common mount 
• Lower optics cost/mass 
• Compact 
• More tracking hardware 
• Alignment problems 
Kare Technical Consulting 3/23/04 23
Optimum Primary Diameter 
Diffraction 
limit ~0.2m 
Production 
optics ~50 cm 
Max. blank diam. 
0.95 - 1.4 m 
Largest monoliths 
made to date 8m 
Tracking hardware 
Const * N ~ D-2 
Mirror cost 
~ N* D2.5 
System 
Cost 
0.1 m 1 m 10 m 
Primary Diameter 
• Minimum size set by tracking hardware cost or diffraction 
• Maximum set by rapid increase in mirror cost with size 
• Small jumps at limits of various “standard” supplier capabilities 
Kare Technical Consulting 3/23/04 24
TANSTAACT(TAG) 
• There Ain’t No Such Thing As A Cheap Telescope 
(That’s Any Good) 
– Many advanced technologies not necessary (or cheap) 
• Non-glass substrates (SiC, Graphite Epoxy) 
• Advanced polishing techniques (magnetorheological polishing) 
• Active/Adaptive primary (PAMELA) 
– Several possibilities still to look at 
• Replica optics 
• Electrodeposited metal optics 
• Lightweight mount (up to half the cost of a telescope) 
• Shifts optimum toward fewer, smaller telescopes than 
original concept 
– “Only” 1000 - 2000 x 1 m, vs. 10,000 x 2 - 3 m 
– Allowed by improved (higher radiance) laser options 
Kare Technical Consulting 3/23/04 25
Telescope Baseline 
• ~1 meter f/2.5 Cassegrain 
– Afocal (technically a Mersenne) 
– Borosilicate (Pyrex) primary 
• “Few-wave” accuracy 
– Multilayer coated for low 
absorption 
• Small (10 cm) secondary 
– Minimize obscuration 
– Limited field of view is OK 
• Alt-Alt mount 
– Tracks smoothly through zenith 
~$100K each @ 1000 units ($22K for primary) 
$2 - 5M investment to be able to make 1/day 
~$100K each @ 1000 units ($22K for primary) 
$2 - 5M investment to be able to make 1/day 
Kare Technical Consulting 3/23/04 26
Photonic Crystal Fibers 
Left: 
“Air-clad” double core fiber 
Right: 
Visible-wavelength high power 
single-mode guiding 
J. Limpert, et al. "Thermo-optical 
properties of air-clad photonic crystal 
fiber lasers in high power operation," 
Opt. Express 11, 2982-2990 (2003) 
• Transport kW power with low loss (<<1 dB/meter) 
www.blazephotonics.com 
–“Holey” fiber region guides single mode; forbids higher modes 
– Most power is transported in void space; avoids nonlinear effects 
• Enabling for low cost beam projectors 
– Eliminates multiple mirrors in beam path 
• Lossy, difficult to align, difficult to clean 
– Isolates laser from telescope motion, dust, etc.... 
Kare Technical Consulting 3/23/04 27
Tracking Subsystem 
• Requirement: point beam to ~5 mradians 
– Track vehicle (control mount) 500 mr @ <10 Hz 
– Compensate atmosphere <100 mr @ ~100 Hz 
“Fast” CMOS camera 
drives tip-tilt mirror; 
100 mr FOV, 500 Hz 
“Slow” CCD camera 
controls mount; 
1 mr FOV, 60 Hz readout 
controller 
3-axis 
(tip/tilt/focus) 
actuated 
mirror 
From laser 
Kare Technical Consulting 3/23/04 28
Beacon Options 
• Reflected laser light 
– Too much local scattered light 
• Thermal radiation from hot heat exchanger 
– Start/restart problem 
– No pointahead for atmospheric correction 
• Ground-based laser with retroreflector 
– Possible, but requires high power (kW), good tracking 
• Beacon on vehicle 
– Narrow-angle with pointing mechanism 
– Wide-angle -- simplest possible system 
• A laser diode and a pingpong ball 
Kare Technical Consulting 3/23/04 29
Baseline Beam Module 
1-m Cassegrain Telescope 
• f/2.5 primary 
• Alt-Alt Mount 
Optics module 
• Fiber output optics 
• Tip-tilt mirror 
• Tracking sensor 
Laser assembly: 
6 x 10 kW 
fiber lasers 
Support module 
• Diode power supply (250 kW DC) 
• Cooling water pump/regulator 
• Tracking sensor controller 
• Mount controller and drivers 
• Tip/tilt controller and drivers 
• Allows for 20% losses in optics, 10% loss in 
transmission, and 10% of modules offline for 
maintenance/repair 
Kare Technical Consulting 3/23/04 30
100 MW System Capital Cost 
• Laser 1020 
– 120 MW Fiber lasers @ $8/watt 960 
– 300 MW DC supply @ $.20/watt 60 
• Optics 144 
– 2000 Primary mirrors @ $22 K 44 
– Other optics, pointing, tracking @ $25 K 50 
– Mount and pad @ $25 K 50 
• Facilities 161 - 350 
– H2 plant (1000 - 30,000 launches/year) 2 - 60 
– Power buffer 15 
– Power line 11-48 
– Launch stand 30 
– Physical plant 100 - 195 
• TOTAL 1325 - 1514 
My long-standing Rule Of Thumb estimate: ~$2 Billion 
Kare Technical Consulting 3/23/04 31
What Happens To Space? 
