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7/28/2019 Exploration Systems Mission Directorate (NASA)

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September 20, 2007September 20, 2007

Exploration Systems Mission

Directorate

Lunar Architecture Update


Directorate


AIAA Space 2007AIAA Space 2007

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NASAs Lunar ArchitectureNASAs Lunar Architecture

Introduction to Session Doug Stanley

Current exploration strategy and status - Doug Cooke

Lunar Architecture update Geoff Yoder Lunar Science Laurie Leshin

Pressurized Rover and EVA concepts - Mike Gernhardt

Session wrap-up and questions

Introduction to Session Doug Stanley

Current exploration strategy and status - Doug Cooke

Lunar Architecture update Geoff Yoder Lunar Science Laurie Leshin

Pressurized Rover and EVA concepts - Mike Gernhardt

Session wrap-up and questions

WWW.NASAWATCH.COM


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Directorate


AIAA Space 2007


Directorate


AIAA Space 2007

Doug CookeDeputy Associate Administrator

NASA Exploration Systems Mission Directorate

September 20, 2007

Doug CookeDeputy Associate Administrator

NASA Exploration Systems Mission Directorate

September 20, 2007

WWW.NASAWATCH.COM


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4

Space Exploration Direction, Authorized by CongressSpace Exploration Direction, Authorized by Congress

Complete the International Space Station Safely fly the Space Shuttle until 2010 Develop and fly the Crew Exploration Vehicle no later than 2014 Return to the Moon no later than 2020 Extend human presence across the solar system and beyond Implement a sustained and affordable human and robotic program Develop supporting innovative technologies, knowledge, and

infrastructures

Promote international and commercial participation in exploration

The Administrator shall establish a program todevelop a sustained human presence on the Moon,

including a robust precursor program to promote

exploration, science, commerce and U.S.

preeminence in space, and as a stepping stone to

future exploration of Mars and other destinations.

NASA Authorization Act of 2005

WWW.NASAWATCH.COM


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1

Lunar Robotic

MissionsLunar Outpost Buildup

Commercial Crew/Cargo for ISS

Ares I Development

Lunar Lander Development

Surface Systems Development

Ares V & Earth Depar ture Stage

0605 07 08 09 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25

Exploration Roadmap

SSP Transiti on

Orion Development

Orion Production and Operation

Space Shutt le Operations

InitialCapability

Orion (CEV)

Mars

Expedition

2030(?)

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Exploration ProgressExploration Progress

In December 2006, we released

Exploration themes and objectives- Developed with

together with

U.S. industry, academia, and science communities

13 other space agencies

Our initial Lunar architecture results- then shared

with the broader community

In 2007, our collective and individual communities havecontinued to make progress in defining what and howwe will achieve our exploration objectives

Here we will present results from latest studies

To be communicated and discussed with the broadercommunity

Compared with architecture studies from these

communities

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Architecture DevelopmentDriven By A Strategy

Architecture DevelopmentDriven By A Strategy

Global Exploration Strategy DevelopmentGlobal Exploration Strategy Development Themes &

Objectives

Architecture AssessmentArchitecture Assessment

Reference Architecture

& Design ReferenceMissionOutpost First at one of

the PolesElements critical to US

Detailed DesignDetailed DesignOperations Concept,Technology Needs,

Element RequirementsMaintain flexibility

NationalPrioritiesDefined

DetailedRequirements

Defined

LAT-1

LAT-2

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Global Exploration Strategy - 6 ThemesGlobal Exploration Strategy - 6 Themes

Human Civilization

Scientific Knowledge

Exploration Preparation Public Engagement

Economic Expansion

Global Partnerships

WWW.NASAWATCH.COM


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Ares I

Crew Launch

Vehicle

Ares I

Crew Launch

Vehicle

Earth Departure StageEarth Departure Stage

OrionCrew Exploration

Vehicle

OrionCrew Exploration

Vehicle

Lunar

Lander

Lunar

Lander

Ares V

Cargo Launch

Vehicle

Ares V

Cargo Launch

Vehicle

US Transportation ArchitectureUS Transportation Architecture

APO AmbBrief + 9

WWW.NASAWATCH.COM


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Lunar Architecture Framework Point of Departure- December 2006Lunar Architecture Framework

Point of Departure- December 2006

Robotic missions will be used to:

Characterize critical environmental

parameters and lunar resources

Test technical capabilities as

needed

The ability to fly robotic missions

from the outpost or from Earth will

be a possible augmentation

Human lunar missions will be used to

build an outpost initially at a polar site

The ability to fly human sorties andcargo missions with the human lander

will be preserved

Initial power architecture will be solar

with the potential augmentation ofnuclear power at a later time

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NASA Implementation Philosophy

The US will perform earlydemonstrations to encourage

subsequent development

External parallel development ofNASA developed capabilities will

be welcomed

The US will build the transportationinfrastructure and initial communication &

navigation and initial surface mobility

Open Architecture: NASA will welcomeexternal development of lunar surface

infrastructure

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Open Architecture: InfrastructureOpen for Potential External Cooperation

Lander and ascent vehicle EVA system

CEV and Initial Surface capability

Long duration surface suit

Power Basic power

Augmented

Habitation Mobility

Basic rover

Pressurized rover Other; mules, regolith moving,

module unloading

Navigation and Communication Basic mission support

Augmented

High bandwidth ISRU Characterization

Demos

Production

Robotic Missions LRO- Remote sensing and map development

Basic environmental data

Flight system validation (Descent and landing)

Lander Small sats

Rovers

Instrumentation

Materials identification and characterization

for ISRU

ISRU demonstration

ISRU Production

Parallel missions

Logistics Resupply Specific Capabilities

Drills, scoops, sample handling, arms

Logistics rover

Instrumentation

Components

Sample return

** US/NASA Developed hardware

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Second Phase of Lunar Architecture StudiesSecond Phase of Lunar Architecture Studies

This phase of studies builds results presented in December

Significant NASA-wide effort

Responsive to more Themes and objectives

Outpost decision addressed broad range of themes andobjectives

Did not fully address objectives requiring travel to other lunarsites- primarily some science objectives

Assessed metrics

Merits and features

Relative risks

Crew time on the Moon Time available for Exploration

Early return from missions

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WWW NASAWATCH COM


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Factors in latest Architecture Study ResultsFactors in latest Architecture Study Results

Six options studied

Derived the best features from each option

Based on better understanding of vehicle performance

Better definition of concepts-

Down to detailed components

To better understand capabilities and feasibility

Most effective use of crew

Steps to better address objectives

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OutlineOutline

Architecture- Guidelines and Attributes

- Strategy

- Options

Communication and Navigation

Figures of Merit

Discriminators

A Hybrid Approach

Architecture- Guidelines and Attributes

- Strategy

- Options

Communication and Navigation

Figures of Merit

Discriminators

A Hybrid Approach


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Architecture Desired AttributesArchitecture Desired Attributes

Enable lunar sustained presence early

Develop infrastructure while actively engaged in science and

exploration

Ensure architecture is flexible to redirection

Ensure architecture supports Objectives

Support the establishment of Mars analog

Allow the earliest partnership opportunities for commerce andInternational Partners

Continuous and measurable progress Continuous and focused public engagement

Enable lunar sustained presence early

Develop infrastructure while actively engaged in science and

exploration

Ensure architecture is flexible to redirection

Ensure architecture supports Objectives

Support the establishment of Mars analog Allow the earliest partnership opportunities for commerce and

International Partners

Continuous and measurable progress

Continuous and focused public engagement

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Architecture StrategyArchitecture Strategy

Successful lunar exploration is not just about developing a Lander ora Habitat

It will require development of a system of exploration elements Transportation Vehicles (Launch Vehicle, Landers)

Habitation

Rover

EVA Systems

Surface Power

Communication

The architecture challenge is to assemble the best mix of these

elements so they work synergistically together to efficiently achievethe objectives

Successful lunar exploration is not just about developing a Lander ora Habitat

It will require development of a system of exploration elements Transportation Vehicles (Launch Vehicle, Landers)

Habitation

Rover

EVA Systems

Surface Power

Communication

The architecture challenge is to assemble the best mix of these

elements so they work synergistically together to efficiently achievethe objectives

WWW.NASAWATCH.COM


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Architectural Options Under EvaluationArchitectural Options Under Evaluation

Option 1: All elements delivered with crewed flights (LAT 1)

Option 2: Derivative of LAT 1 except uncrewed lander can deliver

hardware to surface provided all elements must be sized to fit on acrewed lander.

