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National Aeronautics and Space Administration www.nasa.gov 1

Solar Power for Outer Planets Study Solar Power for Outer Planets Study

Presentation to Outer Planets Assessment Group November 8, 2007

Scott W. Benson/NASA Glenn Research Center

National Aeronautics and Space Administration

www.nasa.gov

(2)

Background & Outline Background & Outline

• Alan Stern request: “…a quick look study for how we could extend the Juno and Rosetta 5 AU-class

missions on solar arrays to enable solar array missions at Saturn (10 AU) and Uranus (20 AU)”

• • Study Process Study Process

• • Cell and Array Technology Findings Cell and Array Technology Findings

• • Power System Sizing Power System Sizing

• • Mission and System Integration Studies Mission and System Integration Studies

• • Technology Planning Technology Planning

• • Conclusions Conclusions

(3)

National Aeronautics and Space Administration www.nasa.gov 3

•• DawnDawn

36.4 m2 planar array area10.3 kW at 1 AU

1.3 kW at 3 AU (-88 °C)Triple Junction cells

•• JunoJuno

Phase B design

45 m2 planar array area9.6 kW BOL at 1 AU

414 W at 5.5 AU (-130 °C)Triple Junction cells

•• RosettaRosetta

61.5 m2 planar array area7.1 kW BOL at 1 AU

400 W at 5.25 AU (-130 °C)Silicon Hi-ETA cells

Most Distant Use of Solar Arrays

Most Distant Use of Solar Arrays

(4)

Study Process Study Process

• • Review prior studies and flight system publications Review prior studies and flight system publications

• • Assess PV cell and array technologies Assess PV cell and array technologies

• • Understand cell performance in outer planet applications Understand cell performance in outer planet applications

• • Analyze power system performance Analyze power system performance

• • Coordinate with technology, vendor and user community Coordinate with technology, vendor and user community through workshop at Space Photovoltaic Research &

through workshop at Space Photovoltaic Research &

Technology (SPRAT) Technology (SPRAT)

• • Coordinate with Juno project Coordinate with Juno project

• • Characterize system integration considerations Characterize system integration considerations

• • Define technology paths Define technology paths

(5)

National Aeronautics and Space Administration www.nasa.gov 5

Solar Cell Technology Findings Solar Cell Technology Findings

Solar Cell Capability Solar Cell Capability

• Nominal low intensity, low temperature (LILT) state-of-the-art (SOA) cell

performance is viable at 5 AU and beyond Cell efficiency increases with lower

temperature but decreases with lower intensity

• LILT Effect: off-nominal drop in cell performance, must be mitigated to effectively use solar power in outer solar system

Understood and mitigated on earlier silicon cells

Effect observed on SOA multi-junction (MJ) cells, cause not yet identified

ƒ Cell-to-cell variation

LILT Effect can be mitigated:

ƒ Cell screening, optimization or advanced concentrator technology

• On-going advances in cell technology can provide improvements NASA will need to adapt those to LILT conditions

GRC FY07 LILT IRAD testing results

Low Light Triple Junction Performance

18 20 22 24 26 28 30 32 34 36

-180 -160 -140 -120 -100 -80 -60 -40 -20 0 20 40

Temperature ( C

1 AU 5.6 AU 22.1 AU

(6)

Applicable Technologies

Applicable Technologies Solar Cells Solar Cells

•• State-State-ofof--art performance at 1AU (AM0, 25C)art performance at 1AU (AM0, 25C) Multi-junction III-V cells, triple-junction: 28 - 30%

Silicon: 16 - 19%

Thin-film: not space-qualified (6 - 10% currently)

•• Expected advances in cell performanceExpected advances in cell performance Multi-junction: 30 - 33% in next 3 years

ƒ Development pursued by both cell vendors

ƒ Driven by military/commercial applications

ƒ 35 - 40% cell design under development

Multi-junction: mass and cost reduction

ƒ Thinned substrate or no-substrate technology to drastically reduce cell/array mass

ƒ Reusable substrates and improved manufacturing to increase yield and reduce cost

•• Advanced cell approachesAdvanced cell approaches

Cells designed or optimized for outer solar system missions

ƒ Eliminate LILT Effect in future MJ cell generations

ƒ Optimize cells for bandgap narrowing at low temperatures

Quantum dots, nanotechnology to increase efficiency

ƒ Far-term: efficiency increase through better utilization of solar spectrum

Projected Efficiency for MJ Solar Cells

10 15 20 25 30 35

1990 1995 2000 2005 2010

Year

Projected Efficiency for MJ Solar Cells

10 15 20 25 30 35

1990 1995 2000 2005 2010

Year

(7)