Architectural Implications 1 
• Cheap small payloads (common to all laser launch) 
1. Microsats/Nanosats: any mission that can be done in 100 
kg pieces will be cheapest that way 
– But that will only account for a few % of launch capacity 
2. Modular satellites/Constellations: Divide up functionality 
into 100 kg co-orbiting blocks (cf. NIAC work on constellations) 
3. On-orbit fueling/refueling/resupply 
– Stimulates development of autonomous microspacecraft 
rendezvous and docking, “tug” spacecraft 
– Opens up high-mass-ratio mission space: Moon/Mars with 
storable propellants 
4. On-orbit assembly: large structures constructed on orbit 
5. True space industry? 
Kare Technical Consulting 3/23/04 32
What Happens To Space Industry? 
Architectural Implications 2 
• Routine, on-demand launch; very high reliability 
– Shift in spacecraft reliability criteria; “ground spares” OK 
• A change in space industry 
– Large aerospace company resources are not required 
– To build vehicles 
– To build beam modules 
– To build payloads 
– “Learning curve” for participation is much less costly 
– A change in space politics 
– More countries can have their own launchers, or “rent 
time” on larger launchers and provide vehicles or payloads 
Kare Technical Consulting 3/23/04 33
What Happens To Human Space? 
Architectural Implications 3 
• Immediate shift in logistics for human LEO missions 
– Missing/broken widgets replaceable by Next Day Space 
• Scaling and reliability enable growing human presence 
– Laser launch is uniquely testable to ~ 10-8 failure probability 
• e.g., 104 launches AND 104 abort/recoveries before flying a 
person 
– Initial human launch capability at TBD payload/laser power 
• Mercury capsule was ~1500 kg; surely we could do better? 
• Potential driver for launch system growth to ~1 GW 
– Growth to 2 or more person vehicle opens up passenger 
launch -- to thousands or 10’s of thousands per year 
Kare Technical Consulting 3/23/04 34
In-Space Power and Propulsion 
Architectural Implications 4 
• Providing electric power shifts module design goals, but 
“power” modules can also be used for launch 
– PV-compatible wavelength preferred (nominally 700 - 900 nm)* 
– Higher beam quality (adaptive optics) may be desired 
– However, dedicated pulsed lasers may be preferred for high-Isp 
pulsed propulsion 
• Low cost modules open design space for space power 
– For GEO power, each satellite can have a dedicated source 
– For LEO/MEO power, modules can be distributed to many sites 
worldwide 
• Launcher site can provide 100-MW power levels anywhere 
out to GEO 
– Relay architectures to be explored 
Kare Technical Consulting 3/23/04 35
Beam Module Satellite Solar Power System 
• Small (10 cm) optics in GEO generate practical (<1 km) 
spot size on Earth 
– Ideal application for diffractive optics? 
• Optics-sized solar panel produces a convenient amount 
of power: ~3 W for 100 cm2 
• SO... build self-contained ~10x10x10 cm beam modules 
and simply stack them up to make a powersat 
– No high power cables 
– No phase locking; 
• No minimum satellite size to deliver power 
• Power can be shared among any number of receivers 
– Modules simply clip to a frame 
Kare Technical Consulting 3/23/04 36
Beam Module SSPS 
Module array on 
simple grid 
Flat film 
reflector 
rotates 1/day 
tilts 1/year 
for sun tracking 
Stationary 
flat film reflector 
Ground 
PV array 
Beacon/ 
command 
transmitter 
Offset from 
ground array 
Possibility: 
Aerostat w. 
microwave 
or fiber bundle 
downlink? 
Note added 3/30/04: 
We have been referred to a similar SSPS 
configuration for microwaves, with a phased 
array transmitter, proposed by Nobuyuki Kaya, 
e.g., in Space Energy and Transportation 1 (3) 
1996, pp. 205-213. Modular laser configurations 
have also been considered; we are still seeking 
details to compare against the concept proposed 
here. 
