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Space Interferometry Mission A NASA Origins Mission SIM C. Phillips August 11, 2006 -1 TFAWS - 2006 SIM PlanetQuest: The TOM-3 (Thermo-Optical-Mechanical) Siderostat Mirror Test C. Phillips August 11, 2006

C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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Page 1: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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Mis

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A NASAOriginsMission

SIM

C. Phillips August 11, 2006 -1TFAWS - 2006

SIM PlanetQuest: The TOM-3 (Thermo-Optical-Mechanical)

Siderostat Mirror Test

C. Phillips

August 11, 2006

Page 2: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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Mis

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A NASAOriginsMission

SIM

C. Phillips August 11, 2006 -2TFAWS - 2006

Agenda

• SIM Spacecraft Overview- Collector Subsystem Description- Siderostat Mirror Description

• Collector Bay Environment• TOM-3 Test Configuration• Integrated Model Description• Conclusion

Page 3: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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A NASAOriginsMission

SIM

C. Phillips August 11, 2006 -3TFAWS - 2006

SIM PlanetQuest – Mission Description

Designed to Detect Earth-Like Planets (as Small as 4 Earth Radii) Around 250 Nearest Stars

Will Also Catalog Positions of 1300 Nearest Stars with Micro-Arc-Second Resolution.

3 Michelson Interferometers Operating in Visible Wavelength

10-meter Science Baseline

5 Year Primary Mission with 10 Year Goal

Earth Trailing Orbit (0.95 to 1.1 AU)

Complex Opto-Mechanical Systems

mK-Level Thermal Stability on Select Components

Page 4: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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A NASAOriginsMission

SIM

C. Phillips August 11, 2006 -4TFAWS - 2006

SIM Instrument ConceptS/C Bus

Collector Bay 1

Collector Bay 2

PSS

3.28m

2.52m

2.56m

COL Bay Apertures (Solar Exclusion Plane)

•S/C MLI Not Shown: Outer Layer is 2nd Surface Kapton, ε = 0.78, α = 0.45

•Solar Distance: 0.95 to 1.1 AU (1515 W/m2 to 1130 W/m2)

Page 5: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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C. Phillips August 11, 2006 -5TFAWS - 2006

SIM Collector Bay Concept

SID Outer Gimbal, PID Kapton Film Heaters, MLI, 25 mK/hr

Wide Angle Stability Requirements in Bold

SID Mirror, Aluminum Thermal Can, PID Kapton Film Heaters, MLI, 25 mK/hr

Science Compressor Bench, Kapton Film PID Surface Heaters, MLI Blanketing, 100 mK/hr

Page 6: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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SIM

C. Phillips August 11, 2006 -6TFAWS - 2006

SIM Collector Siderostat Mirror Design Concept

One Mirror Located in Each Collector Bay

Articulating Mirror (Coarse Stage Can Rotate Mirror +/- 3.5o

Used to Acquire Target Starlight and Direct it Toward Science Light Compressor

35-cm Flat Mirror

25 mK/hr Thermal Stability

22C +/- 5C Absolute Temperature Requirement

Identified Early on in Technology Program as a High Risk Item

Subject of TOM-3 Thermo-Optical-Mechanical Test

Brassboard SID

Latest Flight SID Incarnation

Page 7: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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C. Phillips August 11, 2006 -7TFAWS - 2006

COL Bay Thermal Environment (1 of 2)Primary Boundary Temperature for COL Bay Components is NGST COL Bay Enclosure Inner MLI Temperature and Aperture to Space

The COL Bay is Isolated from the Rest of the Instrument with MLI Blanketing

Range for COL Bay Inner MLI Absolute Temperature is Driven By Solar Loading Vector, Solar Flux, and Materials Degradation

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C. Phillips August 11, 2006 -8TFAWS - 2006

COL Bay Thermal Environment (2 of 2)

}Goal of Thermal Design is to Minimize Temps Inside COL Bay in Order to Minimize Radiative Heat Transfer

OUTBOARD BAY LEFT PANEL MLI INTERIOR LAYER TEMP DURING S/C SLEWING (SUNLIT BOTTOM TO SUNLIT SIDE)

-80

-79

-78

-77

-76

-75

-74

-73

-72

-71

-70

100 105 110 115 120 125

TIME [HR]