National Aeronautics and Space Administration www.nasa.gov 7

Solar Cell LILT Effects Solar Cell LILT Effects

Data collected at GRC on SOA MJ production- line cells

Cause of LILT Effect has not been identified for multi-junction III-V cell technology

Occurs on a cell-to-cell basis

Magnitude of effect is not currently predictable

Little research has been done in this area, none to understand root cause of problem

0 0.001 0.002 0.003 0.004 0.005 0.006 0.007 0.008 0.009

0 0.5 1 1.5 2 2.5 3 3.5

Voltage (V)

Blue Curve Data FF = 64.1%

Efficiency ~ 24.8 %

Red Curve Data FF = 77%

Efficiency ~ 29.8 % Intensity = .02 Suns (7 AU)

Temperature = -150°C

LILT Effect

(8)

LILT Effect Mitigation LILT Effect Mitigation

Cell Screening

• Successful on Dawn

• In progress for Juno

• GRC and Juno data indicate that effect worsens in frequency and magnitude

with lowering intensity

Cell screening may not be applicable beyond Jupiter

Cell Optimization

Silicon cells designed for LILT on Rosetta

5.2 AU, -130 °C

Future cells could be optimized

To eliminate LILT Effect

To optimize cell performance and mass for LILT conditions

Concentration

Maintains intensity

Minimizes LILT Effect

Reduces cell count

Increased spacecraft system effects (pointing requirements)

Low Light Triple Junction Performance

18 20 22 24 26 28 30 32 34 36

-180 -160 -140 -120 -100 -80 -60 -40 -20 0 20 40

Temperature ( C

1 AU 5.6 AU 22.1 AU

5% cell efficiency benefit at Saturn with 8X concentration

(9)

National Aeronautics and Space Administration www.nasa.gov 9

Array Technology Findings Array Technology Findings

Advanced Solar Array Technology Advanced Solar Array Technology

• Multiple technical paths exist to extend photovoltaic power use towards the outer solar system

• UltraFlex

Near-term, high maturity Baseline for Orion power

ƒ TRL6 by 2009 with subsequent qualification

• SquareRigger

Mass competitive at large power levels

Rectangular bays offer better scaling characteristics Compatible with planar and concentrator designs

• Stretched Lens Array SquareRigger (SLASR)

Incorporates lightweight linear refractive concentrator derived from Deep Space 1 SCARLET

SLA component flight demonstration on TACSAT-4 Can scale to very high power levels

• Technology development is required:

To extend UltraFlex diameter beyond state-of-art size

To complete SquareRigger development at the array level

UltraFlexWing

SLASR Bay 2.5 x 5m

(10)

0 100200 300 400 500600 700800 1000900 11001200 1300 1400 15001600 1700 1800 19002000 2100 2200 23002400 2500

5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20

Distance (AU)

Power (W)

SLASR: 179 kg, 211m^2(~18bays) SLASR: 89 kg, 105m^2(~10bays)

Four wing, 6 m diameter Ultraflex: 179 kg, 113 m^2 Planar Squarerigger: 179 kg, 86m^2(~8bays) Two wing, 6 m diameter Ultraflex: 89 kg, 56 m^2 Planar Squarerigger: 89 kg, 43m^2(~4bays)

0 100200 300 400 500600 700 800 1000900 11001200 1300 1400 15001600 1700 1800 19002000 2100 2200 23002400 2500

5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20

Distance (AU)

Power (W)

SLASR: 179 kg, 211m^2(~18bays) SLASR: 89 kg, 105m^2(~10bays)

Four wing, 6 m diameter Ultraflex: 179 kg, 113 m^2 Planar Squarerigger: 179 kg, 86m^2(~8bays) Two wing, 6 m diameter Ultraflex: 89 kg, 56 m^2 Planar Squarerigger: 89 kg, 43m^2(~4bays)

Near Term Capability:

Near Term Capability:

Power from a Fixed Power System Mass Power from a Fixed Power System Mass

Solar array options are sized to be the same mass as the two andfour wing Ultraflex arrays.