Kare Technical Consulting 3/23/04 37
Solar Power Satellite Beam Module 
PV Cell 
10 x 10 cm 
3..5 W out 
Laser 
Driver 
3 W in 
Electronics 
power 1/2 W 
Main mirror or diffractive lens ~10 cm dia 
Laser diode 
1.5 W out 
Guide 
sensor 
Controller 
3-axis MEMS 
actuator 
3 cm 
fold 
mirror 
Actuator driver 
Kare Technical Consulting 3/23/04 38
Conclusions 1: Technology Is Ready 
• Lasers crossed the threshold within the last year 
– Performance is sufficient, and nearly certain to improve 
– Costs are still high, but not inherently so 
• Costs will drop with volume and time 
• Current optics technology is dull, but adequate 
– Modern glass optics are cheap enough with high-radiance lasers 
• Optimum primary size is ~1 meter or less 
– Innovative but unproven technologies are waiting in the wings 
• No show-stoppers elsewhere in the system 
– Mounts, pointing and tracking, etc. are straightforward 
• On-vehicle “omni” beacon looks best for pointing/tracking and makes 
adding adaptive optics straightforward if required 
– Power storage is ripe for innovative tech (advanced batteries, 
flywheels) but not a system driver 
Kare Technical Consulting 3/23/04 39
Conclusions 2: 
Architecture Implications Are Profound 
• Laser launch in general shifts paradigms 
– Small unit payloads, routine prompt access => on orbit industry 
• Modular launcher technology changes industry 
– Small companies can play -- modules can come from many sources 
– Small countries can play -- buy their space launch “by the yard” 
• Crewed flight is a new game 
– Continuous scaling from support (100 kg payloads) to solo 
launches (~1000 kg) to taxi (tour bus?) service 
– Inherently high reliability, inherently testable -- tourist friendly! 
• Significant effects on in-space power and propulsion 
– Requirements are different, but overlapping 
– Low-enough unit costs open new options, e.g., laser-per-satellite 
power systems, distributed power belt for orbit raising 
• Spinoffs: powersats, power beaming, industrial lasers... 
Kare Technical Consulting 3/23/04 40
Where to go? 
• Technology development -- only small niches 
– Most technology is being driven by other uses 
– Some leverage in low-cost optics, SBC lasers 
• Technology integration and demonstration 
– Integrated subscale module 
• COTS fiber laser(s) or SBC laser array (~100 W) 
– Upgradeable to higher power as lasers become available 
• Optics TBD: at least half-scale; full-scale if possible 
• Full tracking system 
– Full scale beam module is a bit much to bite off: ~$10-20 M 
• Higher power-per-module than originally conceived 
• System integration and architecture studies 
– Many, many issues barely touched: siting, markets, safety... 
Kare Technical Consulting 3/23/04 41
Laser Launch Architecture With Modular Ground-Based Laser Array 
Large spacecraft are 
assembled and serviced 
at a LEO assembly facility 
(Crewed or robotic) 
(Optionally) Vehicles 
discard aeroshell, 
drop tanks at 
top of atmosphere 
Heat Exchanger 
(HX) vehicle 
with side-facing 
heat exchanger 
Propellant 
(LH2) storage 
Launch catapult 
boosts vehicles to 
~100 m/s 
Vehicle prep Payload handling 
To GEO, Moon, Mars... 
Supply vehicles 
rendezvous with 
Space Station and 
other future facilities 
Individual beams from 
Beam Modules 
add incoherently at 
the vehicle 
Failed modules do 
not affect launch 
Main Beam 
Module Array 
(100 - 10,000 units) 
Power generation/ 
energy storage 
Array control 
Independent payloads 
go directly to LEO 
Baseline: 
expandable 
vehicles 
discarded. 