TEM

P [D

EG. C

]Series1Series2Series3Series4Series5Series6Series7Series8Series9Series10Series11Series12Series13Series14Series15Series16Series17Series18

Sample Transient Boundary Prediction

Page 9: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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C. Phillips August 11, 2006 -9TFAWS - 2006

TOM-3: Replicating COL Bay Environment

Note: Right and Top Shroud/Heater Plate Panels Not Shown

Shroud Heater Plates (150K to 220K)

Shroud LN2 Plates (90K)

Chamber Ambient Environment (293K)

Brassboard SID Assembly (Mirror Approx. 293K)

Page 10: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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BB-SID Test Setup Photos

SID on bottom heater plate

Typical panel with large heaters

LN2 shroud and chopping mirror in chamber

Page 11: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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BB-SID Vacuum Chamber Configuration

Shroud

Page 12: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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C. Phillips August 11, 2006 -12TFAWS - 2006

Thermal Hardware - SID Heater Control• The SID mirror assembly is temperature controlled by the following four heater

circuits.- Aft Thermal Can. The Aft Can is isolated from the shroud environment by a 20-layer

MLI blanket and has a low-e inner coating to attenuate temperature fluctuations. 7 individual patch heaters are installed in series on the Aft Can and are controlled by a PID heater control algorithm.

- Forward Thermal Can. The purpose of the forward heater can is to reduce lateral gradients across the mirror face. The forward can circuit has three individual patch heaters wired in series, and is PID controlled.

- SID Support (Vertical). The vertical portion of the SID support has five individual heater patches and is PID controlled.

- SID support (Base). The horizontal portion of the SID Support has one heater patch and is also PID controlled.

Circuit 1, Aft Thermal Can

Torlon Thermal Isolator

Circuit 2, Fwd Thermal Can

Mirror

SID Support Vertical

SID Support Base

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How Does Thermal Drive Changes in OPD?

( )22

4 io rrhTOPD +

Δ=

α

α= CTE (+/- 5 Parts/Billion for ULE)

ΔT = Axial Temperature Gradient

h = Mirror Thickness

Ro = Mirror Outer Radius

Ri = Mirror Inner RadiusChanges in OPD Over Time Degrade Optical Performance

Goal of TOM-3 is to Measure and Predict ΔOPD/dt

ro

ri

Page 14: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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Ideas TMG Thermal and Structural Models

Temperature Mapping

Thermal Model

21600 Elements

13600 Nodes

Structural Model

47000 Elements

168000 Nodes

Page 15: C. Phillips SIM August 11, 2006 - TFAWS 2020 · TFAWS - 2006 C. Phillips August 11, 2006 -12 Thermal Hardware - SID Heater Control • The SID mirror assembly is temperature controlled

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SID Sample Steady State Temperature Map

Important Temperature

Gradient

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SID Sample Transient Results/Test Data

TOM Tech Gate 8 - SID Mirror d-Delta-T/dt (SIDBCK3-SIDBCKR2) - Inboard Bay, Narrow Angle Test, 6/5/2005

-2

-1.5

-1

-0.5

0

0.5

1

1.5

2

0 5 10 15 20 25 30 35 40

Test Duration (hr)

d-De

lta-T

/dt (

mK/

hr)

SIDBCK3-SIDBCKR2, Test

SIDBCK3-SIDBCKR2, Correlated Model

SIDBCK3-SIDBCKR2, Uncorrelated Model

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C. Phillips August 11, 2006 -17TFAWS - 2006

Conclusions and Lessons Learned

• Flight Thermal Environment was Successfully Replicated • Measured Siderostat Optical Performance Met Optical Requirements by

a Wide Margin. • Despite a Good Thermal Model Correlation, Uncertainties in Material

Properties Complicated Structural Correlation (assumed ULE CTE of +/-5 ppm, Recently Measured at +30ppm)

• ULE Bool Had Non-Homogeneous CTE (Homogeneous ULE Assumed in Model)

• MLI Blanket Seams Complicated Thermal Model Correlation (Used Average e* of 0.05 where e* was More Like 0.1 Near Seams)

• Thermal Model Probably did not Need to be so Detailed. Mesh Size was Selected Using a Grid Refinement Study and TMG Benchmarking Studies.