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Page 1 of 8 QCM THERMO-GRAVIMETRIC ANALYSIS (QTGA) COMPARISONS Glenn Rosecrans and George Meadows Swales Aerospace 1 , Beltsville, MD ABSTRACT The ASTM E-1559 apparatus has been used for years at NASA/Goddard Space Flight Center (GSFC) to determine in situ outgassing rate information, as well as pertinent in situ TML and multiple VCM values. The apparatus also affords the opportunity to experimentally compute the evaporation rates of molecular species that are reemitted as the Quartz Crystal Microbalances (QCMs) are gradually warmed up at some controlled temperature. Typically the molecular mass that accumulates onto the test QCMs are a compilation of species that are outgassing from the sample due to their respective activation energies and the desorption processes that the sample undergoes at various tested temperatures. It has been speculated that if there is too much molecular buildup of condensed water vapor (ice) onto the QCM crystal that a significantly higher temperature would be needed to break these “ice” bonds. ASTM E-1559 data plots will be used to demonstrate the thermogravimetric effects of water and other miscible molecular species with various water/ice thicknesses and at different evaporation rates. INTRODUCTION The ASTM E-1559 setup at NASA/GSFC utilizes 4 QCMs to collect a molecular mass at 4 different temperature ranges. The coldest QCM is typically cooled to near liquid nitrogen (LN2), at ~90K, and condense most water vapor that impinges onto it and most other heavier weighted outgassed molecules from the sample. The other QCMs are typically set to common temperatures, warmer than the water condensation temperature under high vacuum (<1E-6 Torr). A variety of common aerospace materials and candidate samples were considered for this investigation. These samples have been exposed in the Molekit2 system within the past 2 years. The samples selected for this evaluation considered a variety of materials and varied the water accumulation rate from 100’s of Hertz to 10000’s of Hertz over a test period of 24 to over 100 hours. The reemission process, mass evaporating from the QCM crystal, was also performed with a steady increase in temperature. Under high vacuum the normal range that deposited water vapor begins to evaporate is around - 125C. If there is 50,000 Hz or ~10,000 Angstroms (1000 nm) of accumulation on the QCM crystal does the water vapor take substantially longer to evaporate/reemit because of the thicker layer of contaminate? Does the thermogravimetric effects of water differ when other miscible molecular species are present? ABBREVIATIONS and ACRONYMS ASTM American Society of Testing Materials CCD Charged Couple Device GSFC Goddard Space Flight Center EC Effusion Cell LN2 Liquid Nitrogen Molekit Molecular Kinetics NASA National Air & Space Agency QCM Quartz Crystal Microbalance QTGA QCM Thermogravimetric Analysis RGA Residual Gas Analyzer ________________________________________________________________________________________ 1 work was performed under a Swales MSES contract with NASA/GSFC #NAS5-01090

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Page 1: Page 1 of 8 - NASA

Page 1 of 8

QCM THERMO-GRAVIMETRIC ANALYSIS (QTGA) COMPARISONS

Glenn Rosecrans and George MeadowsSwales Aerospace1, Beltsville, MD

ABSTRACT

The ASTM E-1559 apparatus has been used for years at NASA/Goddard Space Flight Center (GSFC) todetermine in situ outgassing rate information, as well as pertinent in situ TML and multiple VCM values. Theapparatus also affords the opportunity to experimentally compute the evaporation rates of molecular species thatare reemitted as the Quartz Crystal Microbalances (QCMs) are gradually warmed up at some controlledtemperature. Typically the molecular mass that accumulates onto the test QCMs are a compilation of speciesthat are outgassing from the sample due to their respective activation energies and the desorption processes thatthe sample undergoes at various tested temperatures. It has been speculated that if there is too much molecularbuildup of condensed water vapor (ice) onto the QCM crystal that a significantly higher temperature would beneeded to break these “ice” bonds. ASTM E-1559 data plots will be used to demonstrate the thermogravimetriceffects of water and other miscible molecular species with various water/ice thicknesses and at differentevaporation rates.

INTRODUCTION

The ASTM E-1559 setup at NASA/GSFC utilizes 4 QCMs to collect a molecular mass at 4 differenttemperature ranges. The coldest QCM is typically cooled to near liquid nitrogen (LN2), at ~90K, and condensemost water vapor that impinges onto it and most other heavier weighted outgassed molecules from the sample.The other QCMs are typically set to common temperatures, warmer than the water condensation temperatureunder high vacuum (<1E-6 Torr). A variety of common aerospace materials and candidate samples wereconsidered for this investigation. These samples have been exposed in the Molekit2 system within the past 2years. The samples selected for this evaluation considered a variety of materials and varied the wateraccumulation rate from 100’s of Hertz to 10000’s of Hertz over a test period of 24 to over 100 hours. Thereemission process, mass evaporating from the QCM crystal, was also performed with a steady increase intemperature. Under high vacuum the normal range that deposited water vapor begins to evaporate is around -125C. If there is 50,000 Hz or ~10,000 Angstroms (1000 nm) of accumulation on the QCM crystal does thewater vapor take substantially longer to evaporate/reemit because of the thicker layer of contaminate? Does thethermogravimetric effects of water differ when other miscible molecular species are present?

ABBREVIATIONS and ACRONYMS

ASTM American Society of Testing MaterialsCCD Charged Couple DeviceGSFC Goddard Space Flight CenterEC Effusion CellLN2 Liquid NitrogenMolekit Molecular KineticsNASA National Air & Space AgencyQCM Quartz Crystal MicrobalanceQTGA QCM Thermogravimetric AnalysisRGA Residual Gas Analyzer

________________________________________________________________________________________1 work was performed under a Swales MSES contract with NASA/GSFC #NAS5-01090

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SYMBOLS

Å Angstrom cm2 square centimeteroC degrees Celsius g gramHz Hertz K degrees Kelvin nm nanometer (1 nm = 1E-9 m = 10Å)

EXPERIMENTAL METHODS/SETUP

The GSFC setup for the ASTM E-1559 test procedure provides outgassing information and reemissiondata for evaluating spacecraft materials. The setup does have a limitation to the sample size. Currently theeffusion cell can fit samples that are ~1” by ~1.5” by ~2”. The effusion cell has an orifice diameter of ~1/8” andis located on the top of the “can”. The EC can be heated rather instantaneously by heaters attached to the side,up to 300oC. The effusion cell can also be cooled and maintained at temperatures below ambient. One sample,included in this analysis was tested as low as –20oC, which involved attaching several thermal straps from theLN2 chamber to the EC and then adjusting the EC heaters as required. A schematic of the GSFC Molekit systemis shown below in Figures 1A and 1B. GSFC has 2 molecular kinetics facilities for performing E1559 tests,which are practically identical, Molekit2 and Molekit3, respectively. Samples for this investigation includesamples tested from both systems, which had the same QCM set cold for all samples.