Option 3: A single large, fully outfitted and pre-integrated Habitation

launched and landed on a single uncrewed mission

Option 4: The lander has integrated surface mobility (mobile lander)

Option 5: Long range, pressurized rover delivered as early in the

sequence as possible (Captured in each)

Option 6: Nuclear power used for the surface power in lieu of solar

Option 1: All elements delivered with crewed flights (LAT 1)

Option 2: Derivative of LAT 1 except uncrewed lander can deliver

hardware to surface provided all elements must be sized to fit on acrewed lander.

Option 3: A single large, fully outfitted and pre-integrated Habitation

launched and landed on a single uncrewed mission

Option 4: The lander has integrated surface mobility (mobile lander)

Option 5: Long range, pressurized rover delivered as early in the

sequence as possible (Captured in each)

Option 6: Nuclear power used for the surface power in lieu of solar


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MONOLITHIC

Option 3 Single Habitat Delivered in One FlightOption 3 Single Habitat Delivered in One Flight

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Option 3 Single Delivery, Monolithic HabitatOption 3 Single Delivery, Monolithic Habitat

Hab can be integrated, checked out pre-

launch

Supports Mars concepts

Less flexible to redirection and Exploration inflexible

Less tolerant to loss of elementLess adaptable to reduced transportation capability

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Option 4 Mobile LanderOption 4 Mobile Lander

Can use mobili ty to assemble outpost elements but carries a penalty

Challenge is to maximize benefit of lander mobili ty

Can use mobili ty to assemble outpost elements but carries a penalty

Challenge is to maximize benefit of lander mobil ity

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Option 4 Mobile Lander Habitat SystemOption 4 Mobile Lander Habitat System

Friendly to Commercial, IP rolesFlexible to redirection

Very Exploration flexible

Tolerant to loss of element

Resolves much of the unloading and

transportation issueSmaller bone yard

Not adaptable to reduced transportation

capability

High level of complex integration


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Option 6 Nuclear Surface Fission PowerOption 6 Nuclear Surface Fission Power

Helps non-polar Outpost sites

Good for ISRU

Supports Mars

Not flexible, reactor anchors exploration site

Not failure tolerant, still need some solar initially

Emplacement is challenging

Carries political sensitivities


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Cumulative Surface Stay Days (Planned)Cumulative Surface Stay Days (Planned)

2t Crew14t Cargo

Lander

Payload

Capacity

6t Crew19t Cargo

Lander

Payload

Capacity

6t Crew,

No Cargo

Lander

(LAT-1)

Crew surface time does not favor any one option over another

0

500

1000

1500

2000

2500

2019 2020 2021 2022 2023 2024 2025 2026 2027 2028 2029 2030

CumulativeSurfaceStayDays(Plan

ned)

Option 1 Mini-Hab

Option 2 Mini-Hab/Cargo

Option 3 Monolithic

Option 4 Mobile

Option 6-2 Nuclear Mini-Hab

Option 6-3 Nuclear Monolithic

Option 1 Mini-Hab

Option 2 Mini-Hab/Cargo

Option 3 Monolithic

Option 4 Mobile

Option 6-2 Nuclear Mini-Hab

Option 6-3 Nuclear Monolithic

6t Lander

2t Lander

Reduced delivery lander

sacrifices crew surface time

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Crew Time Util ization, Mini-Hab vs.Monolithic vs. Mobile

Crew Time Util ization, Mini-Hab vs.Monolithic vs. Mobile

Percent EVA Time: Option 2 (6MT)

0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21

Mission #

%o

fEV

AHours

Science/Exploration

Assembly

Maintenance


0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21

Mission #

%o

fEV

AHours


0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21

Mission #

%o

fEVAHours

Science/Exploration

Assembly

Maintenance

Science/Exploration

Assembly

Maintenance A large proportion of time is still

available for exploration

Early Assembly and Maintenance

can be significant for construction of

a mini-hab outpost

Option 4 Mobile Lander

Option 2 Mini-Hab Option 3 Monolithic


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Surface Architecture - Discrete elements sized smaller than the monolithic

unit, but larger than the mini-hab concept

Surface Architecture - Discrete elements sized smaller than the monolithic

unit, but larger than the mini-hab concept

Cargo lander needed forrobustness

Outpost built up from only 2or 3 of these elements

Assembly facilitated fromseparate surface mobility

system

Make maximum use ofdelivered hardware to

minimize the bone yard

Cargo lander needed forrobustness

Outpost built up from only 2or 3 of these elements

Assembly facilitated fromseparate surface mobility

system

Make maximum use ofdelivered hardware to

minimize the bone yard

A flexible architecture incorporating best features and lessons

learned from all the Lunar Architecture Team options

Hybrid Approach to OptionsHybrid Approach to Options

H b id A h t O tiH b id A h t O ti

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Capability for global access and extended range surface

exploration is essential

Hybrid Approach to Options(cont.)