Vehicles could 
also be reused 
Secondary Beam 
Module array(s) for 
orbit raising, reentry, 
rendezvous 
propulsion, etc 
Recovery 
area 
Kare Technical Consulting 3/23/04 42

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Laser launcharchitecture

  • 1. Modular Laser Launch Architecture: Analysis and Beam Module Design NIAC Phase I Fellows Meeting 24 March 2004 Jordin T. Kare Kare Technical Consulting 908 15th Ave. East Seattle, WA 98112 206-323-0795 jtkare@attglobal.net Revised 3/23/04 Kare Technical Consulting 3/23/04 1
  • 2. The Laser Launch Concept Leave The Hard Parts On The Ground! Launch many small payloads on demand -- up to 10 per hour Leave The Hard Parts ! On The Ground! Laser and Beam Projector • Big • Heavy • Expensive • STATIONARY Vehicle • Small • Simple • Cheap • Inert 30,000 launches per year x 100 kg = 3000 Metric tons per year!! Rule of Thumb: 1 kg of payload per MWof laser Kare Technical Consulting 3/23/04 2
  • 3. Why Laser Launch? • Massive launch capacity – A 100-kg launcher can put 3000 tons per year in LEO • Very low marginal cost to orbit – Electricity, vehicle, and propellant easily <$100/lb • Potentially low total cost to orbit – If the system is cheap enough to buy and run, and… – If there are enough payloads to launch • Maximum safety -- no stored energy on vehicles – Enables all-azimuth launch from any site • High reliability, easy to maintain – The hard parts stay on the ground – Vehicles are simple, mass-produced, and testable • Ultimate launch-on-demand -- FedEx to space Kare Technical Consulting 3/23/04 3
  • 4. Pulsed Laser Propulsion Works... Kare Technical Consulting 3/23/04 4
  • 5. … But Has The Same Problems As Everything Else • Development cost – Even at $10/watt, $1 Billion for 100 MW • Technical risk – You don’t know if it will work at all without spending $$$ • In this case, for a multi-megawatt test laser • Programmatic risk – You don’t know what it will actually cost until you’ve built it • Big lasers have had cost/schedule/performance problems for 40 years! – Reality is always different from theory; operational systems are always different from prototypes Kare Technical Consulting 3/23/04 5
  • 6. The Heat Exchanger Thruster Primary (H2) Propellant Tank Pump (optional) Lightweight Heat Exchanger Secondary (Dense) Propellant Nozzle(s) Laser Beam Dense propellant injection trades lower Isp for higher thrust, matches exhaust velocity to vehicle velocity • Exhaust Temperature ~1000 C • Specific Impulse ~600 seconds Kare Technical Consulting 3/23/04 6
  • 7. Heat Exchanger Thruster Advantages • Works with any laser wavelength and pulse format • Nearly 100% efficient – high absorption, negligible reradiation • Simple to design – Steady flow – Simple propellant properties (especially for H2) • Simple to build – Electroplating technique demonstrated at LLNL – Modular design scales easily to any area • Simple to test – Works with any radiant source; doesn’t even need a laser Kare Technical Consulting 3/23/04 7
  • 8. Current 100 MW Vehicle Concept Dense propellant tanks Avionics ! Drop tank Stage 2 tank Total H2 tank volume ~25 m3 Payload Aeroshell Pressurant tank Drop tank ! ~6 meters ! Heat exchanger (25 m2) Kare Technical Consulting 3/23/04 8
  • 9. What Do We Do About The #%&@ Laser? • Lasers cost too much – Absolute cheapest high power laser is $20-50/watt • CO2 electric discharge, with very poor beam quality • Should scale to 100 MW, but not easily or cheaply – Stay-on-all-day lasers above ~10 kW don’t exist • AVLIS copper vapor lasers were 10 kW total, at a cost of >>$1000/watt • No one will pay to develop a large laser – Too many bad memories: CO2, HF/DF, Excimer, FEL… – “There are liars, damn liars, and laser builders” Kare Technical Consulting 3/23/04 9
  • 10. Laser Diode Arrays • >50% efficient DC to Light at ~800 nm • 10,000 hour lifetime (60,000 launches!) CW operation • Run on DC current; water cooled • Commercially available from multiple vendors • $4 - $10/watt NOW • $2/watt in a few years in 100 MW quantities • BUT -- not coherent; not high enough radiance to beam 500 km A 1200 Watt CW “stack” from Nuvonyx, Inc. -- a catalog item! A 1200 Watt CW “stack” from Nuvonyx, Inc. -- a catalog item! 1 cm Kare Technical Consulting 3/23/04 10