Figure 1A Figure 1BMolekit 2 &3 Shroud configuration Typical sample introduction from

The Interlock Chamber to Test chamber

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The following is brief explanation of the Molekit test procedure. This is described in more detail in theactual ASTM E1559 procedure (ref. 1). GSFC follows the Test Method B option for most samples. Apreweighed sample is placed inside an effusion cell in the Interlock chamber, which is at ambient pressure andambient temperature. Once the QCMs, located in the Main chamber and under high vacuum, have stabilized attheir desired setpoints, a slight vacuum is pulled on the Interlock chamber to ~1E-3 Torr, which occurs ratherquickly (within minutes). The isolation value is then opened and the sample is manually slide to a setpointelevation inside the Test chamber, which places the EC orifice ~6” away from the QCM crystal elevation. TheEC is set to the desired temperature setpoint and outgassing from the sample through the orifice to the QCMsensues. The outgassing from the sample exits the orifice in a lambertian manner. The four (4) QCMs arepositioned approximately 6” away and centered equidistant from the 0.125” diameter EC orifice. The resultantviewfactor or form factor of the orifice to the QCMs for the GSFC Molekit 2 setup has been determined to be635 cm2. (M3 was 610 cm2). This setup is a line-of-sight (LOS) transport, with little to no reflected moleculesaffecting the net molecular gain by the QCMs. The chamber walls and QCM sink plate are flooded with LN2and thus capture molecular mass that are dispersed from the orifice at angles more than ~5o from normal. TheQCM shield is thermally coupled to the QCM sink plate and provides an additional protection from chambershroud accidental warm-up, due to LN2 outage. The GSFC setup typically sets the 4 QCM Research QCMs to–183oC (90K), -113oC (160K), -60oC (213K), and –20oC (253K). The coldest QCM is capable of condensingwater vapor and most other light weight molecular species. The chamber vessel typically obtains vacuum levelsof 1E-6 Torr or lower and water theoretically condenses at ~-116oC at this pressure and lower with attainment ofbetter pressures. Setting the 2nd coldest QCM to a level just above water condensation affords the attainment ofthe outgassing rate trend data for all non-water molecule species. The other temperature settings allow forcomputation of fractional condensing material. Since these are common setpoint temperatures for each sample,the same QCM is typically set to the same temperature. Therefore the QCMs have a history of condensingmolecular mass at a common temperature. The coldest temperature setpoint has been the same QCM for allthese comparisons. The following table indicates the QCM Research QCM type and serial numbers, and theircommon temperature setpoints for the Molekit 2 &3 system.

Table 1QCM serial numbers and common temperature setpoints in the MOLEKIT 2 & 3 setup

Molekit 2 QCMserial numbers

Molekit 2 QCMtemperature setpoints

Molekit 3 QCMserial numbers

Molekit 3 QCMtemperature setpoints

QCM1: Mark17 S/N 1096 -113oC (160 K) QCM5: Mark17 S/N 2697 -113oC (160 K)QCM2: Mark17 S/N 2697 -60oC (213 K) QCM6: Mark17 S/N 2397 -60oC (213 K)QCM3: Mark17 S/N 2297 -183oC (90K) QCM7: Mark17 S/N 2297 -183oC (90K)QCM4: Mark16 S/N 0691 -20oC (253K) QCM8: Mark17 S/N 1096 -20oC (253K)

The molecular deposition onto all the QCMs, including the coldest QCM should be mixture of speciesdependent on their activation energies and perhaps influenced by the actual sample construction. A typical testdeposition phase can vary from 24 hours to several days. The sample is then removed from the test setup, pulledback into the interlock chamber and the isolation valve is closed again, sample removed and a post test massmeasurement is performed. The QCMs are maintained at their temperature setpoint for a period of several hoursto monitor what sort of reemission occurs after the sample is removed from the test chamber. Typically there islittle to no remission of the deposited mass while maintained at the constant temperatures.

Then the QCMs are warmed up at a specified ramp rate. This QCM Thermogravimetric Analysis(QTGA) can be performed any variety of ways. The ASTM E1559 procedure recommends a ramp rate of1oC/min for the coldest QCM from the set points up to a “bakeout” temperature of 80oC (353K). The GSFCsetup was programmed to perform the QTGA on all the QCMs at ramp rates of 1oC/min. However, mainly forthis investigation, a ramp rate of 0.2 C/min was selected. Typically the GSFC QTGA goes up to 110oC (383K),where the QCMs bakeout for period of time to remove any (tough) molecules. The QTGA setup can beprogrammed to “march” the QCMs up in temperature together, where QCM3 (set to –183oC) will initially beginwarm-up and then at –113oC, QCM1 would also begin warm-up, and so on. The QCMs can also be programmedto warm-up all at once from their temperature setpoints, therefore QCM4, set at –20oC originally, will reach110oC the quickest and remain in bakeout mode awaiting the attainment of the other QCMs to 110oC (383K).

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Either method of warm-up is okay because the QCMs do not see each other and thus do not contribute/transferdeposition to any other QCM. QTGA for all these samples was performed under the “marching up together”method. Equations for computing the insitu outgassing rates, TMLs, VCMs, and evaporation rates are discussedin the ASTM E1559 procedure (ref. 1). Hundreds of tested samples for outgassing characteristics from variousfacilities across the US, including GSFC’s, are available through the NASA SEE program (ref. 2).

This slower method of QTGA takes ~21 hours to complete the warm-up to 110oC versus the standardQTGA method of 1oC/min, which takes less than 5 hours. This slower method was originally requested tosimulate a potential on-orbit warm-up of a critical optical sensor, like a Charged Couple Device. CCDs mayhave a heater mounted on the retaining structural support and through passive means may be heated up in a slowmanner. This investigation was also interested in addressing how warm does the QCM (or a pseudo CCDsurface) have to get to remove molecular buildup from water/ice of various film thicknesses from its surface.Table 2 lists the samples considered for this investigation, which also includes the QTGA ramp rate.

Table 2Samples considered for this investigation

Sample material Exposedtemperature

(oC)

Effectivesample size

(cm2) and pre-test mass (g)

SampleOutgassing

duration(hrs)

QCM3decayn-term

QCM3buildup

(Hz)

QCM3buildup

(Angstroms)

QTGA ramprate

(oC/min)