Hybrid Approach to Options(cont.)

Surface Mobility Early delivery of small, agile

pressurized rover that carries SPE

protection, suit lock (not like

Apollo)

Utilize common elements from

surface carrier where possible(e.g. wheel/motor units)

Surface Mobility Early delivery of small, agile

pressurized rover that carries SPE

protection, suit lock (not like

Apollo)

Utilize common elements from

surface carrier where possible(e.g. wheel/motor units)


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Science Capability

on the Moon

Science Capability

on the Moon

Laurie LeshinNASA Goddard Space Flight Center

LAT Science Capabili ty Focus Element

Constellation Program Science Office

Laurie LeshinNASA Goddard Space Flight CenterLAT Science Capabil ity Focus Element

Constellation Program Science Office


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Top Objectives Examples:Top Objectives Examples:

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p j pPlanetary Science Subcommittee Findings

p j pPlanetary Science Subcommittee Findings

INTERNAL STRUCTURE andDYNAMICS - Geophysical/heat flow

network - requires multiple sites, widely

spaced (global access)

COMPOSITION/EVOLUTION ofLUNAR CRUST - requires extensivesampling at both local and diverse sites

IMPACT FLUX - requires access toimpact basins and sample return for age

dating

SOLAR EMISSIONS/GCR/INTERSTELLAR - requires drilling,

regolith and core sample integrity,

careful documentation

SAMPLE ANALYSIS INSTRUMENTSAND PROTOCOLS - infrastructure for

pristine sample collection, storage,

documentation, and transport needed

Representative Science Payload Elements

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Representative Science Payload Elements

Sample containers and tools to replace

consumables in TSP

Sampling Resupply Kit

(SRK)

Diverse kit including sampling tools and containers,

rover-carried sample selection instruments, andtraverse geophysics instruments

Traverse and Sampling

Package (TSP)

Geophysics station seismology, heat flow, etc.Lunar Interior Monitoring

Station (LIMS)

Orbital science to be carried either in SIM bay or

to be kicked out into lunar orbit mostly

heliophysics science

Orbiter Packages (ORB)

Small observatory for earth observation or

astrophysics applications

Telescope (OBS)

Automated sample handling equipment outside the

hab-lab for handling samples in the rock garden

Automated Sample

Handling System (SHED)

Instruments inside lab at outpost for sample

screening

Lab in Hab (LAB)

Volatiles, plasma field, radiation monitoring, dust

should be deployed early to monitor site evolution

Lunar Environmental

Monitoring Station (LEMS)

DescriptionElement Name

Lunar Telescope

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pScience Goals and Study Objectives

Science Goals and Measurements A simple and autonomous Earth-observing

system

A study of the light and chemical signatures

of Earth can provide information on theplanets habitability and biology

The signature of the direct and

spectroscopic light-curves of the Earth will

be used to understand current and future

observations of Earth-like exoplanets Will measure variations in photometric,

spectral, and polarization signatures over

visible and near-infrared wavelengths

Provides near-simultaneous imaging,

polarimetry, and spectral data of the fullEarth disk

Study Objectives Based on ALIVE Lunar Telescope proposal,

develop a Lunar Telescope support system

to be installed on the Lunar surface


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Science Manifesting GuidelinesScience Manifesting Guidelines

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Science Manifesting GuidelinesScience Manifesting Guidelines

MEDIUM PRIORITY 3 bring as soon as can be accommodated

but after LIMS and OBS. Can bring more then 1 as this is ageneric orbiter

Orbiter Packages (ORB)

MEDIUM PRIORITY 2 bring as soon as can be accommodated

but after LIMS. Can bring more then 1 as this is a generic

telescope

Telescope (OBS)

This is needed once the lab is functioning.Automated Sample

Handling System

(SHED)

This is most critical after stays get long (~a month), and

assuming there is room to set it up in the hab

Lab in Hab (LAB)

MEDIUM PRIORITY 1 Bring 1 LIMS ASAP after LEMS and

adequate sampling supplies. If mobility of ~500 km is possible,

bring 2 more LIMS ASAP. 5 year life replace after 5 years.