  • 11. The Beam Module Concept • DON’T build one big laser and beam director • Build MANY small “Beam Modules” – Completely independent laser and beam director – Minimal common services, ideally only power and water “This division of the laser source among many apertures was initially regarded only as a necessary evil, required by the low radiance of noncoherent [laser diode] arrays. However, we have recently realized that the fact that the laser and optical aperture can be subdivided into small independent “beam modules” is a fundamental advantage of laser propulsion over other advanced propulsion systems, and may well be the key to making laser launch the best option for a future launch architecture” -- J. Kare 7/03 “This division of the laser source among many apertures was initially regarded only as a necessary evil, required by the low radiance of noncoherent [laser diode] arrays. However, we have recently realized that the fact that the laser and optical aperture can be subdivided into small independent “beam modules” is a fundamental advantage of laser propulsion over other advanced propulsion systems, and may well be the key to making laser launch the best option for a future launch architecture” -- J. Kare 7/03 Kare Technical Consulting 3/23/04 11
  • 12. Advantages of Beam Modules • Scalability – System grows smoothly by adding beam modules • Reliability and maintainability – Failed modules have no effect on launch (even in progress) – Beam modules can be replaced as units • Cost – Everything in the system is mass-produced – Plausible cost goal: comparable to a modern automobile (excluding laser) • Development – All the technical risk is in the first few units: $M, not $B – No failure costs very much -- you can’t “crash the prototype” Kare Technical Consulting 3/23/04 12
  • 13. Conceptual Beam Module (as of last year) Optics module • 6 kW* diode array • Stacking optics • Tip-tilt mirror • Tracking sensor Support module • Diode power supply (16 kW* DC) • Diode temperature controller • Cooling water pump/regulator • Tracking sensor controller • Mount controller and drivers • Tip/tilt controller and drivers Telescope • 3-m replica primary • Secondary • 2-axis alt-az mount (possibly alt-alt to avoid zenith singularity) A 100 MW launch system might have ~20,000 of these* -- But you can build ONE A 100 MW launch system might have ~20,000 of these* -- But you can build ONE to start with to start with *Based on 2x1013 radiance and 500 km range; better radiance or shorter range would increase unit power and decrease number required Kare Technical Consulting 3/23/04 13
  • 14. At Least Three Solutions • Fiber Lasers • Spectral Beam Combining • Diode Pumped Alkali Laser (DPAL) All made breakthroughs within the last year! Kare Technical Consulting 3/23/04 14
  • 15. Fiber Lasers See www.spiphotonics.com • Converts non-coherent diode array light to single-mode laser output with up to 90% efficiency; 75% is routine • Demonstrated at 1 kW; 10 kW projected within 1-2 years • Simple and mass-produceable; already in commercial production Kare Technical Consulting 3/23/04 15
  • 16. Spectral Beam Combining (SBC) lmax lmin Diffraction Grating Diode bars Field lens 2-D Microlenses • Diodes operate independently in external cavity Output Coupler – Antireflection coating on laser diode output facets – Each diode automatically operates at the “correct” wavelength • Demonstrated* with ~700 diodes in 7 bars (26 watt output) – >1000-fold stacking should be feasible • SBC efficiency ~50% (power out compared to raw diode bars) •AcuLight, Inc., Bothell, WA, 2004 Kare Technical Consulting 3/23/04 16
  • 17. Diode Pumped Alkali Laser (DPAL) 4 kW 795 nm Rb laser concept • Diode array pump 6.08 kW @ 780 nm • 66% light-to-light efficiency • New concept (2003) developed by W. Krupke et al. (ex-LLNL) • Rb (785 nm) or Cs (895 nm) vapor in He buffer gas – Absorption line pressure-broadened to match diode linewidth – High efficiency requires tight control of diode wavelength, spectrum • Demonstrated at ~30 W level – Performance predicted accurately with no free parameters Kare Technical Consulting 3/23/04 17
  • 18. Laser Subsystem: Alternatives DPAL Rubidium vapor cell 795 nm Baseline Fiber Laser SBC Diodes 8 x 125 W diode bars 805 - 810 nm Yb-doped double-core fiber Lasing medium Wavelength 1.08 mm Module output power 50 kW 10 kW 50 kW 10 kW 6 1.2 1.1 x 1016 54% 18.5 kW 50% 27% 222 kW 162 kW ~300 liter/min* Unit laser power 10 kW 600 W # of lasers/module 6 20 2 2.3 x 1014 60% SBC eff. 1000 W 50% 30% 40 kW 28 kW ~50 liter/min* Beam quality (M2) 1.5 Radiance (P / l2 (M2)2) 3.8 x 1015 W/m2-sr Laser Efficiency (P 80% out / Pdiode) Pump Power per laser 12.5 kW Diode Efficiency 50% DC efficiency (P 40% out / PDC) DC Power (module) 150 kW Cooling Requirement 90 kW Water flow ~100 liter/min Kare Technical Consulting 3/23/04 18
  • 19. 10 9 8 7 6 5 4 3 2 1 0 How Much Will They Cost? Diode Arrays Current Price Range Diamond Optical est. $4/W @ 1000 bars, ~20% drop per 10X qty 95% learning curve 90% learning curve Likely price range @ 200 MW quantity ~$2 - 3.50/W 0.1 1.0 10.0 100.0 1000.0 Total power (MW) $10/W $6/W $/Watt $/W Kare Technical Consulting 3/23/04 19
