path toward a scalable lunar volatiles miner prototype

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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 [email protected]

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Page 1: Path Toward a Scalable Lunar Volatiles Miner Prototype

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

[email protected]

Page 2: Path Toward a Scalable Lunar Volatiles Miner Prototype

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

2 10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

Page 3: Path Toward a Scalable Lunar Volatiles Miner Prototype

Helium-3 Enables Clean Nuclear Fusion

3 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

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

Page 4: Path Toward a Scalable Lunar Volatiles Miner Prototype

D3He and 3He3He Fusion Cycles Have Been Demonstrated in a Fusion Technology Institute Lab

D3He-1999

4 10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

3He3He-2005

Page 5: Path Toward a Scalable Lunar Volatiles Miner Prototype

Terrestrial Helium-3 Resources

5 10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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)

Page 6: Path Toward a Scalable Lunar Volatiles Miner Prototype

The Solar Wind Volatiles

6 10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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)

Page 7: Path Toward a Scalable Lunar Volatiles Miner Prototype

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.

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

Page 8: Path Toward a Scalable Lunar Volatiles Miner Prototype

8 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

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

Page 9: Path Toward a Scalable Lunar Volatiles Miner Prototype

Three Wisconsin Lunar 3He Miner Designs Completed

9

Mark-I Mark-II

Mark-III

1988 1994

2006

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

Page 10: Path Toward a Scalable Lunar Volatiles Miner Prototype

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

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10

Page 11: Path Toward a Scalable Lunar Volatiles Miner Prototype

Volatile Flow and Collection Schematic

11

Preheater

Heater

Recuperator

Intercoolers

Compressor

Volatile Storage Tanks

Fluidized Chamber Circuit

Volatile Collection

Fluidized Chamber

Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

Page 12: Path Toward a Scalable Lunar Volatiles Miner Prototype

Mark-3 Operational Parameters, Mass and Power

Distributions

12 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

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

Page 13: Path Toward a Scalable Lunar Volatiles Miner Prototype

Potential Lunar Mining Roadmap

13

(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

Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

Page 14: Path Toward a Scalable Lunar Volatiles Miner Prototype

14 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

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

Page 15: Path Toward a Scalable Lunar Volatiles Miner Prototype

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)

15 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

CNSA Chang’e-3 Lander and Rover

NASA Morpheus Lander

Astrobotic Technologies Polaris Rover

Page 16: Path Toward a Scalable Lunar Volatiles Miner Prototype

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

16 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

10/14/2013

Objectives of the Mark-IV Miner Prototype

Page 17: Path Toward a Scalable Lunar Volatiles Miner Prototype

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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They Said It Couldn’t be Done

Page 18: Path Toward a Scalable Lunar Volatiles Miner Prototype

Upcoming Lunar 3He Fusion Book

Follow-on to Return to the Moon by Dr. Harrison Schmitt

18 10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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

Page 19: Path Toward a Scalable Lunar Volatiles Miner Prototype

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

19

Thank you Wisconsin Space Grant Consortium!

Page 20: Path Toward a Scalable Lunar Volatiles Miner Prototype

10/14/2013 20

Questions?

Aaron D.S. Olson Fusion Technology Institute

University of Wisconsin-Madison

[email protected]

Page 21: Path Toward a Scalable Lunar Volatiles Miner Prototype

Mining Maria Regolith Could Provide Life Support to Crews in Space

21

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)

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

Page 22: Path Toward a Scalable Lunar Volatiles Miner Prototype

Schematic of the Mark III Miner

22

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

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

Page 23: Path Toward a Scalable Lunar Volatiles Miner Prototype

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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Page 24: Path Toward a Scalable Lunar Volatiles Miner Prototype

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Page 25: Path Toward a Scalable Lunar Volatiles Miner Prototype

10/14/2013 Aaron D.S. Olson National Council of Space Grant Directors' Fall Meeting

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Advisor: Dr. Gerald Kulcinski FTI Director