Lunar Interior

Monitoring Station

(LIMS)

HIGH PRIORITY -- Need one of these for each crewed mission

can stockpile ahead of time

Sampling Resupply Kit

(SRK)

HIGH PRIORITY -- Need one of these for each rover. In absence

of rover, at least need sample supplies up to available mass.

Traverse and Sampling

Package (TSP)

HIGH PRIORITY -- Important to get this down as early as possible

to monitor site evolution as humans come. 5 year life replace

after 5 yrs

Lunar Environmental

Monitoring Station

(LEMS)

Manifesting GuidanceElement Name

The Architecture Maintains Sortie Capability:Possible Sortie Locations to Optimize for Geophysics

The Architecture Maintains Sortie Capability:Possible Sortie Locations to Optimize for Geophysics

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Possible Sortie Locations to Optimize for GeophysicsPossible Sortie Locations to Optimize for Geophysics

Site Lat. Long.

A South Pole 89.9 S 180 W

B Aitken Basin 54 S 162 W

C Orientale Basin 19 S 88 W

D Oceanus Procellarum 3 S 43 W

E Mare Smythii 2.5 N 86.5 E

Site Lat. Long.

F Mare Tranquillitatis 8 N 21 E

G Rima Bode 13 N 3.9 W

H Aristarchus Plateau 26 N 49 W

I Central Far Side Highlands 26 N 178 E

J North Pole 89.5 N 91 E

National Research Council Report: Scientific Contextf E l ti f th M

National Research Council Report: Scientific Contextfor Exploration of the Moon

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for Exploration of the Moonfor Exploration of the Moon

Asked by NASA SMD to provideguidance on the scientific challenges

and opportunities enabled by a

sustained program of robot ic and

human exploration of the Moon during

the period 2008-2023 and beyond

Key Science Findings:

Enabling activities are critical in the near

term Strong ties with international programsare essential

Exploration of the South Pole-AitkenBasin remains a priority

Diversity of lunar samples is requiredfor major advances The Moon may provide a unique location

for observation and study of Earth, near-

Earth space, and the universe

Scientif ic Context for Exploration of the Moon:Highest Priority Science Objectives

Scientific Context for Exploration of the Moon:Highest Priority Science Objectives

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Highest Priority Science ObjectivesHighest Priority Science Objectives Test the cataclysm hypothesis by determining the spacing in time of

the creation of the lunar basins. Anchor the early Earth-Moon impact flux curve by determining the age

of the oldest lunar basin (South Pole-Aitken Basin).

Establish a precise absolute chronology. Determine the compositional state (elemental, isotopic, mineralogic)

and compositional distribution (lateral and depth) of the volatilecomponent in lunar polar regions.

Determine the extent and composition of the feldspathic crust,KREEP layer, and otherproducts of planetary differentiation.

Determine the thickness of the lunar crust (upper and lower) andcharacterize its lateral variability on regional and global scales. Characterize the chemical/physical stratification in the mantle,particularly the nature of the putative 500-km discontinuity and thecomposition of the lower mantle.

Determine the global density, composition, and time variability of thefragile lunar atmosphere before it is perturbed by human activity.

Determine the size, composition, and state (solid/liquid) of the core ofthe Moon.

Inventory the variety, age, distribution, and origin oflunar rock types. Determine the size, charge, and spatial distribution of

electrostatically transported dust grains and assess their likelyeffects on lunar exploration and lunar-based astronomy.


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Extravehicular Activities (EVA) and

Pressurized Rovers

Extravehicular Activities (EVA) and

Pressurized Rovers

Mike GernhardtNASA Johnson Space CenterMike GernhardtNASA Johnson Space Center


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Challenges for EVA on the MoonChallenges for EVA on the Moon

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Dealing with risk and consequences of a significant Solar Particle

Event (SPE) Long duration missions with three 8hr EVAs per person per week

Apollo suits were used no more than 3 times

Individual crewmembers might perform up to 76 EVAs in a 6-month

mission

Suit-induced trauma currently occurs with even minimal EVA time

With Apollo style unpressurized rover (UPR), exploration range islimited EVA sortie time and 10 km walkback constraint

Science community believes that significantly greater range will be

required for optimal science return

Apollo highlighted the importance of dust control for future longduration missions