  • 20. Laser Diode Cost Trends – Substantial reductions in bar cost • $100/bar, 100 W bars in 1-2 years (F. Way, Diamond Optical) • $10/bar (50 W bars?) “to stay competitive” (a major manufacturer) – Substantial reductions in packaging cost • LLNL, Oriel, others developing low-cost packaging – Oriel “TO-220” package aimed at 50% of late-’03 price; available in mid 2004 • Diamond Optical willing to quote ~50 cents/watt – Unpredictable gains in performance • Bars have been stuck at 60 W for several years (100 W Real Soon Now) • Major improvement may require radical approach (e.g., VCSEL arrays) – But...Current market does not support large investments in improved processing/packaging • ~$100M/year for all high power arrays, vs. $4B/year for discrete diodes at peak of telecomm market • ~$1B market for launch system would drive industry Kare Technical Consulting 3/23/04 20
  • 21. How Much Will They Cost? Complete Lasers • Current commercial fiber lasers are $500/watt* -- Too Much. BUT – Relatively low unit power: 100 W – Based on discrete packaged diodes @ $100 - 150/watt, not bars – Semi-custom production: typically ~10 units • Best prediction for high-volume, multi-kW lasers: $7 - 10/W – 3 - 4X diode cost – Best estimate of component cost in quantity – Consistent with projected cost of fiber ($2K / 1 kW) – Consistent with ~85% learning curve for complex assemblies • Other laser options in same range Kare Technical Consulting 3/23/04 21
  • 22. Telescope Requirements • Total Area – Set by laser radiance (W/m2-sr) and vehicle flux requirement • e.g., fiber laser @ 3.8 x 1015 W/m2 sr requires ~330 m2 of optics – Secondary limits from mirror heating, thermal blooming • Still need to double check blooming • Mirror size and quality – Diffraction: Dmirror > f l R / d • R / d ~ 105 (500 km / 5 m) f ~ 2 (2.44 for classical limit) • ~ 16 cm @ 0.8 mm, 22 cm @ 1.08 mm – Wavefront error: Slope < 0.5 x 10-6 • ~5 waves per meter (vs. 1/10 wave for astronomical telescope) • Pointing and tracking – Pointing range (nominal) +/- 80° along track, +/- 45° crosstrack – Closed loop tracking to <<10 mrad; open loop pointing to ~1 mrad Kare Technical Consulting 3/23/04 22
  • 23. Optics Options Cassegrain • Simple optics • Compact mount • Obscuration losses (few %) Off-axis Cassegrain • Low loss • Asymmetric optics • Bulky Diffractive primary • Potentially low cost primary • Potentially light weight • No obscuration • No current technology • Chromatic aberration Stationary telescope with tracking flat • All hardware is stationary • Minimum moving mass • Cheap primary • Additional large optic (flat) • Field rotation Multiple small telescopes on common mount • Lower optics cost/mass • Compact • More tracking hardware • Alignment problems Kare Technical Consulting 3/23/04 23
  • 24. Optimum Primary Diameter Diffraction limit ~0.2m Production optics ~50 cm Max. blank diam. 0.95 - 1.4 m Largest monoliths made to date 8m Tracking hardware Const * N ~ D-2 Mirror cost ~ N* D2.5 System Cost 0.1 m 1 m 10 m Primary Diameter • Minimum size set by tracking hardware cost or diffraction • Maximum set by rapid increase in mirror cost with size • Small jumps at limits of various “standard” supplier capabilities Kare Technical Consulting 3/23/04 24
  • 25. TANSTAACT(TAG) • There Ain’t No Such Thing As A Cheap Telescope (That’s Any Good) – Many advanced technologies not necessary (or cheap) • Non-glass substrates (SiC, Graphite Epoxy) • Advanced polishing techniques (magnetorheological polishing) • Active/Adaptive primary (PAMELA) – Several possibilities still to look at • Replica optics • Electrodeposited metal optics • Lightweight mount (up to half the cost of a telescope) • Shifts optimum toward fewer, smaller telescopes than original concept – “Only” 1000 - 2000 x 1 m, vs. 10,000 x 2 - 3 m – Allowed by improved (higher radiance) laser options Kare Technical Consulting 3/23/04 25
  • 26. Telescope Baseline • ~1 meter f/2.5 Cassegrain – Afocal (technically a Mersenne) – Borosilicate (Pyrex) primary • “Few-wave” accuracy – Multilayer coated for low absorption • Small (10 cm) secondary – Minimize obscuration – Limited field of view is OK • Alt-Alt mount – Tracks smoothly through zenith ~$100K each @ 1000 units ($22K for primary) $2 - 5M investment to be able to make 1/day ~$100K each @ 1000 units ($22K for primary) $2 - 5M investment to be able to make 1/day Kare Technical Consulting 3/23/04 26
  • 27. Photonic Crystal Fibers Left: “Air-clad” double core fiber Right: Visible-wavelength high power single-mode guiding J. Limpert, et al. "Thermo-optical properties of air-clad photonic crystal fiber lasers in high power operation," Opt. Express 11, 2982-2990 (2003) • Transport kW power with low loss (<<1 dB/meter) www.blazephotonics.com –“Holey” fiber region guides single mode; forbids higher modes – Most power is transported in void space; avoids nonlinear effects • Enabling for low cost beam projectors – Eliminates multiple mirrors in beam path • Lossy, difficult to align, difficult to clean – Isolates laser from telescope motion, dust, etc.... Kare Technical Consulting 3/23/04 27
