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422 424 426 428 155 160 165 170 175 180 185 190 195 200 205 210 Wavelength (nm) Intensity (arb. units) Bare Al LPS on Al JSC-1a on Al 392 394 396 398 400 0 200 400 600 800 1000 1200 1400 1600 Wavelength (nm) Counts 316 SS JSC−1a on SS Biofilm on SS 0 300 600 900 1200 1500 1800 0 1000 2000 3000 4000 5000 6000 7000 Fe emission at 392 nm Ca emission at 393.5 nm 316 SS Biofilm on SS JSC−1a on SS Laser Induced Breakdown Spectroscopy as an in-space sample return canister sterilization method and instrument Christopher B. Dreyer, John R. Spear, Kennda L. Lynch, Lenea Johnson, and Amy J. Bauer* Colorado School of Mines, Golden, CO 80401 and *Applied Research Associates, Littleton, CO 80127 Introduction We are investigating the use of focused laser beams to ablate the surface of spacecraſt surfaces and contaminating materials. e method can be applied such that the ablated material is heated to a plasma, making it a laser induced breakdown spectroscopy (LIBS) approach (Figure 1). Potential benefits include: • Sterilization in space or on a planetary surface. • Direct characterization of ablated material. • Complete vaporization of surface material. Proof of concept tests have been conducted to show the ability to remove surface contaminantes while simultaneously identify contaminates via LIBS. Materials studied to date are listed in Table 2. Laser irradiance was set at approx. 10 GW/cm2. e sample was translated horizontally, causing the focused beam to sweep out 6 mm in 45 seconds. Images of ablated contaminantes are shown in Figure 6, 7, and 8. LIBS can be used to identify the type of surface contaminant. A simple comparison of Fe emission near 392 nm to Ca emission near 393.5 nm (Figure 10) reveal that a biofilm ladened surface can be differentiated from the bare surface and a geological contaminant. Conceptual Design Proof of Concept Work Figure 4: Lipopolysaccharide layer on 6061 Aluminum, photo (top), SEM (bottom). Results: Ablation e 1064nm output of a pulsed Nd:Yag laser, 8 ns duration, at 4 Hz, was focused to an elliptical focus of approx. 80 μm width and 4 mm height. e beam was focused into a vacuum chamber containing a 3-axis sample translation stage (Figure 5). Plasma emission was delivered to Ocean Optics miniature spectrometers via optical fibers. Tests were at 7 to 9 torr in a CO2 atmosphere (SS) and air (aluminum). Figure 5: CSM LIBS vacuum chamber. Top: overview. Bottom left: chamber interior with sample holder and collection fibers. Bottom right: Ocean Optics spectrometers. Figure 6: Laser ablation cleaning of a biofilm from 316 SS. A 4x6 mm area of biofilm was removed, scanning left to right. Left, visible image. Right, SEM image of removed edge. Figure 7: Laser ablation of lipopolysaccharide (LPS) on 6061 Al. Results: Aluminum samples Results: LIBS Figure 8: JSC-1a, a lunar mare simulant composed of crushed basalt [5], on stainless steel (left side) before and after ablation, held on with spray adhesive. Right side, dusting of JSC-1a on 6061 aluminum after ablation. Spectra from 316 SS was dominated by Fe emisison, making identification of emission from other elements difficult. With 6061 aluminum the base metal is less dominate. Evenly distributed bio-layers and thin geological layers produce more consistent pulse-to-pulse spectra (Figure 11). Figure 10: Cluster analysis of LIBS data identifies the different samples. Conclusions Contaminantes can be removed from a surface via laser ablation with simultaneous identification of the ablated material via LIBS. Areas of future work are: • Test with a greater variety of substrates and microbes. • Determine microbe viability aſter full sterilization of a surface. • Examine microbe transport during ablation. • Test with a tightly focused and low pulse energy beam, which is more likely for a space flight application, and optimize analysis. • Tests of LIBS and ablation at very low pressure (more similar to an in-space application) which is known to dramatically decrease emission intensity [6][7]. Literature Cited [1] Perni, S. J. et al. (2011) J Biomater. Appl. 22, 5, 387-400. [2] G.S. Omar, et al., (2008) BMC Microbiology, 8:111. [3] Vorobyev, A.Y., et al. (2006) App. Phys. A, 82, 357. [4] Cremers, D.A. and L. Radziemski (2006) Handbook of Laser-induced Breakdown Spectroscopy, John Wiley and Sons. [5] McKay D. S. et al. (1994) "JSC-1: A new lunar soil simulant". Eng., Construction, and Operations in Space IV, ASCE, 857-866. [6] Effenberger A.J., Jr. (2010) Scott J.R. Sensors. 