lets phase 3 review 4/29/08
DESCRIPTION
LETS Phase 3 Review 4/29/08. Agenda. Team Introduction Daedalus Concept Concept of Operations Subsystem Overview Daedalus Performance Daedalus Vision Public Outreach Questions. Team LunaTech. Nick Case, Project Manager Morris Morell, Systems Engineer Travis Morris, GN&C - PowerPoint PPT PresentationTRANSCRIPT
LETS Phase 3 Review4/29/08
Agenda
• Team Introduction• Daedalus Concept• Concept of Operations• Subsystem Overview • Daedalus Performance• Daedalus Vision• Public Outreach• Questions
Team LunaTech• Nick Case, Project Manager• Morris Morell, Systems Engineer• Travis Morris, GN&C• Greg Barnett, Thermal Systems• Adam Garnick, Power Systems• Katherine Tyler, Power Systems• Tommy Stewart, Structures and Mechanisms• Julius Richardson, Conops• John Grose, Payload and Communications• Adam Fanning, Communications• Eric Brown, Technical Editor
Partners
• Mobility Concepts– Southern University
• Robert Danso• McArthur Whitmore
• Sample Return Vehicle Design– ESTACA
• Julie Monszajin• Sebastien Bouvet
CDD Requirements
Daedalus Lander
1.The Need
2.The Mission
3.The Solution
Daedalus Lander•Simple, Adaptable, Autonomous Lander
•Solar Cell and Li-Ion Battery Power
•Semi-passive Thermal System
•Ka-Band and UHF Communications System
•Lunar Penetrator Exploration System (LPES) “Fire and Forget”
Daedalus Heritage
Structure based on Viking Lander
Communication based on MER
Power System based on Mars
Phoenix & Venus Express
DSMAC Technology for
GN&C based on Cruise Missile
Penetrators based on LUNAR-A
Daedalus Mass Statement
Concept of Operations
LPESPayload•Micro-Seismometers
•Impact Accelerometer and Tilt Sensors
•Heat Flow Probe
•Geochemistry Package
•Water/Volatiles Detector
Design Requirements•1-1.2 Year Lifetime
•Impact Velocity: ~350 m/s
•Impact Force: ~4500 G’s
•Impact Depth: 1~2 m
•Scatter Distance: 500 m Penetration WebESTIMATED PENETRATOR SIZE
•Length: 480mm to 600mm
•Diameter: 60mm
•Estimated Mass: 14kg
LPES•22 Penetrators
•16 Launched into Shackleton Crater
•6 Launched into Lighted Region
•Spring-Loaded Ejection System
LUNAR-A
Daedalus ScienceDaedalus Payload Mass kg Power W Stereo imaging system or Radar or Lidar 0.8 6 Mast for stereo imaging system 3.5 9.5 Drill and drill deployment mechanism 20 30 Arm 13 43 Scoop 0.5 0 Mass Spectrometer 19 75 Geotechnical Experiments - cone penetrometer 1.5 0 Geotech - bearing plate 1 0 Geotech - shear vane 0.5 0 Magnets 0.5 0 XRD/XRF 2 10 Total 62.3 173.5 Estimated 168
Basic Requirements for Single Site Science Box:Determine Lighting conditions every 2 hours over the course of one yearStudy Micrometeorite fluxObserve Electrostatic dust levitation and its correlation with lighting conditions
Daedalus Power• Lithium Ion Batteries
– Total of 9 Sony 1860HC – Total mass of 42.24 kg– Total Volume of 1.341 ft^3
• Solar Cells– Total of 3 Gallium Arsenide Panels– Total mass of 46 kg– Total Surface area of 6.161 ft^3– Total Power of 937 Watts