  • 28. Tracking Subsystem • Requirement: point beam to ~5 mradians – Track vehicle (control mount) 500 mr @ <10 Hz – Compensate atmosphere <100 mr @ ~100 Hz “Fast” CMOS camera drives tip-tilt mirror; 100 mr FOV, 500 Hz “Slow” CCD camera controls mount; 1 mr FOV, 60 Hz readout controller 3-axis (tip/tilt/focus) actuated mirror From laser Kare Technical Consulting 3/23/04 28
  • 29. Beacon Options • Reflected laser light – Too much local scattered light • Thermal radiation from hot heat exchanger – Start/restart problem – No pointahead for atmospheric correction • Ground-based laser with retroreflector – Possible, but requires high power (kW), good tracking • Beacon on vehicle – Narrow-angle with pointing mechanism – Wide-angle -- simplest possible system • A laser diode and a pingpong ball Kare Technical Consulting 3/23/04 29
  • 30. Baseline Beam Module 1-m Cassegrain Telescope • f/2.5 primary • Alt-Alt Mount Optics module • Fiber output optics • Tip-tilt mirror • Tracking sensor Laser assembly: 6 x 10 kW fiber lasers Support module • Diode power supply (250 kW DC) • Cooling water pump/regulator • Tracking sensor controller • Mount controller and drivers • Tip/tilt controller and drivers • Allows for 20% losses in optics, 10% loss in transmission, and 10% of modules offline for maintenance/repair Kare Technical Consulting 3/23/04 30
  • 31. 100 MW System Capital Cost • Laser 1020 – 120 MW Fiber lasers @ $8/watt 960 – 300 MW DC supply @ $.20/watt 60 • Optics 144 – 2000 Primary mirrors @ $22 K 44 – Other optics, pointing, tracking @ $25 K 50 – Mount and pad @ $25 K 50 • Facilities 161 - 350 – H2 plant (1000 - 30,000 launches/year) 2 - 60 – Power buffer 15 – Power line 11-48 – Launch stand 30 – Physical plant 100 - 195 • TOTAL 1325 - 1514 My long-standing Rule Of Thumb estimate: ~$2 Billion Kare Technical Consulting 3/23/04 31
  • 32. What Happens To Space? Architectural Implications 1 • Cheap small payloads (common to all laser launch) 1. Microsats/Nanosats: any mission that can be done in 100 kg pieces will be cheapest that way – But that will only account for a few % of launch capacity 2. Modular satellites/Constellations: Divide up functionality into 100 kg co-orbiting blocks (cf. NIAC work on constellations) 3. On-orbit fueling/refueling/resupply – Stimulates development of autonomous microspacecraft rendezvous and docking, “tug” spacecraft – Opens up high-mass-ratio mission space: Moon/Mars with storable propellants 4. On-orbit assembly: large structures constructed on orbit 5. True space industry? Kare Technical Consulting 3/23/04 32
  • 33. What Happens To Space Industry? Architectural Implications 2 • Routine, on-demand launch; very high reliability – Shift in spacecraft reliability criteria; “ground spares” OK • A change in space industry – Large aerospace company resources are not required – To build vehicles – To build beam modules – To build payloads – “Learning curve” for participation is much less costly – A change in space politics – More countries can have their own launchers, or “rent time” on larger launchers and provide vehicles or payloads Kare Technical Consulting 3/23/04 33
  • 34. What Happens To Human Space? Architectural Implications 3 • Immediate shift in logistics for human LEO missions – Missing/broken widgets replaceable by Next Day Space • Scaling and reliability enable growing human presence – Laser launch is uniquely testable to ~ 10-8 failure probability • e.g., 104 launches AND 104 abort/recoveries before flying a person – Initial human launch capability at TBD payload/laser power • Mercury capsule was ~1500 kg; surely we could do better? • Potential driver for launch system growth to ~1 GW – Growth to 2 or more person vehicle opens up passenger launch -- to thousands or 10’s of thousands per year Kare Technical Consulting 3/23/04 34
  • 35. In-Space Power and Propulsion Architectural Implications 4 • Providing electric power shifts module design goals, but “power” modules can also be used for launch – PV-compatible wavelength preferred (nominally 700 - 900 nm)* – Higher beam quality (adaptive optics) may be desired – However, dedicated pulsed lasers may be preferred for high-Isp pulsed propulsion • Low cost modules open design space for space power – For GEO power, each satellite can have a dedicated source – For LEO/MEO power, modules can be distributed to many sites worldwide • Launcher site can provide 100-MW power levels anywhere out to GEO – Relay architectures to be explored Kare Technical Consulting 3/23/04 35