Carbon PhenolicRocket Nozzle

80 22.84 cm2

9.417 g55.2 0.513 77905 15269 0.2

Carbon PhenolicRocket Nozzle

50 21cm2

8.218 g78.7 0.535 39462 7735 0.2

Carbon PhenolicRocket Nozzle

30 21.92 cm2

8.657 g52.2 0.49 20253 3970 0.2

JWST ISIM composite 50 105.75 cm2

8.689 g56 0.708 8743 1714 0.2

JWST ISIM compositew/Micro cracks

40 105.75 cm2

8.645 g146 0.605 9487 1859 0.2

JWST ISIM composite -20 105.75 cm2

8.689 g265 0.5 2661 522 0.2

Swift AlumHoneycomb CarbonComposite

80 63.5 cm2

4.283 g72.8 0.971 3970 778 1.0

Swift AlumHoneycomb CarbonComposite

50 62.4 cm2

4.684 g77.4 0.768 2741 537 1.0

Swift AlumHoneycomb CarbonComposite

30 62.4 cm2

4.933 g96.6 0.71 2240 439 1.0

3M 1205 acrylicadhesive tape

80 42.41cm2

0.562 g50 1.02 2168 425 0.2

EC 2216 gray epoxy 80 5.82 cm2

1.795 g76.4 0.66 3695 724 0.2

EC 2216 gray epoxy 50 4.92 cm2

1.714 g73.3 0.678 2104 412 0.2

EC 2216 gray epoxy 30 5.22 cm2

1.689 g78.5 0.62 1232 241 0.2

Eccobond 285 w/catalyst 9 (100:3.5)black epoxy

102 11.64 cm2

6.603 g76 0.616 1571 308 0.2

Eccobond 285 w/catalyst 9 (100:3.5)black epoxy

80 11.64 cm2

6.857 g75.3 0.696 805 158 0.2

Z306 w/9924 primeron Al foil

80 31.3 cm2

0.103 g44 0.91 861 169 1.0

Z306 w/9924 primeron Al foil

50 71.1 cm2

0.286 g27.4 0.95 1465 287 1.0

Z306 w/9924 primeron Al foil

30 142.5 cm2

0.537 g71 1.06 1938 380 1.0

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The samples had a variety of exposure temperature and lengths of exposures which characterized theoutgassing effects. The effective surface area of the samples were premeasured as well as the pre-test masswithout the substrate. The outgassing decay term (1/tn) was determined by taking a power curvefit of the samplelog OGR versus the log of exposure time (hrs). Some of the samples exhibited diffusion-limited outgassingcharacteristics, but one in particular, the JWST composite sample (w/Microcracks) at 40oC, was noticeablydropping off in outgassing after 100 hours of exposure. The molecular accretion onto QCM3 was also includedand a simple film thickness conversion to Angstroms was included by assuming the average molecular density of1.0 g/cm3. The QTGA ramp rate is also noted for each sample. Most similar samples had similar QTGA ramprates.

RESULTS

A simple way of showing the results from all the samples is have them plotted onto a single graph thatessentially plots the change in the QCM frequency (Hz) versus QCM temperature (oC). The change in QCMfrequency is the subtraction of the sample tested QCM frequency at a temperature minus the baseline QCMfrequency at the same temperature. This is also explained the ASTM E1559 procedure (ref.1). Figure 2demonstrates the effectiveness of the QTGA evaporation for each sample considered. The QCM frequency wasnot normalized to demonstrate that there is still some non-water molecular mass on the crystal during QTGA upto –80oC and beyond. One can then take Figure 2 one step further and calculate the percentage (%) left on thecrystal at each temperature of the QTGA process by normalizing the accumulated mass and multiplying by 100.

1

10

100

1000

10000

100000

-140 -136 -132 -128 -124 -120 -116 -112 -108 -104 -100 -96 -92 -88 -84 -80QCM Temperature, Degrees Celsius

QC

M D

elta

Fre

qu

ency

fro

m B

asel

ine,

Her

tz

Eccobond 285 w/Cat9 @80C

Swift Carbon Comp @80C

3M 1205 @ 80C

Eccobond 285 w/Cat9 @102C

EC2216 @80C

Carbon Phenolic RN @30C

Carbon Phenolic RN @80C

Carbon Phenolic RN @50C

JWST ISIM Carbon Comp @50C

JWST ISIM Carbon Comp @-20C

Swift Carbon Comp @50C

Swift Carbon Comp @30C

JWST ISIM Microcrack@40C

Z306 @80C

Z306 @50C

Z306 @30C

Figure 2QCM Mass remaining in terms of Frequency during QTGA

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Two quick inferences can be drawn from Figure 2 and from referencing the samples listed in Table 2.

1. The higher the molecular deposition levels on the QCMs tended to increase the QCM temperature requiredto remove the condensed water vapor. However, even thousands of Angstroms of ice/water mass can beremoved by –100oC if the reemission rate is slow enough.

2. Samples with a higher percentage of non-water concentrations demonstrated that an even warmer QCMtemperature (>–100oC) is needed to remove the water from the surface. The reemission of the 3M 1205acrylic tape residue on the QCM required a temperature of –91oC to be reached before the majority of watervapor was removed.

As mentioned the outgassing from these samples occurred over a period of days. Water and gases areknown to outgas fairly quickly under vacuum. Therefore the bulk diffusion outgassing process took place afterthe initial surface desorption phase and thus formed mixed monolayers onto the QCM crystal over the top ofwater monolayers. The percentage of water that was deposited onto the QCMs was computed by a simplecomparison of the respective sample’s molecular deposition, in terms of Hertz, gained on QCM3, set to –183oC,versus the gain on QCM1, typically set to –113oC.

Table 3Water percentage from samples

Sample materialExposed

temperature(oC)

QCMbuildup

(Hz)

QCMbuildup

(Angstroms)

QCMdecayn-term

Waterevaporated

by oC

Estimated % ofwater from

sample

QTGA ramprate

(oC/min)Carbon PhenolicRocket Nozzle

80 77905 15269 0.513 -102 99.8 0.2

Carbon PhenolicRocket Nozzle

50 39462 7735 0.535 -104 99.91 0.2

Carbon PhenolicRocket Nozzle

30 20253 3970 0.49 -108 99.88 0.2

JWST ISIM composite 50 8743 1714 0.708 -111 99.4 0.2JWST ISIM compositew/Micro cracks

40 9487 1859 0.605 -110 99.92 0.2

JWST ISIM composite -20 2661 522 0.5 -107 99.7 0.2Swift AlumHoneycomb CarbonComposite

80 3970 778 0.971 -106 96.7 1.0

Swift AlumHoneycomb CarbonComposite

50 2741 537 0.768 -108 98.6 1.0

Swift AlumHoneycomb CarbonComposite

30 2240 439 0.71 -109 99.2 1.0

3M 1205 acrylicadhesive tape

80 2168 425 1.02 -91 65 0.2

EC 2216 gray epoxy 80 3695 724 0.66 -115 98.8 0.2EC 2216 gray epoxy 50 2104 412 0.678 -115 99.32 0.2EC 2216 gray epoxy 30 1232 241 0.62 -117 99.45 0.2Eccobond 285 w/catalyst 9 (100:3.5)black epoxy

102 1571 308 0.616 -116 99.3 0.2

Eccobond 285 w/catalyst 9 (100:3.5)black epoxy

80 805 158 0.696 -119 99.75 0.2

Z306 w/9924 primeron Al foil

80 861 169 0.91 -96 34 1.0

Z306 w/9924 primeron Al foil

50 1465 287 0.95 -90 63 1.0

Z306 w/9924 primeron Al foil

30 1938 380 1.06 -85 78 1.0

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Table 3 indicates that the majority of molecular outgassing from the samples was predominately watervapor. Only the tape and the Z306 paint samples yielded sub 95% water concentrations. Muscari (ref. 3) andGlassford & Garrett (ref. 4) presented RGA and outgassing data that indicated similar findings for similarmaterials. There were ~20 samples of aerospace materials tested from each reference. If the sourcetemperatures are not warm enough to drive out bulk contaminants, water was the primary source especially atlow exposure temperatures. Z306 and acrylic tapes, have significant light weight molecules that outgas andcondense at temperatures warmer than -113oC and create a mixture of outgassed monolayers over the initiallyoutgassed water monolayers.

Table 3 doesn’t appear to show a strong relation to QTGA ramp rate and water evaporation temperature(Column 6), but one would think if the ramp rate was too high, like 5oC/min there may be a noticeable lag inwater vapor desorption. This work was done years ago by the QCM manufacturers whom computed the mostlogical ramp rate for a steady state QTGA. A slow ramp rate does allow the entrained water to “bubble” to thesurface of the QCM and reemit. The outgassing decay term also shows some relation to the exposed sampletemperature. The higher the source exposure temperature, the outgassing decay term is typically higher. Thisseems to hold true for composite samples (i.e. carbon phenolic rocket nozzle, the JWST ISIM compositesamples, and the Swift Honeycomb samples), but not for epoxies and the Z306 paint.

