virtual lunar regolith handling habitat and thermal gas ... · 0, swip). furthermore the handling...

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Technische Universität München Lehrstuhl für Raumfahrttechnik Contact: Claas Olthoff, [email protected], +49 89 289 15997, www.astronautics.de Lunar regolith handling and thermal gas extraction Gas Analysis Unit and Electronics Supporting Structure / Thermal Insulation Heater Core Tube Lunar surface Simulation of Heat Transfer in Lunar Regolith Stamp heater concept for in-situ thermal extraction of volatiles Lunar regolith heating and gas extraction experiments 5CORNG VTCPURQTV GZRGTKOGPVCVU QP RCTVKCNI RCTCDQNKE ƅKIJV Since 2009, TUM has been leading the DLR-funded research project LUISE (Lunar In-Situ Resource Experiments), which covers supporting studies for future access to lunar resources and possible utilization of such. LUISE and related projects include the study of thermal properties of the lunar regolith and the development of thermal extraction processes to release volatiles from lunar regolith (e.g. OH, H, H 2 0, SWIP). Furthermore the handling and transport of lunar samples is being investigated to evaluate possible volatile loss along the sampling chain and to improve sample FGNKXGT[ VQ UEKGPVKƄE KPUVTWOGPVU Virtual Habitat Simulation Infrastructure Biological Module Crew Module P/C Module The Virtual Habitat (V-HAB) life support system (LSS) simulation tool has been under development at TUM since 2006. The MATLAB ® -based software enables dynamic simulations of spacecraft and spacesuit life support systems including their interactions with the environment and the humans inside. Built upon an object-oriented framework, V-HAB provides the capability for holistic, multi-domain simulations for many applications in closed environments. Using a set of intelligent, variable time step solvers, a wide variety of physical, chemical and biological effects can be simulated. V-HAB also includes a dynamic human physiology model to provide realistic inputs to the LSS. A V-HAB model of the International Space Stations LSS has been validated using ƅKIJV FCVC RTQXKFGF D[ 0#5# CPF '5# LiOH CO2 Removal Filter Store Flow Volume (gas) Filter Bed (solid) exec(): p2p ƅow rate ISS CO 2 partial Pressure in PA Simulation Duration: 100 h ROBEX & Accelerators The Helmholtz Alliance „Robotic Exploration of Extreme Environments – ROBEX“ brings together space and deep-sea research. At the TUM Institute of Astronautics (LRT), several different optical and metallic materials are tested for impact abrasion from lunar regolith. To achieve this, particles of the lunar regolith simulant JSC-1A are accelerated to speeds of up to 360 m/s using an electromagnetic eddy current accelerator developed at LRT. Investigations included changes in sample mass, surface roughness and transmissivity, as well as the effect of different impact angles. Results show that even relatively low impact velocities below 150 m/s cause UKIPKƄECPV FGVGTKQTCVKQP 6JG TGUWNVU CNUQ KPFKECVG VJCV VJG KTTGXGTUKDNG CFJGUKQP QT lodging of dust particles is a major contributor to surface degradation, especially for ductile materials. Mass Range: μg Velocity: 5 - 12 km/s Simulation of Micrometeoroids and Space Debris Impact induced arcing of a solar cell bus bar Impact of a 2 mm steel sphere @ 280 m/s on a TiAl alloy turbine blade Electrothermal Accelerator Mass Range: mg - g Velocity: < 5.5 km/s Particle Impacts Microscopic imagery of three targeted materials (from top to bottom): glass, Makrolon ® , Aluminum Supporting Structure Electrode Capacitor Bank Switch Barrel High Pressure Chamber (Capillary with wire) Projectile Coaxial Plasma Accelerator with Compressor Coil Thermal Moon Simulator The Thermal Moon Simulator (TherMoS) is a dynamic thermal simulation VQQN URGEKƄECNN[ HQEWUGF QP OQXKPI QDLGEVU QP VJG NWPCT UWTHCEG 7UKPI C TC[ VTCEKPI CNIQTKVJO DCUGF QP VJG 0XKFKC 1RVK: HTCOGYQTM 6JGT/Q5 ECP DG WUGF VQ calculate the dynamic radiative heat transfer between rovers or astronauts moving through the lunar terrain made up of boulders and craters which create a varied thermal environment. In order to accurately calculate the temperatures of the lunar surface, TherMoS includes a sophisticated thermal model of different kinds of lunar regolith coupled with an orbit propagator, so for any point in time the surface temperatures can be FGVGTOKPGF 6JKU OQFGN JCU DGGP XCNKFCVGF CICKPUV FCVC HTQO VJG &'8+0'4 instrument on the Lunar Reconnaissance Orbiter. TherMoS is being used for path planning and optimization on the lunar surface as well as in combination with a V-HAB-based spacesuit simulation called V-SUIT. x 10 -4 4 x loc [km] 2 0 -2 -4 0 y loc [km] x 10 -3 4 2 1.5 1 0.5 0 x 10 -4 z loc [km] Time, Lunation 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 Temperature, K 0 50 100 150 200 250 300 350 400 Lunar Temperature model comparison Cremers '71 Vasavada '99 Hale '02 TherMoS Hadley Rille Surface Temperatures Hadley Rille Elevation Map Spacesuit Model S T E P S S u p p o r t i n g T e c h n o l o g i e s f o r t h e H u m a n E x p l o r a t i o n o f P l a n e t a r y S u r f a c e s

