path toward a scalable lunar volatiles miner prototype
TRANSCRIPT
Path Toward a Scalable Lunar Volatiles Miner Prototype
National Council of Space Grant Directors’ Fall Meeting
Charleston,SC
10/14/2013
Aaron D.S. Olson Fusion Technology Institute, University of Wisconsin-
Madison
Outline
Uses of Lunar Volatiles
Helium-3 Fusion
Life Support Volatiles
Lunar Volatiles Miner Designs
Operation of the Mark-III
Development Path
The Mark IV Miner Objectives
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Helium-3 Enables Clean Nuclear Fusion
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Contrast of some key nuclear fusion reactions
High energy neutrons: radioactive waste and reactor wall issues
Deuterium-Tritium
D + T → n (14.07 MeV) + 4He (3.52 MeV)
Output energy mostly from protons, some neutrons are still produced in side D-D reactions
D + 3He → p (14.68 MeV) + 4He (3.67
MeV)
Deuterium-Helium-3
No neutrons, Nuclear Power Without Radioactive Waste!
Helium-3 and Helium-3
3He + 3He → 2p + 4He (12.86 MeV)
14.07 MeV
n
3.52 MeV
n n
n
n
Tritium (3H or T)
n
Deuterium (2H or D)
14.68 MeV
n
3.67 MeV
n n
n
n
Helium-3 (He3)
n
Deuterium (2H or D) 12.86 MeV
n n
n n
Helium-3 (He3) Helium-3 (He3)
n
D3He and 3He3He Fusion Cycles Have Been Demonstrated in a Fusion Technology Institute Lab
D3He-1999
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3He3He-2005
Terrestrial Helium-3 Resources
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Three main sources of Helium-3 on the Earth Atmosphere: Helium-3 concentration in atmosphere is ≈ 7x10-12 by volume. Total in the entire atmosphere is ≈ 4,000 metric tonnes Natural Gas: potentially as much as 280 kg in reserves and speculative sources that are not being tapped Decay of Tritium: Tritium decays into Helium-3 after 12.3 years, about 1 kg/yr of Helium-3 is produced Shortage: increased usage in the last decade has nearly depleted the supply of Helium-3 from Tritium decay (down to < 10 kg as of 2010) Also drove price from (~$1,000,000/kg) to (> $7,000,000/kg)
The Solar Wind Volatiles
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Ionized solar wind is deflected by the Earth’s Magnetosphere Composition : Mostly Hydrogen
•Biogenic elements: H, C, N •Noble gases: He, Ar, Kr, Xe, Ne
Solar Wing Volatiles (SWV) embedded in top few hundred angstroms Meteoritic bombardment churns SWV several meters deep into regolith SWV Retained preferentially in regions with higher Titanium content (Ilmenite: FeTiO3)
Lunar Helium-3 Enables Clean Nuclear Fusion
7
L.J. Wittenberg, J.F. Santarius,
and G.L. Kulcinski, “Lunar
Source of 3He for Commercial
Fusion Power,” Fusion Technology 10, 167 (1986).
Lunar 3He concentration measured in Apollo 11, 12, 14, 15, 16, & 17 plus USSR Luna 16 & 20 samples.
Analysis indicates that ~109 kg of 3He exists near the lunar surface, which equals ~1000 years of world energy supply.
40 tonnes of 3He would supply the entire 2012 US electricity needs.
~10 kg 3He (200 MW-y fusion energy) is accessible on Earth for R&D.
A small fraction of the inventory (~1023 kg) of 3He in the Solar System’s gas giant planets would supply world energy needs for far longer than the age of the universe.