An MSX-funded paper investigated a similar QTGA effect (ref. 5). Their miscible species includedmethanol and toluene mixed with water. The water/ice still evaporated by –100oC for both mixtures. Themixtures did show that the complete evaporation of water vapor lagged in desorbing from the QCM crystal thanhomogeneous layered depositions. Another interesting finding from that paper was the concept of a delayedevaporation due to pressure. The higher the pressure the higher the QCM temperature had to get to remove thewater/ice buildup. However, a couple orders of magnitude increase in pressure only shifted the QCMtemperature upwards a few degrees for water removal. An increase to 1E-1 Torr only required an increase of~20oC, up to ~-80oC, for complete water vapor removal from the QCM crystal.

Another way to review the evaporation or desorption of the water is to compare evaporation rates andevaporation curves. Figure 3 (next page) demonstrates a similar linear trend towards water evaporation from thecrystal. This is characteristic of the kinetic constant of water evaporation. Several samples exhibit a minorbump in this linear trend, around –125oC (153K), where the phase change of ice to water (vapor) may beoccurring. Water or then vapor is still continuing to be removed from the crystal until the majority of the gainedwater mass has been removed from the crystal. The sharp downward trends, on the right sides of the plots, areindicative that the majority of the water vapor has been depleted from the crystal, thereby leaving a smallerpercentage of a variety of species. The softer bell-curve evaporative curves are more indicative of waterevaporating from a mixed concentration, where the water evaporating has to move through monolayers ofwater/non-water mixtures. This water removal through a mixed monolayer takes a little longer based on themonolayer(s) buildup. The actual removal of the water (and vapor) from the critical volume is not addressedhere but is typically a function of the vent paths from the volume, pressure between volumes, and surroundingsurface temperatures.

SUMMARY

Water evaporation from a surface is dependent on the amount of molecular buildup, in terms ofAngstroms or monolayers, and on whether the water must reemit through a miscible or mixed concentration.The results support the rationale that the thicker the miscible or mixed concentration, the slower the evaporativeprocess of the water.

REFERENCES

1. ASTM E1559-00, Standard Test Method for Contamination Outgassing Characteristics of SpacecraftMaterials, published by ASTM, maintained by ASTM Subcommittee E21.05, January 2001.

2. NASA Space Environments & Effects (SEE) Program, website http://see.msfc.nasa.gov/

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3. J. Muscari, “Non-metallic Materials Contamination Studies Final Technical Report,” MCR-80-637, MartinMarietta Corp., 16 December 1980.

4. A.P.M. Glassford & J. Garrett, “Characterization of Contamination Generation Characteristics of SatelliteMaterials,” WRDC-TR-89-4114, Lockheed Missiles & Space Company, Inc., 22 November 1989.

5. B. Bargeron, T.E. Phillips, and R.C. Benson, “Thermogravimetric Analysis of Selected CondensedMaterials on a Quartz Crystal Microbalance,” Proc. SPIE, Vol. 2261, 1984, pp. 188-199.

0.1

1

10

100

1000

10000

-140 -136 -132 -128 -124 -120 -116 -112 -108 -104 -100 -96 -92 -88 -84 -80

QCM Temperature, Degrees Celsius

QC

M F

req

uen

cy R

ate,

Her

tz/H

ou

r

Eccobond 285 @80C

Carbon Phenolic RN @50C

Swift comp @50C

Swift Comp @30C

3M 1205 @80C

Eccobond 285 @102C

EC 2216@80C

Carbon Phenolic RN @30C

Carbon Phenolic RN @80C

JWST ISIM Comp @50C

Swift comp @80C

JWST ISIM Comp @-20C

JWST ISIM Microcrack@40C

Z306 @80C

Z306 @50C

Z306 @30C

Figure 3QCM Reemission Rates

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November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

1

QCM Thermo-gravimetric Analysis (QTGA) Comparisons

AuthorsGlenn Rosecrans, Sr. Contamination EngineerGeorge Meadows, Sr. Contamination Engineer

Both of Swales Aerospace, Beltsville, MD USA(301)595-5500, www.swales.com

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November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

2

QTGA purposes• A QCM can mimic a critical optical surface and through a controlled

increase in temperature provide reemission characteristics of condensed molecular mass.

• QTGA data has been produced from various aerospace laboratories and from flight experiments for over 30 years providing various wealth of published documentation.

• Molecular outgassing is function of pressure and temperature. Critical molecular deposition is a function of receiver temperature with respect to source temperature. At pressures below 1E-6 Torr and temperatures below 150K (-123C) water condenses. These condensed water/ice molecules are mixed with most other outgassed species to form miscible condensed monolayers.

• Pure species, like water, have distinctive desorption characteristics.• How do the reemission traits of water change when a compilation of

molecular species from various typical aerospace products are present?

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November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

3

Various GSFC tested samples Sample material

Exposed

temperature (oC)

Effective sample size

(cm2) and pre-test mass (g)

Sample Outgassing

duration (hrs)

QCM3 decay n-term

QCM3 buildup

(Hz)

QCM3 buildup

(Angstroms)

QTGA ramp rate

(oC/min)

Carbon Phenolic Rocket Nozzle

80 22.84 cm2 9.417 g

55.2 0.513 77905 15269 0.2

Carbon Phenolic Rocket Nozzle

50

21cm2 8.218 g

78.7 0.535 39462 7735 0.2

Carbon Phenolic Rocket Nozzle

30 21.92 cm2 8.657 g

52.2 0.49 20253 3970 0.2

JWST ISIM composite 50 105.75 cm2 8.689 g

56 0.708 8743 1714 0.2

JWST ISIM composite w/Micro cracks

40 105.75 cm2 8.645 g

146 0.605 9487 1859 0.2

JWST ISIM composite -20 105.75 cm2 8.689 g

265 0.5 2661 522 0.2

Swift Alum Honeycomb Carbon Composite

80 63.5 cm2 4.283 g

72.8 0.971 3970 778 1.0

Swift Alum Honeycomb Carbon Composite

50 62.4 cm2 4.684 g

77.4 0.768 2741 537 1.0

Swift Alum Honeycomb Carbon Composite

30 62.4 cm2 4.933 g

96.6 0.71 2240 439 1.0

3M 1205 acrylic adhesive tape

80 42.41cm2 0.562 g

50 1.02 2168 425 0.2

EC 2216 gray epoxy 80 5.82 cm2 1.795 g

76.4 0.66 3695 724 0.2

EC 2216 gray epoxy 50 4.92 cm2 1.714 g

73.3 0.678 2104 412 0.2

EC 2216 gray epoxy 30 5.22 cm2 1.689 g

78.5 0.62 1232 241 0.2

Eccobond 285 w/ catalyst 9 (100:3.5) black epoxy

102 11.64 cm2 6.603 g

76 0.616 1571 308 0.2

Eccobond 285 w/ catalyst 9 (100:3.5) black epoxy

80 11.64 cm2 6.857 g

75.3 0.696 805 158 0.2

Z306 w/9924 primer on Al foil

80 31.3 cm2 0.103 g

44 0.91 861 169 1.0

Z306 w/9924 primer on Al foil

50 71.1 cm2 0.286 g

27.4 0.95 1465 287 1.0

Z306 w/9924 primer on Al foil

30 142.5 cm2 0.537 g

71 1.06 1938 380 1.0

Page 12: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

4

GSFC’s ASTM E-1559 apparatus

Typical Molekit 2 & 3 configuration

LN2 ShroudsAnd QCM shield

Page 13: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

5

QCM settingsMolekit 2 QCM serial numbers

Molekit 2 QCM temperature setpoints

Molekit 3 QCM serial numbers

Molekit 3 QCM temperature setpoints

QCM1: Mark17 S/N 1096 -113oC (160 K) QCM5: Mark17 S/N 2697 -113oC (160 K)