• Power Regulation and Control– 6 Auxiliary Power Regulators. 2 per Solar Cell – 1 Battery Charge/Discharge Regulator per battery– ON Semiconductor LM350 Positive Voltage Regulators– STM Microelectronix ST0269 Digital Signal/Microprocessor– Crydom CMX60D10 Solid State Relays
Daedalus Thermal• Passive Techniques
• Paints – White and Black
• Multi-layered Insulation
• 15 layers
• Betacloth, aluminized Kapton
• Dacron Netting, Kapton laminate
• Thermal Switches
• Diaphragm Thin Plate Switch (Paraffin)
• Between heat generators and sinks
• Active Systems
• Electrical Resistance Heaters
• Tayco solid-state controller
• Variable Radioisotope Heater Units
• 50 Employed (50 Watts)
• Cassini-Huygens (117)
• 10 VRHU containers
• Variable Conductance Heat Pipes
• Aluminum(1.27cm) & Ammonia
• Integrated with radiator panels
• Axial groove composite wickMLI – exposed separator layers shown
GN&C
•Provides Completely Autonomous Landing sequence
•Very Precise landing location
•Landing location determined before launch
•Hazard Avoidance
Objective: To deliver Daedalus from 5km altitude safely and accurately to the lunar surface
Guidance CompBAE Systems
RAD6000
ACS 12 AeroJet
MR-108
Main Engines2 AeroJet
MR-80 IMUHoneywell HG1930
LiDARBall Aerospace
Long Range Optical Camera
Attitude thrust commands
Altitude thrust commands
high res photograph
Altitude signal
Surface terrain signals
attitude signals
Accelerometer signals
relative vel signal
Daedalus Communications
Earth Receiver and Transmitter
Lunar Penetrators
LRO
Penetrators to LRO using UHF
Data Rate: 2 Kbps
LRO to Earth using Ka-band
Data Rate: 100 Mbps
Daedalus to LRO using Ka-Band
Data Rate: 100 Mbps
View Time: 1 Hour per Day (approx)
Daedalus
Daedalus Structures
•A 8200 Newton load was applied to the foot of the leg assembly. •Loads were then transferred to the chassis•Results indicate the Minimum Factor of Safety is 1.15
Landing Scenario
Daedalus Structures
•To simulate loads experienced at launch a 54000 Newton load was applied.• Results indicate the Minimum Factor of Safety is 1.3
Launch Scenario
Daedalus PerformanceFigures of Merit Goal Daedalus
Number of surface objectives accomplished
15 Samples in permanent dark and 5 samples in lighted
terrain
16 Samples in permanent dark and 7 samples in lighted
terrain
Percentage of mass allocated to payload
Higher is better 40% of Dry Mass
Ratio of objectives (SMD to ESMD) validation
2 to 1 1.95 to 1
Efficiency of getting data in stakeholders hands vs. capability of mission
Higher is better 83.5 %
Percentage of mass allocated to power system
Lower is better 14% of Dry Mass
Ratio of off-the-shelf hardware to new
development hardware Higher is better 1.67 to 1
Daedalus Vision
1970 1980 1990 2000
Mariner
7 & 9
Viking
1 & 2
Mars Global Surveyor
Mars Pathfinder
2001 Mars Odyssey
Mars Express Orbiter
Mars Exploration
Rovers
Mars Reconnaissance
Orbiter
Mars Phoenix Lander
Mars Science Laboratory
Present
Mars Exploration Roadmap
Daedalus VisionProposed LPRP Timeline Using Daedalus
LCS
(2011)
LCROSS
(2008)
LRO
(2008)
Daedalus I
(2012)
Daedalus II
(2014)
SRV
(ESTACA)
Rover
(Southern)
Daedalus Vision