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Radiator/Condenser
Isotopic Separation
1 kg 3He
50 K
1.5 K
0
1000
2000
3000
4000
5000
6000
7000 6100
3300
500
1700 1600 1900
3100
Kg/k
g o
f H
elium
-3
Fuel: H2, CH4, H2O
Life support:
CO2, CH4, N2, H2O
Cryogenics: 4He
3He Mining Produces Valuable Volatile By-Products
Three Wisconsin Lunar 3He Miner Designs Completed
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Mark-I Mark-II
Mark-III
1988 1994
2006
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Excavate and Convey
Beneficiate via Sieves
Beneficiate via Fluidized Bed
Heat and Evolve Volatiles
Bucket Wheel
Screw Conveyor
Preheater Heater
Recuperator
Intercoolers
Ejection Mechanism
Sieves
Regolith Processing in the Mark III Miner
Screw Conveyor
Vacuum 0.015 MPa
Enclosure
Slides
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Volatile Flow and Collection Schematic
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Preheater
Heater
Recuperator
Intercoolers
Compressor
Volatile Storage Tanks
Fluidized Chamber Circuit
Volatile Collection
Fluidized Chamber
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Mark-3 Operational Parameters, Mass and Power
Distributions
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Selected Annual Miner Parameters
3He extraction (kg) 66*
Mining time (hr): 90 % of lunar
days
3942
Excavation rate (tonnes/hr) 1258
Processing rate (tonnes/hr) 556
Excavation depth (m) 3.0
Forward miner speed (m/hr) 23
Area excavated (km2) 1.0
Thermal process power (MW) 12.3
Operating power (M-II, M-III)
(kWe)
200,
350
Miner mass (M-II, M-III) (tonnes) 18, 9.9
*assuming a 20ppb 3He grade, however only
10ppb was used by Sviatoslavsky and Gajda in
their miner designs leading to reported annual
acquisition of 3He at 33 kg
18%
4%
11%
17% 9% 6%
18%
3%
14%
Mass: 9.9 tonnes
Bucket Wheel Excavator
Regolith Separation
Heater
Volatile Storage
Screw Conveyor
Regolith Transportation
Locomotion
Structural Components
Power and Electronics
34%
2% 49%
4% 5%
4%
1%
1%
Power: 350 kWe
Potential Lunar Mining Roadmap
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(NASA RESOLVE)
(UW Mark-II concept) ( Demonstration scale concept)
Ground Truth ~2013-2020
Demo and Small Scale ~2020-2030
Industrial Mining ~Post 2030
No surface assets
Limited landing
capability
Limited material return
Limited surface assets
Matured landing
capability
Matured material return
Matured surface assets
Advanced landing
capability
Advanced material
return
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0.01
0.10
1.00
10.00
100.00
1000.00
10000.00
1E-2
1E-1
1E+0
1E+1
1E+2
1E+3
1E+4
1E+5
0.1 1 10 100 1000
Nu
mb
er o
f P
eop
le S
up
port
ed (
#/y
r)
Vola
tile
s P
rod
uce
d (
kg/y
r)
Regolith Mining Rate (tonnes/hr)
Helium-3
Water (H20)
Number of Crew
Mining for Solar Wind Volatiles Could Provide Life Support for 333 People
3.8 tonnes/hr 46 tonnes/hr 1258 tonnes/hr
International Civil Agencies and New Space Companies are
Developing Lunar Capabilities
NASA: Resource Prospector, Lunabotics, Morpheus lander
CNSA: Chang’e 3,4…
ISRO: Chandrayaan-2
Roscosmos: Luna 25,26…
JAXA: SELENE 2,3…
Google Lunar X-Prize
20 proposed lunar missions (2013-21)
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CNSA Chang’e-3 Lander and Rover
NASA Morpheus Lander
Astrobotic Technologies Polaris Rover
Mark-IV: The First 3He and Volatiles Miner Prototype
Demonstrate 3He extraction process
Produce volatiles for life support and other in-space needs O2, H2O, H2,
4He, N2, CO2,CO, CH4
Scalable to meet lunar exploration and space development needs prior to operational 3He fusion power plants
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Objectives of the Mark-IV Miner Prototype
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They Said It Couldn’t be Done
Upcoming Lunar 3He Fusion Book
Follow-on to Return to the Moon by Dr. Harrison Schmitt
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Discusses Increasing need for
power worldwide Potential role of 3He
Fusion technology Lunar Bases and
Resources Legal Regimes for
Lunar Mining Economics of 3He
Procurement Space Applications of
3He Fusion Current Lunar
Initiatives
Authors: Dr. Harrison Schmitt, Dr. Gerald Kulcinski, Dr. John Santarius, Aaron Olson
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Thank you Wisconsin Space Grant Consortium!
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Questions?
Aaron D.S. Olson Fusion Technology Institute
University of Wisconsin-Madison
Mining Maria Regolith Could Provide Life Support to Crews in Space
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Volatiles Delivered to ISS in 2012*
Volatile Mass (kg)
Mass/crew
member (kg) #
Air 38 6.3
Nitrogen^ 30 5.0
Oxygen 253 42.2
Water 1965 327.5
*8 Cargo resupply missions conducted
by: the Russian Progress, European
ATV, Japanese HTV and Space-X
Dragon
^ Assumes ~78% N2 air composition
# 6 Crew more or less constant in 2012
Products of Heating Mare Regolith to 700 °C
Volatile
Mass evolved per
tonne of regolith
mined (g)**
Mass evolved
per kg of 3He
evolved (kg)
H2 43 6100 4He 22 3100 3He 0.007 1
H2O 23 3300
N2 4.0 500
CH4 11 1600
CO 13.5 1900
CO2 12 1700
**After beneficiation, 450 kg of regolith is
heated Delivered Oxygen is not equal to the metabolic requirement of 0.84 kg O2 /day 0.84 kg Oxygen is for the average adult American male Water is electrolyzed on board for Oxygen production
Delivered water is not equal to the requirement of 3.9 kg H2O/crew member per day ECLSS water recycling system (urine filtration)
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Schematic of the Mark III Miner
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Vacuum
0.015 MPa
Enclosure
Sieves
Fluidized Chamber
Compressors
Screw Conveyor
s
Ejection Mechanism
Screw Conveyor
s Bucket Wheel Excavator
Gas Storage Tanks
Intercoolers
Chute
Slides
Electrostatic Separator
Belt Conveyor
s Heater
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Advisor: Dr. Gerald Kulcinski FTI Director