QCM2: Mark17 S/N 2697 -60oC (213 K) QCM6: Mark17 S/N 2397 -60oC (213 K)

QCM3: Mark17 S/N 2297QCM3: Mark17 S/N 2297 --183183ooC (90K)C (90K) QCM7: Mark17 S/N 2297QCM7: Mark17 S/N 2297 --183183ooC (90K)C (90K)

QCM4: Mark16 S/N 0691 -20oC (253K) QCM8: Mark17 S/N 1096 -20oC (253K)

GSFC’s ASTM E1559 setup uses 4 QCMs to gain a variety of partialcondensations and reemission data.Note the same cold QCM has been used for both setups (at different times) for material testing

Page 14: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

6

Typical QCM deposition phaseJWST ISIM composite sample at 50C

QCM2 at -60C curvefit

3345

3350

3355

3360

3365

3370

3375

0 10 20 30 40 50 60

time (hrs)

QC

M fr

eque

ncy

(Hz)

raw

curvefit

JWST ISIM composite sample at 50CQCM3 at -183C raw deposition data onto QCM

2000

3000

4000

5000

6000

7000

8000

9000

10000

11000

12000

0 10 20 30 40 50 60

time (hrs)

QC

M fr

eque

ncy

(gai

n in

Hz

abov

e ba

selin

e )

raw

JWST ISIM composite sample at 50CQCM4 at -20C curvefit

3505

3510

3515

3520

3525

3530

0 10 20 30 40 50 60

time (hrs)

QC

M fr

eque

ncy

(Hz)

rawcurvefit

Raw and curvefit deposition phases

JWST ISIM composite sample at 50CQCM1 at -113C curvefitting raw data

2870

2875

2880

2885

2890

2895

2900

2905

2910

0 10 20 30 40 50 60

time (hrs)

QC

M fr

eque

ncy

(Hz)

raw

curvefit

Page 15: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

7

Deposition equations( ) ( )[ ]

[ ]( ) [ ]( )( )

⎟⎠⎞

⎜⎝⎛××⎟

⎠⎞

⎜⎝⎛⋅×

−=⎟

⎠⎞

⎜⎝⎛ −

s3600hr1

)cm(SAcmFF

Hzcmg1096.1

hrstimehrstime

HzHz

scmgOGR 2

2

29

1t2t

1t2t2

freqfreq where: freq = QCM frequency at time 2 compared with frequency at time 1 time = time in hours of frequency data QCMms = QCM mass sensitivity of a QCM Research 15 MHz QCM= 1.96E-9 g/cm2/Hz FF = form factor of EC orifice to QCMs (Molekit2 FF = 635 cm2) SA = source surface area (in EC, varies, units in cm2) *******************************************************************

( ) ( ) ( )[ ] ( ) ( )100)g(SM

cmFFHzcm

g1096.1HzHz%TMLorVCM2

29

0t2t freqfreq ××⎟⎠⎞

⎜⎝⎛⋅×−= −

where: freq = QCM frequency at time 2 compared with initial frequency at time 0 QCMms = QCM mass sensitivity of a QCM Research 15 MHz QCM= 1.96E-9 g/cm2/Hz FF = form factor of EC orifice to QCMs (Molekit2 FF = 635 cm2) SM = source surface mass (preweighed in EC, varies, units in g) ******************************************************************** Curvefitting QCM raw data can be expressed with use of the following expression[1]:

( )[ ] ⎥⎦

⎤⎢⎣

⎡−×⎟

⎠⎞

⎜⎝⎛+= b

0t2t0tcf)timetime(

baHzfreqfreq

where: freq = QCM frequency at time 0; curvefit frequency dependent on a and b time = incremental time steps (hours) from time 0

b

( ) ( )( ) ( )

( ) ( )( ) ( )⎥

⎢⎢

⎡ −

⎥⎥

⎢⎢

⎡ −

=

hrhrhr

LOG

Hz

HzHzLOG

timehrtimetimetime

freqHzfreqfreqfreq

1t

2t

0t

0t2t

0t

0t2t

a ( ) ( )[ ]( ) ( ) b

0t1t

0t1t)hrhr

b*HzHz

timetime(freqfreq

−−

= Ref. [1] documented by M. Woronowicz in “Obtaining Model Outgassing Rate Parameters from Molekit Frequency Data,” SAI-21030173/MSW-38, Swales Aerospace, 7 March 1999.

Page 16: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

8

Typical Outgassing plots#2 #3#1

Outgassing rate of JWST ISIM carbon composite at 50C

1.0E-13

1.0E-12

1.0E-11

1.0E-10

1.0E-09

1.0E-08

0 10 20 30 40 50 60

exposure time (hrs)

outg

assi

ng ra

te (g

/cm

^2/s

ec)

wrt -113C

wrt -60C

wrt -183C

wrt -20C

Outgassing Rate decay of JWST ISIM carbon composite at 50C

y(-183C) = 3.391E-09x-7.081E-01

y(-60C) = 8.334E-12x-7.823E-01

y(-20C) = 5.682E-12x-8.236E-01

y(-113C) = 9.846E-12x-8.130E-01

1.0E-13

1.0E-12

1.0E-11

1.0E-10

1.0E-09

1.0E-08

1 10 100

exposure time (hrs)

outg

assi

ng ra

te (g

/cm

^2/s

ec)

wrt -113C

wrt -60C

wrt -183C

wrt -20C

Long term Outgassing of JWST ISIM Carbon Composite at 50C

1.0E-14

1.0E-13

1.0E-12

1.0E-11

1.0E-10

1.0E-09

1.0E-08

0 50 100 150 200 250 300 350 400 450 500

time (hrs)

Out

gass

ing

rate

(g/c

m^2

/sec

)

wrt -183C

wrt -113C

wrt -60C

wrt -20C

• Plot 1) Using the equations listed in the ASTM E1559 one can convert the raw or curvefit QCM data into an Outgassing Rate (g/cm2/sec) versus time

• Plot 2) One can then take the OGR plot and then plot it LOG (OGR) vs. LOG (time) to the determine the powerfit decay and gain the n-term (1/tn).