Increased Decompression Sickness (DCS) risk and prebreatherequirements associated with 8 psi 32% O2 cabin pressure versus

Apollo with 5 psi 100% O2 The high frequency EVA associated with the projected lunar

architectures will require significant increases in EVA work

efficiency (EVA prep time/EVA time)

The Wall of EVA The Wall of EVA

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0

50

100

150

200

66 68 70 72 74 76 78 80 82 84 86 88 90 92 94 96 98 0 2

EVA

Hours

Gemini

Apollo/

SkylabPre-Challenger

ShuttleShuttle

Station

Construction

Year

The Mountain of EVA The Mountain of EVA

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0

500

1000

1500

2000

2500

3000

3500

4000

4500

5000

1966

1968

1970

1972

1974

1976

1978

1980

1982

1984

1986

1988

1990

1992

1994

1996

1998

2000

2002

2004

2006

2008

2010

2012

2014

2016

2018

2020

2022

2024

2026

2028

2030

Year

EV

AH

ours

ISS Construction(projected)

Available Lunar EVA Hours

(LAT-2 Option 2)

Gemini

Apollo/SkylabPre-ChallengerShuttle

Shuttle

The Wall

The Mountain

EVA Work Efficiency Index:Exploration EVA Should Target WEI >3.0

EVA Work Efficiency Index:Exploration EVA Should Target WEI >3.0

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Commercial saturation divinghas WEI of 3-10 depending ondepth

Commercial saturation divinghas WEI of 3-10 depending ondepth

TOTAL EVA Work Efficiency Index =EVA Time

(Total EMU/A/L Prep + Prebreathe + A/L Depress + A/L Repress + Total Post EVA)

PREBREATHE

PROTOCOL

Shuttle 10.2 Staged

Decompression (12hrs at 10.2)

ISS: 4 hour In

Suit

ISS CEVIS Exercise

(Using ISS O2)

EVA Overhead

ActivitiesTIME IN MINUTES

TIME IN

MINUTESTIME IN MINUTES

Suit checkout 115 185 185

REBA powered

hardware checkout25 25 25

SAFER checkout 30 30 30

Airlock config 95 90 90

Consumables Prep 60 120 120

EVA prep - prebreathe

related 60 0 80

EVA prep - EMU

related30 30 30

Suit donning & leak

check60 60 60

SAFER donningCompleted during

Prebreathe

Completed during

Prebreathe

Completed during

Prebreathe

Purge 8 12 12

Prebreathe 75 240 60

Airlock depress 15 30 40

Airlock egress 15 15 15

Airlock ingress 15 15 15

Airlock repress 15 15 15

Suit doffing 25 25 25

SAFER doffing & stow 10 10 10

Post EVA processing 105 90 90

TOTAL 758 992 902

EVA WORK

EFFICIENCY INDEX 0.51 0.39 0.43

Total Suit/Airlock OverheadTotal Suit/Airlock Overhead

Life Science controls significant

portion of EVA overhead:

Prebreathe

Biomedical sensors

Nutrition and Hydration Systems

Additionally the EVA system

needs:

Suits with fewer distinct

components

Automatic checkout and servicing

Lower volume airlock/suit lock

Improved Don/Doff etc.

Life Science controls significant

portion of EVA overhead:

Prebreathe

Biomedical sensors

Nutrition and Hydration Systems

Additionally the EVA system

needs:

Suits with fewer distinct

components

Automatic checkout and servicing

Lower volume airlock/suit lock

Improved Don/Doff etc.

Exploration EVA Should Target WEI 3.0p g

Large Pressurized RoversLarge Pressurized Rovers

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Previous Lunar / Mars studies have proposed a Large

Pressurized Rover (LPR) to extend exploration range LPR designs complex and heavy, mass >8000kg Mobile landers may offer preferable solution to large scale

pressurized mobility

LAT-1 assumed only one LPR, delivered late in architecture Contingency Return Range: 240km

UPR with 24hrs of energy and consumables (+ margin)

on/behind the LPR provides 240km return capability 24-hr unpressurized translation

No SPE protection

Limited by allowable in-suit translation time (24hrs)


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Apollo LRV vs. Small Pressurized Rover DimensionsApollo LRV vs. Small Pressurized Rover Dimensions

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61259cm (102)

310cm (122) 183cm (72)

203cm (80)

Small Pressurized Rover Design Features (Slide 1 of 2)Small Pressurized Rover Design Features (Slide 1 of 2)

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Suitports: allows suit donning and

vehicle egress in < 10min withminimal gas loss

Work Package Interface:allows attachment of modularwork packages e.g. winch,cable reel, backhoe, crane

Ice-shielded Lock / FusibleHeat Sink: lock surrounded by2.5cm frozen water provides SPEprotection. Same ice is used as afusible heat sink, rejected heatenergy by melting ice vs.evaporating water to vacuum.