10(5):4907-4925. [7] Choi, S-J and Yoh, J.J, (2011) Optics Express, 19(23) 23097 For further information: Please contact [email protected], (303)273-3890 laser ablated unaltered biofilm Figure 3: Biofilm on 316 stainless steel, photo (top), SEM (bottom). Ca II } Fe } Fe A system using a 10 mJ/pulse laser, a ChemCam-like optical system, and scanning with a robotic arm, would use ~76W. Time for one sterilization pass of a sample return canister 9 cm diameter by 10 cm length (0.028 m2) is 37 min. Sterilization requires ~50 W-hr and 888,000 laser shots per pass. 589 590 591 592 600 800 1000 1200 1400 1600 1800 2000 Wavelength (nm) Intensity (arb. units) Bare Al LPS on Al JSC-1a on Al 334 336 338 340 200 210 220 230 240 250 260 270 Wavelength (nm) Intensity (arb. units) Bare Al LPS on Al JSC-1a on Al Ca I Ti I manifold Na I emission 0 50 100 150 200 250 0 100 200 300 400 500 Calcium Emission Titanium Emission Bare Al JSC-1a on Al LPS on Al 0 50 100 150 200 250 0 1000 2000 3000 4000 Calcium Emission Sodium Emission Bare Al JSC-1a on Al LPS on Al 0 50 100 150 200 250 30 40 50 60 70 80 90 100 Calcium Emission Aluminum Emission Bare Al JSC-1a on Al LPS on Al Figure 9: UV and portion of visible spectra from the plasma recorded by three Ocean Optics spectrometers. e LIBS spectrum contains hundreds of emission lines emanating from neutral and ionized species in the hot plasma. Figure 9 shows the spectra from 200 to 510 nm. Most are from Fe in the stainless steel and JSC-1a. 200 250 300 350 400 450 500 0 1000 2000 3000 Wavelength (nm) Counts 316 SS JSC−1a on SS Biofilm on SS Cluster analysis of aluminum samples using Ti, Ca, and Na emission shows that the three groups can be identified (Figure 12). More work is needed to eliminated collection misalignment, improve sample cleanliness, and spectrometer timing need to be optimized. Figure 12: Cluster analysis of LIBS spectra of contaminantes on 6061 Al. Figure 11: LIBS spectra from contaminantes on 6061 aluminum. 2 mm 2 mm 2 mm 4 mm 2 mm 2 mm Figure 2: Conceptual layout of a device for sterilizing an object. Figure 1: Ablation sequence in which a focused pulsed laser generates a plasma. The laser is scanned to remove a surface layer. The extent to which foreign material is transported away from the plasma is being investigated. Low irradiance lasers (~1 W/cm2) have been used to kill microbes [1][2]. Irradiance >10 MW/cm2 [3] will ablate most materials, and for LIBS ~10 GW/cm2 [4] is needed. Sub-ablation irradiance can weaken cell membranes causing loss of membrane integrity and produce oxidative species that destroy enzymes and DNA. In practice the concept may use a robotic arm to scan the laser (Figure 1). Emission from a plasma is collected by a spectrometer. e particular means of implementing the method will depend on the object and mission objectives. e laser irradiance has important implications for setting the laser power consumption, laser spot size, scanning rate, and time for sterilization. e time to fully treat a surface of area (A) is: Where a is the area treated by the laser per laser pulse and f is the laser repetition rate. To ensure complete sterilization several passes may be necessary. Table 1: Relationship between spot size and laser repetition rate at 10W laser (25% efficiency), 10 GW/cm2 irradiance 2 ns pulse, and sterilization area of 1m 2 . τ s = 22.2 hours per 1m 2 . Spot diameter (μm) Pulse Energy (mJ) Repetition Rate (Hz) 1000 157.1 15.9 500 39.3 63.7 100 1.57 1591.5 50 0.393 6366.2 250 9.8 398.9 l Sample Container Robotic Arm Miniature laser and spectrometer Reasonable for spaceflight Lipopolysaccharide Base Material Contaminant Form 316 SS biofilm growth, natural spring 316 SS JSC-1a <100 μm thick layer + adhesive 6061 Al JSC-1a <100 μm thin dusting 6061 Al thin even layer 4.5ng/ml 316 SS bare bare 6061 Al polished finish polished finish Table 2: Materials and contaminates proof of concept tests.
Transcript
Page 1: Laser Induced Breakdown Spectroscopy as an in-space ......5000 6000 7000 Fe emission at 392 nm Ca emission at 393.5 nm 316 SS Biofilm on SS JSC−1a on SS Laser Induced Breakdown Spectroscopy