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Page 1: Virtual Lunar regolith handling Habitat and thermal gas ... · 0, SWIP). Furthermore the handling and transport of lunar samples is being investigated to evaluate possible volatile

Technische Universität München Lehrstuhl für Raumfahrttechnik

Contact: Claas Olthoff, [email protected], +49 89 289 15997, www.astronautics.de

Lunar regolith handling and thermal gas extraction

Gas Analysis Unit and Electronics

Supporting Structure / Thermal Insulation

Heater

Core Tube

Lunar surface

Simulation of Heat Transfer in Lunar Regolith

Stamp heater concept for in-situ thermal extraction of volatiles

Lunar regolith heating and gas extraction experiments

Since 2009, TUM has been leading the DLR-funded research project LUISE (Lunar In-Situ Resource Experiments), which covers supporting studies for future access to lunar resources and possible utilization of such. LUISE and related projects include the study of thermal properties of the lunar regolith and the development of thermal extraction processes to release volatiles from lunar regolith (e.g. OH, H, H

20, SWIP).

Furthermore the handling and transport of lunar samples is being investigated to evaluate possible volatile loss along the sampling chain and to improve sample

VirtualHabitat

Simulation Infrastructure

BiologicalModule

Crew Module

P/CModule

The Virtual Habitat (V-HAB) life support system (LSS) simulation tool has been under development at TUM since 2006. The MATLAB®-based software enables dynamic simulations of spacecraft and spacesuit life support systems including their interactions with the environment and the humans inside. Built upon an object-oriented framework, V-HAB provides the capability for holistic, multi-domain simulations for many applications in closed environments. Using a set of intelligent, variable time step solvers, a wide variety of physical, chemical and biological effects can be simulated. V-HAB also includes a dynamic human physiology model to provide realistic inputs to the LSS. A V-HAB model of the International Space Stations LSS has been validated using

LiOH CO2 Removal

Filter Store

Flow Volume

(gas)

Filter Bed

(solid)

exec():p2p owrate

ISS CO2 partial Pressure in PA

Simulation Duration: 100 h

ROBEX & Accelerators

The Helmholtz Alliance „Robotic Exploration of Extreme Environments – ROBEX“ brings together space and deep-sea research. At the TUM Institute

of Astronautics (LRT), several different optical and metallic materials are tested for impact abrasion from lunar regolith. To achieve this, particles of the lunar regolith simulant JSC-1A are accelerated to speeds of up to 360 m/s using an electromagnetic eddy current accelerator developed at LRT. Investigations included changes in sample mass, surface roughness and transmissivity, as well as the effect of different impact angles.Results show that even relatively low impact velocities below 150 m/s cause

lodging of dust particles is a major contributor to surface degradation, especially for ductile materials.

Mass Range: μgVelocity: 5 - 12 km/s

Simulation of Micrometeoroids and Space Debris

Impact induced arcing of a solar cell bus bar

Impact of a 2 mm steel sphere

@ 280 m/s on a TiAl alloy turbine blade

Electrothermal AcceleratorMass Range: mg - gVelocity: < 5.5 km/sParticle Impacts

Microscopic imagery of three targeted materials (from top to bottom): glass, Makrolon®, Aluminum

Supporting Structure

Electrode

Capacitor Bank Switch

Barrel

High Pressure Chamber(Capillary with wire)

Projectile

Coaxial Plasma Accelerator

with Compressor Coil

Thermal Moon Simulator

The Thermal Moon Simulator (TherMoS) is a dynamic thermal simulation

calculate the dynamic radiative heat transfer between rovers or astronauts moving through the lunar terrain made up of boulders and craters which create a varied thermal environment.In order to accurately calculate the temperatures of the lunar surface, TherMoS includes a sophisticated thermal model of different kinds of lunar regolith coupled with an orbit propagator, so for any point in time the surface temperatures can be

instrument on the Lunar Reconnaissance Orbiter. TherMoS is being used for path planning and optimization on the lunar surface as well as in combination with a V-HAB-based spacesuit simulation called V-SUIT.

x 10-44

xloc

[km]

20-2-4

0

yloc

[km]

x 10-3

4

2

1.5

1

0.5

0

x 10-4

z loc [k

m]

Time, Lunation0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

Tem

pera

ture

, K

0

50

100

150

200

250

300

350

400

Lunar Temperature modelcomparison

Cremers '71Vasavada '99Hale '02TherMoS

Hadley Rille Surface Temperatures Hadley Rille Elevation Map

Spacesuit Model

STEPS

Sup

port

ing T

echnolo

gies

for th

e Human Exploration

of P

laneta

ry S

urfaces