Chariot-Style Aft Driving

Station: enables crew to driverover while EVA, also part ofsuitport alignment

Two Pressurized Rovers: low mass, low volumedesign enables two pressurized vehicles, greatlyextending contingency return (and thus exploration)range

Suit PLSS-based ECLSS:reduces mass, cost, volumeand complexity of PressurizedRovers ECLSS

linklink


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Comparison of Unpressurized vs. Small Pressurized Rovers(1-day, 1 site sorties)

Comparison of Unpressurized vs. Small Pressurized Rovers(1-day, 1 site sorties)

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Range

from Base

(km)

Exploration

Area (km2)

Boots-on-

Surface EVA

Time (hrs)

Total EVA

Time (hrs)

Total

Crew

Time (hrs)

Total EVA

Time (hrs)

Total

Crew

Time (hrs)

% Reduction

in EVA

Hours

% Increase in

Exploration

Area

1 3 3.3 5.2 7.9 3.6 7.1 31%

10 314 3.3 7.0 9.7 3.6 8.9 49%

15 707 3.3 8.0 10.7 3.6 9.9 55%

20 1257 3.3 3.6 10.9

Not

possible w/

UPR

78%

30 2827 3.3 3.6 12.9

Not

possible w/

UPR

300%

40 5027 3.3 3.6 14.9

Not

possible w/

UPR

611%

Pressurized RoverUPR

Greater total crew time required with UPRbecause of suitlock depress time

Constraints are 8hr EVA and 15hr crew day LinkLink

Exploration Range: Unpressurized Rover vs. Large Pressurized Rovervs. Small Pressurized Rovers

Exploration Range: Unpressurized Rover vs. Large Pressurized Rovervs. Small Pressurized Rovers

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Large Pressurized RoverLarge Pressurized Rover

Range: 240kmRange: 240km

Small Pressurized RoversSmall Pressurized Rovers


Unpressurized RoverUnpressurized Rover


Lunar outpostLunar outpost


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Outpost

450km Small Pressurized Rovers 7450km Small Pressurized Rovers 7--day Sortie Example (1MPU)day Sortie Example (1MPU)

3 EVA sites per Small Pressurized Rover3 EVA sites per Small Pressurized Rover

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0.0 km. 150.0 km. 250.0 km. 500.0 km.Sortie Day Number: 0

Cumulative Distance: -

p

Sleep (9hr)EVA (3.25hr)

Outbound Route

Inbound Route


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Outpost

450km Small Pressurized Rover 7450km Small Pressurized Rover 7--day Sortie Example (1MPU)day Sortie Example (1MPU)


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0.0 km. 150.0 km. 250.0 km. 500.0 km.

1

2

Sortie Day Number: 2

Cumulative Distance: 277km


Outbound Route

Inbound Route


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Outpost



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0.0 km. 150.0 km. 250.0 km. 500.0 km.

2

3

1




Outbound Route

Inbound Route

21 4

EVA 1EVA 1

450km450km


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Outpost



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0.0 km. 150.0 km. 250.0 km. 500.0 km.

2

3

1




Outbound Route

Inbound Route

21

43

5

6

11

Outpost



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0.0 km. 150.0 km. 250.0 km. 500.0 km.

2

3

1




Outbound Route

Inbound Route

21

43

5

6

Sortie Duration 7 days

Crew 4 (2 per vehicle)

Distance Covered 909 km

EVA Time 10.75 Hours per crewmember

Boots-on-Surface Time 9.75 Hours per crewmember

Sites Surveyed 6 (3 per vehicle team)

Energy required (per vehicle) 307 KWh

Sortie Summary

Small Pressurized Rovers vs. Large Pressurized Rover:Weight and Range Comparison

Small Pressurized Rovers vs. Large Pressurized Rover:Weight and Range Comparison

2 x MPRVs 2 x 2657 5314 kg

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2 x Chassis C 2 x 1309 2618 kgTotal Mass 7932 kg