• Plot 3)One can then take the decay term and conservatively estimate the long term OGR (i.e. diffusion limited processes are ignored)

Page 17: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

9

Various Sample TML and VCM PlotsTML and VCM from 3M-1205 adhesive outgassing at 80C

0.00

0.05

0.10

0.15

0.20

0.25

0.30

0.35

0.40

0.45

0.50

0 5 10 15 20 25 30 35 40 45 50

time (hrs)

TML

and

VCM

(%)

TML at -183C

VCM at -113C

VCM at -60C

VCM at -20C

Insitu TML yielded 0.4804%,Exsitu TML was 0.8224%,for ~42% missed

VCM of JWST ISIM Carbon Composite from 50C exposure

0.0E+00

5.0E-05

1.0E-04

1.5E-04

2.0E-04

2.5E-04

3.0E-04

3.5E-04

4.0E-04

0 10 20 30 40 50 60

time (hrs)

VCM

(%)

0.00

0.02

0.04

0.06

0.08

0.10

0.12

0.14

0.16

TML

(%)

wrt -113Cwrt -60Cwrt -20CTML(>)

Insitu TML yielded 0.1254%,Exsitu TML yielded 0.1294%,for <3% difference

VCM trend of EC 2216 (gray) at 80C

0

5

10

15

20

0 10 20 30 40 50 60 70 80

time (hrs)

VCM

(mic

rogr

ams/

cm^2

)

cf wrt -113C

cf wrt -60C

cf wrt -20C

Insitu TML was 0.256% after 76 hrsExsitu was 0.26%, ~98.5% collectedVCM at -113C was 0.75% of TMLVCM at -60C was 0.36% of TMLVCM at -20C was 0.21% of TML

TML and VCM of Z306 + 9924 primer @50C

0.0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0 4 8 12 16 20 24 28

Time (hours)

TML

& V

CM

(%)

Insitu TML

VCM @-113C

VCM @-60C

VCM @-20C

Insitu TML yielded 0.611%,Exsitu TML yielded 1.15%,or ~ 47% missed

Page 18: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

10

Evaporative processes (QTGA)• The preprogramming of QTGA-like processes has been incorporated in many

optical cavities and thermal systems– Tradeoff….Mechanical Design $ vs. Increased Science Data.

• Though the optical warmups typically suspend data collection, most systems rebound with optimal throughput. Subsequent diffusion processes continue to provide molecular mass over years to still condensed mass on various, thus necessitating additional warmups.

– Condensed Water is of main concern for IR sensors– Hydrocarbons, silicones are of main concern for UV optics.– Lack of QTGA capability, Synergistic effects, and lack of product

removal from the cavity (venting) may never correct molecular induced degradation (i.e. Chandra optics BO)

• The ASTM E-1559 process does provide a best case scenario for reviewing QTGA processes.– Preprogrammed Rates for all QCMs at 1.0C/min or 0.2C/min up to 110C– Reemitted mass condenses on cold walls/shields and doesn’t return to any

of the QCMs– Can load up realistic quantities of a molecular film within a relatively

short period with possibly a cornucopia of materials

Page 19: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

11

QTGA equations( ) ( )[ ]( ) ( )[ ] ( ) ⎟⎟

⎞⎜⎜⎝

⎛⎟⎠⎞

⎜⎝⎛×−⎟

⎠⎞

⎜⎝⎛⋅×⎟

⎜⎜

−=⎟

⎠⎞

⎜⎝⎛ −

s3600hr1)hrs(1t)hrs(2t/

Hzcmg1096.1

HzHz

HzHz

scmgEvapRate 2

9

1t2t

1t2t2 bfreqbfreq

freqfreq where the evaporation rate is a function of the change in sample and baseline frequencies with respect to QCM temperature: freq = QCM frequency from sample data at temp2 compared with frequency at temp1 bfreq = QCM frequency from baseline data at temp2 compared with frequency at temp1t1, t2 = timesteps of QTGA process in hours QCMms = QCM mass sensitivity of a QCM Research 15 MHz QCM= 1.96E-9 g/cm2/Hz * Evaporation rate can be expressed in terms of g/cm2 as well (remove time from equation) * Evaporation rate can be expressed in terms of g as well (remove time and multiply by area of QCM crystal area of ~0.32 cm2) and perhaps multiply by 1000 to get in terms of milligrams (mg). *********************************************************************** *To gain the percent mass lost (%) from the QCM during the QTGA process use the following expression, which compares the delta frequency in sample and baseline at each temp/time step to the (maximum) delta frequency that should occur at time zero.

( ) ( ) ( )[ ] ( ) ( )[ ]( ) ( )100HzHz/HzHz%mainingRePercent bfreqfreqbfreqfreq 0t0t1t1t×−−=

************************************************************************* To just look at the change in frequency (Hz) during the QTGA just consider the difference between sample and baseline frequencies at each temp/time step, freqt1-bfreqt1. * To gain the evaporation rate of the mass in terms of Hz/hr, just consider the incremental change in sample to baseline frequencies per temperature/timestep (t2 to t1) considered.

( ) ( )[ ]( ) ( )[ ] ( )( ))hrs(1t)hrs(2t/

HzHz

HzHz

hrHzEvapRate

bfreqbfreqfreqfreq

1t2t

1t2t −⎟⎟

⎜⎜

−=⎟

⎠⎞

⎜⎝⎛

Page 20: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

12

QTGA via Molekit

M O L E K IT 3 T e s t, Z 3 0 6 w /P r im e r o n A l F o il @ 5 0 oC , Q C M D e lta R e e m is s io n s

-2 0

0

2 0

4 0

6 0

8 0

1 0 0

1 2 0

1 4 0

1 6 0

1 8 0

2 0 0

2 2 0

2 4 0

2 6 0

2 8 0

3 0 0

3 2 0

3 4 0

3 6 0

3 8 0

4 0 0

4 2 0

4 4 0

4 6 0

4 8 0

5 0 0

5 2 0

5 4 0

5 6 0

5 8 0

-9 5 -9 0 -8 5 -8 0 -7 5 -7 0 -6 5 -6 0 -5 5 -5 0 -4 5 -4 0 -3 5 -3 0 -2 5 -2 0 -1 5 -1 0 -5 0 5 1 0 1 5 2 0 2 5 3 0 3 5 4 0

Q C M T e m p e ra tu re , D e g re e s C e ls iu s

QC

M S

ampl

e an

d B

asel

ine

Ree

mis

sion

Fre

quen

cy, H

ertz

-2 0

0

2 0

4 0

6 0

8 0

1 0 0

1 2 0

1 4 0

1 6 0

1 8 0

2 0 0

2 2 0

2 4 0

2 6 0

2 8 0

3 0 0

3 2 0

3 4 0

3 6 0

3 8 0

4 0 0

4 2 0

4 4 0

4 6 0

4 8 0

5 0 0

5 2 0

5 4 0

5 6 0

5 8 0-9 5 -9 0 -8 5 -8 0 -7 5 -7 0 -6 5 -6 0 -5 5 -5 0 -4 5 -4 0 -3 5 -3 0 -2 5 -2 0 -1 5 -1 0 -5 0 5 1 0 1 5 2 0 2 5 3 0 3 5 4 0

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

Q C M 5 (-1 1 3 C )D e lta R e e m is s io n

Q C M 6 (-6 0 C ) D e lta R e e m is s io n

Q C M 7 (-1 8 3 C ) D e lta R e e m is s io n

Q C M 8 (-2 0 C ) D e lta R e e m is s io n

Q C M 7 h a d to lo s e 1 4 6 2 H z -5 6 0 H z o r ~ 9 0 0 H z o f w a te r v a p o r to g e t h e re

Non-water vapor QTGA, typically trend together on reemissions

M O L E K IT 2 T e s t , C a rb o n P h e n o lic R o c k e t N o z z le @ 8 0 o C , Q C M D e lta R e e m is s io n s