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Laser Induced Breakdown Spectroscopy as an in-space sample return canister sterilization method and instrument

Christopher B. Dreyer, John R. Spear, Kennda L. Lynch, Lenea Johnson, and Amy J. Bauer*

Colorado School of Mines, Golden, CO 80401 and *Applied Research Associates, Littleton, CO 80127

IntroductionWe are investigating the use of focused laser beams to ablate the surface of spacecra� surfaces and contaminating materials. �e method can be applied such that the ablated material is heated to a plasma, making it a laser induced breakdown spectroscopy (LIBS) approach (Figure 1).

Potential bene�ts include: • Sterilization in space or on a planetary surface. • Direct characterization of ablated material. • Complete vaporization of surface material.

Proof of concept tests have been conducted to show theability to remove surface contaminantes while simultaneouslyidentify contaminates via LIBS. Materials studied to dateare listed in Table 2.

Laser irradiance was set at approx. 10 GW/cm2. �e sample was translated horizontally, causing the focused beam to sweep out 6 mm in 45 seconds. Images of ablated contaminantesare shown in Figure 6, 7, and 8.

LIBS can be used to identify the type of surface contaminant. A simple comparison of Fe emission near 392 nm to Ca emission near 393.5 nm (Figure 10) reveal that a bio�lm ladened surface can bedi�erentiated from the bare surface and a geological contaminant.

Conceptual Design

Proof of Concept Work

Figure 4: Lipopolysaccharide layer on 6061 Aluminum, photo (top), SEM (bottom).

Results: Ablation

�e 1064nm output of a pulsed Nd:Yag laser, 8 ns duration, at 4 Hz, was focused to an elliptical focus of approx. 80 μm width and 4 mm height. �e beam was focused into a vacuum chamber containing a 3-axis sample translation stage (Figure 5). Plasma emission was delivered to Ocean Optics miniature spectrometers via optical �bers. Tests were at 7 to 9 torr in a CO2 atmosphere (SS) and air (aluminum).

Figure 5: CSM LIBS vacuum chamber. Top: overview.Bottom left: chamber interior with sample holder and collection �bers. Bottom right: Ocean Optics spectrometers.

Figure 6: Laser ablation cleaning of a bio�lm from 316 SS. A 4x6 mm area of bio�lm was removed, scanning left to right. Left, visible image.Right, SEM image of removed edge.

Figure 7: Laser ablation of lipopolysaccharide (LPS) on 6061 Al.

Results: Aluminum samples

Results: LIBS

Figure 8: JSC-1a, a lunar mare simulant composed of crushed basalt [5], on stainless steel (left side) before and after ablation, held on with spray adhesive. Right side, dusting of JSC-1a on 6061 aluminum after ablation.

Spectra from 316 SS was dominated by Fe emisison, making identi�cation of emission from other elements di�cult. With 6061 aluminum the base metal is less dominate. Evenly distributed bio-layers and thin geological layers produce more consistent pulse-to-pulse spectra (Figure 11).

Figure 10: Cluster analysis of LIBS data identi�es the di�erent samples.

ConclusionsContaminantes can be removed from a surface via laser ablation with simultaneous identi�cation of the ablated material via LIBS. Areas of future work are: • Test with a greater variety of substrates and microbes. • Determine microbe viability after full sterilization of a surface. • Examine microbe transport during ablation. • Test with a tightly focused and low pulse energy beam, which is more likely for a space flight application, and optimize analysis. • Tests of LIBS and ablation at very low pressure (more similar to an in-space application) which is known to dramatically decrease emission intensity [6][7].