Solar array mass includes hardware outboard of gimbal

SquareRigger standard bay size of 2.5 m by 5 m

2.5 yr gravity assist period + 2 years at AU location + 2 AU/year transit time

Heliocentric space (no planetary radiation effects)

Useful power will be lower based on

planetary eclipses/

radiation degradation

SOA cell efficiency of 30% at 1 AU

LILT Effect-free cells

8X concentration with SLASR

*

Juno

- SOA cells - planar array - mass not

normalized

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National Aeronautics and Space Administration www.nasa.gov11

System Integration Considerations System Integration Considerations

•• Mass impacts of carrying the solar array into deep spaceMass impacts of carrying the solar array into deep space

Additional/larger systems: solar array, batteries, power conditioning systems, pointing systems (larger reaction wheels)

Heavier thermal systems (lack of RPS waste heat) Structures/mechanisms to attach the solar arrays

(impact from capture propulsion system)

Net impact is reduced payload compared to RPS systems

•• Launch vehicle integrationLaunch vehicle integration

Volume constraints in packaging stowed arrays

•• Spacecraft integration and operations in mission orbitSpacecraft integration and operations in mission orbit

Multiple subsystem requirements for pointing and slew Possible incompatibilities with science objectives

•• Power system designPower system design

Maintaining power through eclipse periods Radiation tolerant design

Managing power in inner solar system, when generated power from array can be 10’s - 100’s of kW

(12)

Mission Applications Mission Applications

•• A range of missions were considered to encompass power system siA range of missions were considered to encompass power system sizing zing and spacecraft integration drivers, including:

and spacecraft integration drivers, including:

Heliocentric distance: 5 -Heliocentric distance: 5 - 20 AU20 AU

Operations concept & power management: moon orbitersOperations concept & power management: moon orbiters Radiation: Radiation: Jovian moon orbiterJovian moon orbiter

Simplest missions: flybysSimplest missions: flybys

•• FlagshipFlagship-class-class

Saturn Orbiter, Titan Orbiter Uranus Orbiter

Ganymede or Europa Orbiter

•• PIPI--ledled

Saturn Flyby

Centaur Flyby or Rendezvous

•• Saturn Orbiter analyzed in COMPASS team studySaturn Orbiter analyzed in COMPASS team study

Used GSFC Enceladus architecture option Saturn-OL as reference

•• EuropaEuropa, Centaur and Uranus missions assessed analytically, Centaur and Uranus missions assessed analytically

Representative point analyses performed with selected mission power

(13)

National Aeronautics and Space Administration www.nasa.gov13

Example: Saturn Orbiter Mission Example: Saturn Orbiter Mission

Mission assumptions:Mission assumptions:

Titan/Enceladus cycling orbit

335 W continuous nominal power (per Enceladus study) 11.5 yr VVEEGA voyage to Saturn

Saturn and rings eclipse periods Total radiation degradation of 15%

Power system design optionsPower system design options

SOA cells/array:

ƒ Nine SLASR bays at 237 kg

ƒ Twelve Planar Squarerigger bays at 470 kg

ƒ Four, 7.2 m diameter Ultraflex arrays at 415 kg Projected cells/array:

ƒ Eight SLASR bays at 205 kg

ƒ Ten Planar Squarerigger bays at 321 kg

ƒ Four, 6.7m diameter Ultraflex arrays at 268 kg

System-System-level driverslevel drivers

COMPASS study performed to assess system drivers, details follow

Technology feasibilityTechnology feasibility

Target power level can be achieved with near-term PV technology

Near-SOA Ultraflex Arrays SOA MJ Cell Performance

48 kW BOL at 1 AU Interplanetary voyage 377 W at Saturn arrival

- Planetary radiation - Energy storage for

eclipse periods

335 W EOL power 40 m2

(14)

Other Missions Other Missions

System

System--level driverslevel drivers

Radiation and eclipse power level

Orbital operations and pointing requirements

Technology feasibility Technology feasibility

SLASR and UltraFlex provide feasible paths

Four, 7.0 m diameter Ultraflex arrays at 513 kg

Requires detailed radiation degradation trade study

Advanced SLASR Arrays Advanced SLASR Arrays SOA MJ Cell Performance SOA MJ Cell Performance 45 kW BOL at 1 AU, 362 kg

Interplanetary voyage 1400 W at Jupiter arrival -Planetary radiation, 30%

total degradation -Energy storage for

eclipse periods 720 W EOL at Europa

50 m2

Europa Orbiter Europa Orbiter

SOA

SOA Ultraflex Ultraflex ArraysArrays SOA MJ Cell Performance SOA MJ Cell Performance 33 kW BOL at 1 AU, 287 kg

Interplanetary voyage 300 W EOL at Echeclus

27 m2

System

System--level driverslevel drivers

Similar to Saturn Orbiter study

Technology feasibility Technology feasibility

Target power level can be achieved with near-term PV technology

Advanced SLASR Arrays Advanced SLASR Arrays Projected MJ Cell Performance Projected MJ Cell Performance 95 kW BOL at 1 AU, 327 kg