-1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0

6 5

7 0

7 5

8 0

8 5

9 0

-1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0Q C M T e m p e ra tu re , D e g re e s C e ls iu s

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

-1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0

6 5

7 0

7 5

8 0

8 5

9 0-1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

Q C M 1 ( -1 1 3 C )D e ltaR e e m is s io n

Q C M 2 (-6 0 C ) D e ltaR e e m is s io n

Q C M 3 ( -1 8 3 ) D e ltaR e e m is s io n

Q C M 4 ( -2 0 C ) D e ltaR e e m is s io n

Q C M 3 h a d o ff lo a d e d 7 7 8 0 0 H zo f w a te r v a p o r to g e t to th is p o in t

M O L E K IT 2 T e s t , J W S T IS IM C a r b o n C o m p o s ite 2 @ 5 0 o C , Q C M D e lta R e e m is s io n s

- 1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0

-1 2 0 -1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0Q C M T e m p e r a tu r e , D e g r e e s C e ls iu s

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

- 1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0-1 2 0 -1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

Q C M 1 ( -1 1 3 C ) D e ltaR e e m is s io n

Q C M 2 ( -6 0 C ) D e ltaR e e m is s io n

Q C M 3 ( -1 8 3 C ) D e ltaR e e m is s io n

Q C M 4 ( -2 0 C ) D e ltaR e e m is s io n

Q C M 3 a t - 1 8 3 C o r ig in a lly h a d 8 8 0 0 H z o f w a te r v a p o r to re m o v e b e fo re r e a c h in g th e s e le v e ls

M O L E K IT 2 T e s t, E C 2 2 1 6 , R T C u re @ 8 0 oC , Q C M D e lta R e e m is s io n s

-1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0

-1 2 0 -1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0Q C M T e m p e ra tu re , D e g re e s C e ls iu s

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

-1 0

-5

0

5

1 0

1 5

2 0

2 5

3 0

3 5

4 0

4 5

5 0

5 5

6 0-1 2 0 -1 1 0 -1 0 0 -9 0 -8 0 -7 0 -6 0 -5 0 -4 0 -3 0 -2 0 -1 0 0 1 0 2 0 3 0 4 0 5 0 6 0 7 0 8 0 9 0 1 0 0

QC

M D

elta

Ree

mis

sion

Fre

quen

cy, H

ertz

Q C M 1 (-1 1 3 C ) D e lta R e e m is s io n d a ta o m itte d

Q C M 2 (-6 0 C ) D e lta R e e m iss io n

Q C M 3 (-1 8 3 C )D e lta R e e m iss io n

Q C M 4 (-2 0 C ) D e lta R e e m iss io n

Q C M 3 h a d to lo s e ~ 3 7 0 0 H zo f w a te r v a p o r to g e t h e re

Page 21: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

13

QTGA (evaporation rates vs. temp)QCM Evaporation Rate of Z306 + 9924 primer from exposure at 50C

1.0E-13

1.0E-12

1.0E-11

1.0E-10

1.0E-09

1.0E-08

-200 -150 -100 -50 0 50 100 150

Temperature (deg C)

Evap

orat

ion

rate

(g/c

m^2

/sec

)

Evap from -183C

Evap from -113C

Evap from -60C

Q T G A fro m exp o su re to E C 2 216 @ 80C

1 .0E -13

1 .0E -12

1 .0E -11

1 .0E -10

1 .0E -09

1 .0E -08

1 .0E -07

-200 -1 50 -10 0 -5 0 0 50 1 00Q C M te m p era tu re (d eg C )

Evap

orat

ion

Rat

e (g

/cm

^2/s

ec)

fro m -18 3 C

fro m -11 3 C

fro m -60 C

fro m 0 C

Q TG A o f JW S T IS IM C om posite a t 50C exposure

1.0E -13

1.0E -12

1.0E -11

1.0E -10

1.0E -09

1.0E -08

1.0E -07

-200 -150 -100 -50 0 50 10 0

Q C M tem p erature (d eg C )

Evap

oriz

atio

n ra

te (g

/cm

^2/s

ec)

Q 3 from -183CQ 1 from -113CQ 2 from -60CQ 1 from -20C

Evaporation rate of 3M1205 from 80C exposure

1.0E-13

1.0E-12

1.0E-11

1.0E-10

1.0E-09

1.0E-08

-200 -175 -150 -125 -100 -75 -50 -25 0 25 50 75 100

QCM tem perature (deg C)

evap

orat

ion

rate

(g/c

m^2

/sec

)

from -183C

from -113C

from -60C

from -20C

Page 22: Page 1 of 8 - NASA

November 2004 – IEST Space Simulation Conference QCM Thermo-gravimetric Analysis (QTGA) Comparisons

14

QTGA Plot (Percent Remaining)P ercent M ass rem ain ing during Q TG A from exposure to JW S T IS IM co m posite a t 50C

0

10

20

30

40

50

60

70

80

90

100

-200 -150 -100 -50 0 50 100

Q C M tem perature (deg C )

Perc

ent r

emai

ning

(%)

0 .00

0 .05

0 .10

0 .15

0 .20

0 .25

0 .30

0 .35

0 .40

0 .45

0 .50

Perc

ent r

emai

ning

from

Q3(

%)

from -183Cfrom -60Cfrom -20Cfrom -112C

99.65% h igh ly vo la tile0 .2% m ed vo la tility0 .15% low vo la tility

QTGA of 3M_1205 tape from exposure at 80C

0

10

20

30

40

50

60

70

80

90

100

-200 -175 -150 -125 -100 -75 -50 -25 0 25 50 75 100

QCM tem perature (deg C)

Perc

ent r

emai

ning

(%)

from -183C

from -113C

from -60C

from -20C

P e rce n t M as s R e m ain in g fro m Q T G A o f E C 2 2 1 6 ex p o s u re a t 8 0C

0

1 0

2 0

3 0

4 0

5 0

6 0

7 0

8 0

9 0

1 0 0

-2 0 0 -1 5 0 -1 0 0 -5 0 0 50 1 0 0Q C M te m p e ratu re (d e g C )

Perc

ent M

ass

Rem

aini

ng (%

)

0 .0

0 .5

1 .0

1 .5

2 .0

2 .5

Perc

ent M

ass

Rem

aini

ng Q

4 (%

)

Q 3 from -1 83 C

Q 1 from -1 13 C

Q 2 from -6 0C

Q 4 from 0C

Q 3 from 90 K (> )

R eg io n 198 .5 %

R eg ion 30 .5%

R e g ion 50 .3%R eg io n 4

0 .7%

Percent m ass rem aining during QTGA from exposure to Z306 + 9924 prim er @ 50C

0

10

20

30

40

50

60

70

80

90

100

-200 -150 -100 -50 0 50 100 150

Tem perature (deg C)

Perc

ent m

ass

rem

aini

ng o

n Q

CM

(%)

0

5

10

15

20

25

30

35

40

45

50Pe

rcen

t mas

s re

mai

ning

on

QC

M (%

)

Q7 from -183C

Q5 from -113C

Q6 from -60C

Q7 from -90C(>)

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QTGA of Samples Considered

1

10

100

1000

10000

100000

-140 -136 -132 -128 -124 -120 -116 -112 -108 -104 -100 -96 -92 -88 -84 -80QCM Temperature, Degrees Celsius