Literature Cited[1] Perni, S. J. et al. (2011) J Biomater. Appl. 22, 5, 387-400. [2] G.S. Omar, et al., (2008) BMC Microbiology, 8:111. [3] Vorobyev, A.Y., et al. (2006) App. Phys. A, 82, 357. [4] Cremers, D.A. and L. Radziemski (2006) Handbook of Laser-induced Breakdown Spectroscopy, John Wiley and Sons. [5] McKay D. S. et al. (1994) "JSC-1: A new lunar soil simulant". Eng., Construction, and Operations in Space IV, ASCE, 857-866. [6] Effenberger A.J., Jr. (2010) Scott J.R. Sensors. 10(5):4907-4925. [7] Choi, S-J and Yoh, J.J, (2011) Optics Express, 19(23) 23097

For further information: Please contact [email protected], (303)273-3890

laser ablated

unaltered bio�lm

Figure 3: Bio�lm on 316 stainless steel, photo (top), SEM (bottom).

Ca II

} Fe }Fe

A system using a 10 mJ/pulse laser, a ChemCam-like optical system, and scanning with a robotic arm, would use ~76W. Time for one sterilization pass of a sample return canister 9 cm diameter by 10 cm length (0.028 m2) is 37 min. Sterilization requires ~50 W-hr and 888,000 laser shots per pass.

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Figure 9: UV and portion of visible spectra from the plasma recorded bythree Ocean Optics spectrometers.

�e LIBS spectrum contains hundreds of emission lines emanatingfrom neutral and ionized species in the hot plasma. Figure 9 shows the spectra from 200 to 510 nm. Most are from Fe in the stainless steel and JSC-1a.

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316 SSJSC−1a on SSBiofilm on SS

Cluster analysis of aluminum samples using Ti, Ca, and Na emissionshows that the three groups can be identi�ed (Figure 12). More work is needed to eliminated collection misalignment, improve sample cleanliness, and spectrometer timing need to be optimized.

Figure 12: Cluster analysis of LIBS spectra of contaminantes on 6061 Al.

Figure 11: LIBS spectra from contaminantes on 6061 aluminum.

2 mm

2 mm2 mm 4 mm

2 mm

2 mm

Figure 2: Conceptual layout of a device for sterilizing an object.

Figure 1: Ablation sequence in which a focused pulsed laser generates a plasma. The laser is scanned to remove a surface layer. The extent to which foreign material is transported away from the plasma is being investigated.

Low irradiance lasers (~1 W/cm2) have been usedto kill microbes [1][2]. Irradiance >10 MW/cm2 [3] will ablate most materials, and for LIBS ~10 GW/cm2 [4] is needed. Sub-ablation irradiance can weaken cell membranes causing loss of membrane integrity and produce oxidative species that destroy enzymes and DNA.

In practice the concept may use a robotic arm to scan the laser (Figure 1). Emission from a plasma is collected by a spectrometer. �e particular means of implementing the method will depend on the object and mission objectives.

�e laser irradiance has important implications for setting the laser power consumption, laser spot size, scanning rate,and time for sterilization.

�e time to fully treat a surface of area (A) is:Where a is the area treated by the laser per laser pulse and f is the laser repetition rate. To ensure complete sterilization several passes may be necessary.

Table 1: Relationship between spot size and laser repetition rate at 10W laser (25% e�ciency), 10 GW/cm2 irradiance

2 ns pulse, and sterilization area of 1m2. τs = 22.2 hours per 1m2.

Spot diameter (μm)

Pulse Energy (mJ)

Repetition Rate (Hz)

1000 157.1 15.9500 39.3 63.7

100 1.57 1591.550 0.393 6366.2

250 9.8 398.9

l

Sample ContainerRobotic Arm

Miniature laser and spectrometer

Reasonable for spaceflight

Lipopolysaccharide

Base Material Contaminant Form

316 SS bio�lm growth, natural spring316 SS JSC-1a <100 μm thick layer + adhesive

6061 Al JSC-1a <100 μm thin dusting6061 Al thin even layer 4.5ng/ml

316 SS bare

bare6061 Al

polished �nish

polished �nish

Table 2: Materials and contaminates proof of concept tests.

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