  • 36. Beam Module Satellite Solar Power System • Small (10 cm) optics in GEO generate practical (<1 km) spot size on Earth – Ideal application for diffractive optics? • Optics-sized solar panel produces a convenient amount of power: ~3 W for 100 cm2 • SO... build self-contained ~10x10x10 cm beam modules and simply stack them up to make a powersat – No high power cables – No phase locking; • No minimum satellite size to deliver power • Power can be shared among any number of receivers – Modules simply clip to a frame Kare Technical Consulting 3/23/04 36
  • 37. Beam Module SSPS Module array on simple grid Flat film reflector rotates 1/day tilts 1/year for sun tracking Stationary flat film reflector Ground PV array Beacon/ command transmitter Offset from ground array Possibility: Aerostat w. microwave or fiber bundle downlink? Note added 3/30/04: We have been referred to a similar SSPS configuration for microwaves, with a phased array transmitter, proposed by Nobuyuki Kaya, e.g., in Space Energy and Transportation 1 (3) 1996, pp. 205-213. Modular laser configurations have also been considered; we are still seeking details to compare against the concept proposed here. Kare Technical Consulting 3/23/04 37
  • 38. Solar Power Satellite Beam Module PV Cell 10 x 10 cm 3..5 W out Laser Driver 3 W in Electronics power 1/2 W Main mirror or diffractive lens ~10 cm dia Laser diode 1.5 W out Guide sensor Controller 3-axis MEMS actuator 3 cm fold mirror Actuator driver Kare Technical Consulting 3/23/04 38
  • 39. Conclusions 1: Technology Is Ready • Lasers crossed the threshold within the last year – Performance is sufficient, and nearly certain to improve – Costs are still high, but not inherently so • Costs will drop with volume and time • Current optics technology is dull, but adequate – Modern glass optics are cheap enough with high-radiance lasers • Optimum primary size is ~1 meter or less – Innovative but unproven technologies are waiting in the wings • No show-stoppers elsewhere in the system – Mounts, pointing and tracking, etc. are straightforward • On-vehicle “omni” beacon looks best for pointing/tracking and makes adding adaptive optics straightforward if required – Power storage is ripe for innovative tech (advanced batteries, flywheels) but not a system driver Kare Technical Consulting 3/23/04 39
  • 40. Conclusions 2: Architecture Implications Are Profound • Laser launch in general shifts paradigms – Small unit payloads, routine prompt access => on orbit industry • Modular launcher technology changes industry – Small companies can play -- modules can come from many sources – Small countries can play -- buy their space launch “by the yard” • Crewed flight is a new game – Continuous scaling from support (100 kg payloads) to solo launches (~1000 kg) to taxi (tour bus?) service – Inherently high reliability, inherently testable -- tourist friendly! • Significant effects on in-space power and propulsion – Requirements are different, but overlapping – Low-enough unit costs open new options, e.g., laser-per-satellite power systems, distributed power belt for orbit raising • Spinoffs: powersats, power beaming, industrial lasers... Kare Technical Consulting 3/23/04 40
  • 41. Where to go? • Technology development -- only small niches – Most technology is being driven by other uses – Some leverage in low-cost optics, SBC lasers • Technology integration and demonstration – Integrated subscale module • COTS fiber laser(s) or SBC laser array (~100 W) – Upgradeable to higher power as lasers become available • Optics TBD: at least half-scale; full-scale if possible • Full tracking system – Full scale beam module is a bit much to bite off: ~$10-20 M • Higher power-per-module than originally conceived • System integration and architecture studies – Many, many issues barely touched: siting, markets, safety... Kare Technical Consulting 3/23/04 41
  • 42. Laser Launch Architecture With Modular Ground-Based Laser Array Large spacecraft are assembled and serviced at a LEO assembly facility (Crewed or robotic) (Optionally) Vehicles discard aeroshell, drop tanks at top of atmosphere Heat Exchanger (HX) vehicle with side-facing heat exchanger Propellant (LH2) storage Launch catapult boosts vehicles to ~100 m/s Vehicle prep Payload handling To GEO, Moon, Mars... Supply vehicles rendezvous with Space Station and other future facilities Individual beams from Beam Modules add incoherently at the vehicle Failed modules do not affect launch Main Beam Module Array (100 - 10,000 units) Power generation/ energy storage Array control Independent payloads go directly to LEO Baseline: expandable vehicles discarded. Vehicles could also be reused Secondary Beam Module array(s) for orbit raising, reentry, rendezvous propulsion, etc Recovery area Kare Technical Consulting 3/23/04 42