Interplanetary voyage 200 W EOL at Chiron

100 m2

Centaur:

Centaur: EcheclusEcheclus Centaur: ChironCentaur: Chiron

System

System--level driverslevel drivers

Array size amplifies all spacecraft integration considerations Technology feasibility Technology feasibility

Technology is achievable

Significant changes in spacecraft concept required

Advanced SLASR Arrays Projected MJ Cell Performance

232 kW BOL at 1 AU, 781 kg Interplanetary voyage 400 W EOL at Uranus

250 m2

Uranus Orbiter Uranus Orbiter

System

System--level driverslevel drivers

Array size amplifies all spacecraft integration considerations Technology feasibility Technology feasibility

Significant changes in spacecraft concept required

(15)

National Aeronautics and Space Administration www.nasa.gov15

Solar Saturn Probe Design Study Solar Saturn Probe Design Study

•• Reference ASRG-Reference ASRG-powered spacecraftpowered spacecraft

Power: 335 W 3 ASRGs

Science payload: ~1000 kg, includes lander

•• Solar-Solar-powered spacecraftpowered spacecraft

48 kW solar arrays at 1AU Science payload: ~550 kg

Solar Powered Subsystem

Mass Change Compared

to RPS probe Cause

Payload -450 kg Increase in bus subsystems mass

Power + 340 kg Solar arrays, mechanisms, PMAD

ACS + 30 kg Heavier wheels (ACS propellant increased)

C&DH/Comm + 15 kg Increase in pointing, more complex spacecraft operations

Thermal + 30 kg Additional blankets, heaters, RHUsdue to lack of waste heat for RPS

Structures + 30 kg Solar array booms

(16)

National Aeronautics and Space Administration www.nasa.gov

Power at Saturn:

Interplanetary-only (no

eclipses, planetary radiation)

Fixed mass power system

Key Technology:

Key Technology:

Cell Improvements Cell Improvements +5% eff., lower mass

+58% Power

SLASR/SOA Cells SLASR/SOA Cells

360 W

360 W, 233 kg, , 233 kg, 9 bays (2.5 m x 5 m) 9 bays (2.5 m x 5 m)

SLASR/

SLASR/

Projected Cells Projected Cells 420 W

420 W, 233 kg, , 233 kg, 9 bays (2.5 m x 5 m) 9 bays (2.5 m x 5 m) Key Technology:

Key Technology:

Lightweight Arrays Lightweight Arrays +80% Power

+110% Power

Power improvements achievable through technology investment

Power improvements achievable through technology investment

Technology Leverage Summary Technology Leverage Summary

Underlying Development and Technologies Underlying Development and Technologies

Qualify UltraFlex for low temperature application LILT Effect Evaluation for MJ Cells

Blanket Technologies for Low Temperature Conditions

UltraFlex

UltraFlex/ / SOA Cells

SOA Cells 200 W

200 W, 233 kg, , 233 kg, 4

4 wings, wings, 5.

5.4 m diameter4 m diameter

UltraFlex/

Projected Cells 316 W, 233 kg,

4 wings, 6.3 m diameter

(17)

National Aeronautics and Space Administration www.nasa.gov17

Conclusions Conclusions

•• Near-Near-term term UltraflexUltraflex arrays and SOA multi-arrays and SOA multi-junction cells can provide junction cells can provide capability to perform low power (200

capability to perform low power (200--300 W) missions out to 10 AU300 W) missions out to 10 AU 300 W mission to an inner Centaur appears achievable300 W mission to an inner Centaur appears achievable

•• Further investigation of LILT Effect is warranted if PV power isFurther investigation of LILT Effect is warranted if PV power is to be to be considered for more demanding outer planet missions

considered for more demanding outer planet missions LILT Effect can be avoided through multiple approachesLILT Effect can be avoided through multiple approaches

•• Advanced cell and array technologies would extend the practical Advanced cell and array technologies would extend the practical application of PV power through mass and efficiency benefits

application of PV power through mass and efficiency benefits

Clear technology paths exist to enhance PV application to outer Clear technology paths exist to enhance PV application to outer planet planet missions

missions

•• Implementation of PV power will decrease payload massImplementation of PV power will decrease payload mass

•• Feasibility of PV use critically depends on mission and spacecraFeasibility of PV use critically depends on mission and spacecraft ft concept

concept

References

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