Daedalus I• Mission to Shackleton Crater• Lunar South Pole
Reconnaissance achieved by LPES
• Single Site Science Conducted• Scientific data used to justify
funding for Daedalus II
Daedalus II• Return Mission to Shackleton
Crater• Further Investigation based on
LPES findings• Robotic Rover and Sample
Return Vehicle Capability
Daedalus Vision
•Provide a basic, yet powerful and adaptable Lunar Exploration Transportation System
•Build upon the design practices and valuable data collected
•Evolve the Daedalus to accomplish each mission
•Provide a Low-Cost Solution for LPRP
This is the Vision for Daedalus…. and the Mission of
LunaTech
Public Outreach
• Union Hill School• May 8, 2008• 4th Grade• Presentation about
the Moon, LPRP and Daedalus
• Launch a Model Rocket
Questions
Thermal Backup 1MAE 491 Preliminary Calculations for Thermal Control SubsytemLETS Design, Team LunatechGreg Barnett
Ambient Temperature: -173 degC
Worst-Case Cold Scenario
1-D, Steady State Analysis
Information: kal 185.2watt
m K tins 1in tal
1
8in Ti 20 273( )K L 6in
kins_eff 2.5 105
BTU
hr ft R kins_eff 4.327 10
5watt
m K To 110K Tinf 100K
Tsur 100K Eheater 80watt A 20.5m2 tins 0.025m tal 3.175 10
3 m
Calculation of Cross-Sectional Area of Supports: Assumed 8 aluminum rods of 0.25in radius
r 0.25in Arod r2 rods 8 Ac Arod rods
Ac 1.013 103 m
2 Cross-Section of all supports
Thermal Backup 2
Effective Emittance:
fA1
100.373 log 3( )
fA 0.664 fN 1.164 For 15 layers
fP 1.322 For 2% Penetrations
Th 293 Tc 130
Tm
3Th
4Tc
4
4 Th Tc Tm 221.489 5.67108
eff 0.0001361
4 Tm2
0.000121Tm0.667
fN fA fP eff 0.017
Thermal Resistance: Rtotal
tal
kal A
tins
kins_eff A Rtotal 28.636
K
watt 5.6710
8watt
m2
K4
Thermal Backup 3
Energy Balance:
ERHU 50watt
Given
Ti To
Rtotaleff A To
4Tsur
4
Eheater ERHUTi To
Rtotalkal Ac
Ti To
L
To
Eheater
Find To Eheater To 134 C Temperature of outside surface
Erequired Eheater
Erequired 145watt Power required to maintain 20C inside vehicle
Thermal Backup 4
MAE 491 Preliminary Calculations for Thermal Control SubsytemLETS Design, Team LunatechGreg Barnett
Ambient Temperature: 100 degC / 373 K
Worst-Case Hot Scenario
1-D, Steady State Analysis
Albedo Assumed Negligible
Information: kal 185.2watt
m K tins 1in tal
1
8in L 6in Gsolar 1368
watt
m2
kins_eff 2.5 105
BTU
hr ft R kins_eff 4.327 10
5watt
m K Ti 20 273( )K Tsur 373K
A 20.5m2 tins 0.025m tal 3.175 10
3 m mli 0.15 mli 1 mli Atop 6.25m2
Thermal Backup 5
Effective Emittance for MLI:
fA1
100.373 log 3( )
fA 0.664 fN 1.164 For 15 layers
fP 1.322 For 2% Penetrations
Th 373 Tc 293 Hot and Cold Side Temperatures
Tm
3Th
4Tc
4
4 Th Tc Tm 334.594 5.67108
eff 0.0001361
4 Tm2
0.000121Tm0.667
fN fA fP eff 0.011
Thermal Resistancefor Conduction:
Rtotal
tal
kal A
tins
kins_eff A Rtotal 28.636
K
watt 5.6710
8watt
m2
K4
Thermal Backup 6Energy Balance:
To 400K
ERHU 50watt
EVCHP 150watt
Given
To Ti
RtotalmliGsolar Atop eff A To
4Tsur
4
ERHU
To Ti
Rtotal EVCHP
To
EVCHP
Find To EVCHP To 311C Temperature of outside surface
EVCHP 60watt Power that must be removed from cabin by VCHPs tomaintain 20 degC