QC

M D

elta

Fre

quen

cy fr

om B

asel

ine,

Her

tz

Eccobond 285 w/Cat9 @80CSwift Carbon Comp @80C3M 1205 @ 80CEccobond 285 w/Cat9 @102CEC2216 @80CCarbon Phenolic RN @30CCarbon Phenolic RN @80CCarbon Phenolic RN @50CJWST ISIM Carbon Comp @50CJWST ISIM Carbon Comp @-20CSwift Carbon Comp @50CSwift Carbon Comp @30CJWST ISIM Microcrack@40CZ306 @80CZ306 @50CZ306 @30C

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Water Evaporation temperaturesSample material Sample Temp DFreq (Hz) n-term Angstroms microns micrograms Evap Temp % water (degC/min)Eccobond 285 w/cat 9 80C 805 0.696 158 0.016 0.500 -119 99.75 0.2EC2216 gray epoxy 30C 1232 0.62 241 0.024 0.765 -118 99.45 0.2Eccobond 285 w/cat 9 102C 1571 0.616 308 0.031 0.975 -116.5 99.3 0.2EC2216 gray epoxy 80C 3695 0.659 724 0.072 2.294 -115 98.8 0.2EC2216 gray epoxy 50C 2104 0.678 412 0.041 1.306 -115 99.32 0.2JWST ISIM carbon composite 50C 8743 0.708 1714 0.171 5.427 -111 99.4 0.2JWST ISIM carbon comp w/MCs 40C 9487 0.605 1859 0.186 5.889 -110 99.92 0.2Swift Al HC carbon comp 30C 2240 0.71 439 0.044 1.390 -109 99.2 1Carbon Ph Rocket Nozzle 30C 20253 0.49 3970 0.397 12.572 -108 99.88 0.2Swift Al HC carbon comp 50C 2741 0.768 537 0.054 1.701 -108 98.6 1JWST ISIM carbon composite -20C 2661 0.5 522 0.052 1.652 -107 99.7 0.2Swift Al HC carbon comp 80C 3970 0.971 778 0.078 2.464 -106.7 96.7 1Carbon Ph Rocket Nozzle 50C 39462 0.535 7735 0.773 24.495 -104 99.91 0.2Carbon Ph Rocket Nozzle 80C 77905 0.513 15269 1.527 48.358 -102 99.8 0.2Carbon Ph Rocket Nozzle 50C 98082 0.71 19224 1.922 60.883 -101 99.91 0.2Z306 w/9924 on Al foil 80C 861 0.907 169 0.017 0.534 -96 34 13M 1205 (Acry. Adh.) 80C 2168 1.02 425 0.042 1.346 -91 65 0.2Z306 w/9924 on Al foil 50C 1465 0.95 287 0.029 0.909 -90 63 1Z306 w/9924 on Al foil 30C 1938 1.06 380 0.038 1.203 -85 77.8 1

Earlier table sorted by ascending (complete) evaporation temperature.faster reemission rate drags evap tempThicker water accretion drags evap temphigher n-term indicates less water, higher misc. VCM %

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QCM Reemissions Rates (samples)

0.1

1

10

100

1000

10000

-140 -136 -132 -128 -124 -120 -116 -112 -108 -104 -100 -96 -92 -88 -84 -80QCM Temperature, Degrees Celsius

QC

M F

requ

ency

Rat

e, H

ertz

/Hou

rEccobond 285 @80CCarbon Phenolic RN @50CSwift comp @50CSwift Comp @30C3M 1205 @80CEccobond 285 @102CEC 2216@80CCarbon Phenolic RN @30CCarbon Phenolic RN @80CJWST ISIM Comp @50CSwift comp @80CJWST ISIM Comp @-20CJWST ISIM Microcrack@40CZ306 @80CZ306 @50CZ306 @30C

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Arhenius plots from samples

Water evaporation rates are difficult to distinguish when multiple molecular species are mixed in the water monolayers.

-22

-20

-18

-16

-14

-12

-10

5.00 5.50 6.00 6.50 7.00 7.50

1000/QCM temperature (1000/deg K)

Evap

orat

ion

rate

(g/c

m^2

/sec

)* S

QR

T (T

in d

eg K

)

Z306 at 30CJWST ISIM at 40C3M 1205 at 80C

slope (S) yields latent heat *1000 * R (cal/mole)S1= ~15800 cal/mole (Z306)S2 = ~7200 cal/mole (Z306)S3 = ~11,950 cal/mole (JWST)S4 = ~23,000 cal/mole (3M 1205)

S1S2

S3

S4

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Summary

QTGA is a function of chemical composition deposited on a surface and the surface at which the source begins it’s evaporationWater evaporation is inhibited by the thickness of the molecular buildup, however the water evaporation can be a complete process at a fairly cold temperature (by -90C as long as venting is sufficient).Water molecules will work it’s way through more volatile layers of deposited mass but it’s complete reemission will be inhibited. Other non-volatile molecular residue only becomes “volatile” as the appropriate temperature is attained to activate the molecule(s) and may effect the evaporative processes of pure substances.An experimental QTGA process can be used to assist in programmatic decisions on warm-up capabilities and operational requirements.

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Paper References• ASTM E1559-00, Standard Test Method for Contamination Outgassing

Characteristics of Spacecraft Materials, published by ASTM, maintained by ASTM subcommittee E21.05, January 2001.

• NASA Space Environments & Effects (SEE) Program, website http://see.msfc.nasa.gov/

• “Non-metallic Materials Contamination Studies Final Technical report,” MCR-80-637, the late Joe Muscari, Martin Marietta Corp., 16 Dec 1980.

• “Characterization of Contamination Generation Characteristics of Satellite Materials,” WRDC-TR-4114, Peter Glassford and Jeff Garrett, Lockheed Missiles & Space Company, Inc., 22 November 1989.

• “Thermogravimetric Analysis of Selected Condensed Materials on A Quartz Crystal Microbalance,” B. Bargeron, T.E. Phillips, and R.C. Benson, Proc. SPIE, Vol. 2261, 1984, pp. 184-189.

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AcknowledgementsThe authors wish to thank numerous folks who have contributed to this effort either directly or indirectly. First this work was performed under a Swales MSES contract #NAS5-01090 through NASA/GSFC. The GSFC contamination lead is Randy Hedgeland whom approves of the subtasks to include materials testing. The Molekit facility has been in operation for over 10 years at GSFC, under the observation of the Thermal Branch, and has performed hundreds of outgassing tests. The GSFC Thermal branch heads over the years who have approved purchase orders for Molekit facility modifications and upkeep over the years include Wes Ousley, Dennis Hewitt, Roy McIntosh, and Norm Ackerman. Space-grade QCM supplier’s like Dan and Scott Wallace of QCM Research, and Dan McKeown of Faraday Laboratories, for providing the QCMs for the Molekit system over the years. The authors also would like to acknowledge the past work with the QCMs development for use as a useful real-time tool for measuring material outgassing. The past published works from Raymond Kruger, John Scialdone, and Jack Triolo (GSFC), Peter Glassford and Jeff Garrett (LMSC), Gene Zeiner (Hughes), Dave Hall (Aerospace Corp), Bob Wood (AEDC), Joseph Muscari (Martin Marietta), Carl Maag (JPL), and Manny Oy, et.al., (JHU/APL) still continue to influence the contamination engineering community today.