Max. Range (no MPUs) 189 km

Max. Range (2 MPUs) 960 km

1 x Large (LAT-1) Pressurized Rover 1 x 8006 8006 kg

1 x UPR (24hr capability assumed) 1 x 1180 1180 kg

Total Mass 9186 kg

Max. Range 240 km

Mass Difference: -1254kg (-13.7%)

Range Difference: +720km (+400%)


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Advantages of Small Pressurized RoversAdvantages of Small Pressurized Rovers

Operational / Engineering:

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Exploration:

Exploration range of up to 1000km (vs. 240km w/ largepressurized rover)

Shirt-sleeve envnmt with visibility as good as suited EVAs

Multi-spectral sensors & instruments always available

Single-person EVA capability

Potential for transfer under pressure from Ascent Moduleand/or hab (PLSSs kept in controlled envnmnt for re-use)

Reduced cycles on suit

Uses suit PLSS for life support

Potential for 4hr (lighter weight) PLSS- Mars forward

Potential to achieve Work Efficiency Index (WEI) of up to 9.0

for individual EVA excursions Reduces suit nutrition, hydration and waste mgmnt needs

Eliminates need for contingency walkback, decreasing designreqts for suit

>50% reduction in EVA time for equal or greater productivityand increased range

Health & Safety:

SPE protection within 20mins

Pressurized safe-haven within 20mins

DCS treatment within 20mins

Expedited on-site treatment and/or medication of injuredcrewmember

Reduces suit induced trauma

Better options for nutrition, hydration, waste management

Increased DCS safety, decreased prebreathe reqts throughintermittent recompression (would allow 3.5psi suit)

Provides resistive and cardiovascular exercise (75% VO2peak) during otherwise unproductive translation time

Better background radiation shielding vs. EVA suit

Dust control through use of suitport

Architectural:

2 Pressurized Rovers weigh less than single large pressurizedrover

Enables earlier delivery, possibly on crewed landers

Up to 12,000 kg H2O mass savings ( with Rover and PLSSHeat Sink)

1000kg+ O2 and N2 mass savings and up to 144 days lessdepress time using suitport vs. suitlock

Earlier long-duration crew missions

Aggressive development of Hab ECLSS less important

Gods-eye view capability (highly desirable for publicoutreach)

Vehicle design and required technologies highly relevant to

Mars missions

link

Small Pressurized Rovers AnimationSmall Pressurized Rovers Animation

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Suit Alignment Guides and Suitport Ingress/Egress

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Interiorbu

lkhead

Ring being

swiveled up

Stem rotated

90 so ring

faces suit

Ring being

swiveled up

Stem rotated

90 so ring

faces suit

Long guide

cone

Guide pinTurret at85

Suit Alignment Guides

Suitport Ingress / Egress

link

Consumables AssumptionsConsumables Assumptions

Conservative metabolic rates assumed:

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Light work = 10mL/kg/min, Heavy work = 20mL/kg/min

Sitting in Pressurized Rovers = 3.9mL/kg/min

Sitting in suit on UPR = 6.8mL/kg/min

Constant H2O consumption rates assumed:

In suit = 0.329 kg/hr

In Pressurized Rovers = 0.0 kg/hr (fusible heat sink)

In suit with fusible heat sink = 0.0 kg/hr

0

5

10

15

20

25

30

35

40

45

1 2 3 4 5 6 7 8

Speed (mph)

Metab

olicRate(ml/kg/min)

Moon, suite d

Earth, unsuite d

Moon, unsuited weighted

Moon, unsuite d

Metabolic Cost of Suit mass ,

pressure/volume/kinematics

Typical Science/Exploration EVATypical Science/Exploration EVA

Boots-on-Surface EVA Time

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Geologic context determination

(30mins)

Rock sample acquisition (15mins)

Soil sample acquisition (15mins)

Rake sample acquisition (15mins) Drive tube acquisition (15mins)

Core sample acquisition (1h 45mins)

= 3h 15mins per site

return

SummarySummary

These new ideas build on the results shown in December

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Better understanding of performance and capabilities

Preserving an open architecture approach

Capturing a broader range of Lunar objectives

New features and concepts to be discussed and comparedwith ideas from broader community- Commercial, Industry,Science, International

We are open to other new ideas for effective Exploration

Responsibility for development of lunar infrastructure still tobe determined through discussions with our partners inExploration

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exploration systems mission directorate (nasa)

Documents