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Planetary Protection

Planetary protection is a hard constraint on a robot before it is a policy about a planet. It sets how long hardware is baked and at what temperature, which materials survive that bake, how much of assembly and test schedule is spent waiting on assays, and what a mobility or sampling system is allowed to touch. The difficulty is that the quantity the policy is written against, the probability that a released organism survives and proliferates on another body, cannot be measured on the hardware that matters: nobody can fly a spacecraft to Mars, wait a generation, and check whether it started an ecosystem. Every number downstream of that gap is either a specification a vehicle must meet or a bioburden accounted on a vehicle that flew, and the two must not be read the same way.

The requirement was a probability before it was a bake schedule

Section titled “The requirement was a probability before it was a bake schedule”

The forward-contamination requirement began as a probability budget, not a hardware spec. The Space Science Board’s 1964 to 1965 exobiology study adopted a sterilization goal for a Mars lander of no more than a 1 in 10,000 chance of carrying a single viable organism aboard, starting from an assumed pre-sterilization bioburden of 100 million organisms and a dry heat cycle of 135 C for 24 hours to bring it down [1]. COSPAR adopted the same 1e-4 figure in 1964, together with a 3e-5 limit on the probability of an unsterilized flyby or orbiter accidentally impacting the planet [2]. When two 1967 papers in Science argued that both organism release and organism survival on Mars were negligible and that the standards should be relaxed, Sagan, Levinthal and Lederberg replied that every probability in the chain was uncertain by two orders of magnitude or more, that the burden of proof sat with whoever wanted to relax the standard, and that a compound risk near 1e-2 is not zero when the stakes are the biological exploration of a planet [2].

The model behind that reply, m times Pg, where m is the expected number of organisms released and Pg the probability that one released organism survives and proliferates, was itself challenged on structural rather than numerical grounds in 1973 [3]. Harrison and North showed the formula depends on two independence assumptions, that separate organisms’ fates are independent given the number released and that one organism’s survival odds do not depend on how many were released, and argued both are false because a large release implies a hard landing, which implies an uncertain landing site, which changes any single organism’s chances, and their proposed replacement was a three-stage landing, biorelease and proliferation model in which the landing model is made detailed enough that the independence assumptions hold given its output [3]. That three-stage structure is the ancestor of the category and special-region system used today.

Sterilization as engineering practice predates the probability framework it later answered to. Viking’s terminal sterilization bake was 111.7 C for 30 hours as flown, timed from when the coldest point on the lander reached temperature, against contemporary NASA specifications that ranged 104 to 125 C [4][5]. The one Viking hardware failure the program history records from that era was unrelated to heat: the surface sampler arm snagged on the holder of a magnet cleaning brush during a pre-flight system demonstration, fixed with a minor hardware change and a mission rule against magnet cleaning until all biology samples were taken [4].

The bakeout specification moved by a factor of seventeen

Section titled “The bakeout specification moved by a factor of seventeen”

Dry heat microbial reduction is credited against time at temperature. These are requirements from the current specification, not measured survival curves:

CreditConditionExposure
4-log, exposed surface126 C85.98 h
4-log, encapsulated126 C429.91 h
6-log, encapsulated126 C1289.74 h
6-log, encapsulated155 C71.45 h

Source: [5].

The superseded specification allowed 5 hours at 125 C exposed and 25 hours at 125 C encapsulated, so encapsulated hardware must now survive more than seventeen times the thermal exposure once assumed [5]. The revision followed the isolation of heat-resistant bacteria from spacecraft assembly cleanrooms. Its governing input is an assumption rather than a measurement: the fraction of spores that are super-tolerant to heat is stated as unknown and assumed at 1 in 1000, and that assumed frequency is what caps the credit any dry heat process can be given [5]. The same revision removed the previously required vacuum of at least 1e-4 torr and the dry humidity control.

The trade a designer makes is bake duration against material temperature limit, and the 155 C option buys an eighteenfold reduction in duration for 29 C less margin on every material and part inside the bake [5]. MER’s own pre-launch estimate used the same 125 C class of bakeout for hardware that could tolerate it, choosing wipe or HEPA isolation for what could not [8]. Vapor hydrogen peroxide is the alternative where heat is not survivable, and it is also specified rather than measured: a D-value of 200 (mg/L)s at 0.5 to 1.1 mg/L peroxide for a 2 to 6 order of magnitude reduction, and a Ct value of at least 14000 (mg/L)s at 6 to 8.6 mg/L for an overkill process [5]. Material compatibility for it has been measured, more than 100 materials evaluated at JPL at a six-log condition repeated four times to cover rework and requalification, most showing little or no property change and some changing by more than 15 percent [5].

What was achieved on flight vehicles, and which requirement bound

Section titled “What was achieved on flight vehicles, and which requirement bound”
VehicleTotal bioburdenTotal limitDensityDensity limit
MSL flight system at launch278,000 spores500,00022 spores/m2300 spores/m2
MER-A landed hardware101,000 spores300,00074 spores/m2300 spores/m2
MER-B landed hardware209,000 spores300,00074 spores/m2300 spores/m2

Sources: MSL [5], MER [6]. Limits are Category IV-A requirements. Both vehicles were Category IV-A, with no life detection instrument and no access to a special region, so none of these allowances transfers to a mission that has either; a mission that does, such as a Europa lander, is scoped under the same category system to a different, far stricter set of numbers still being worked out at the concept stage [7].

Both MER vehicles came in at the same 74 spores/m2, about a quarter of the density allowance, while MER-B used 70 percent of its total-count allowance [6]. The binding constraint was total count, not density [6]. An earlier MER estimate, made months before launch, had already flagged total count rather than density as the number to watch [8]. MSL came in at about 7 percent of its allowed density [5].

None of these is a direct count, and the grade matters more here than the value. The MSL figure is an accounting total built from a Planetary Protection Equipment List, with assays at roughly 10 percent sampling at last access and analytic dry heat and entry heating credit taken for the rest [5]. The MER figures are three-sigma worst case estimates whose briefing states no assay method, no sample count and no laboratory, and they exclude bulk and mated bioburden inside the warm electronics box under an exemption, so they are not the total organisms landed [6]. Every number is culturable aerobic endospores only, which says nothing about anaerobes, fungi, unculturable organisms, or dead but chemically detectable material, which is what an organic detection requirement cares about [5][6].

The count is not the whole exposure. The MSL payload fairing interior was cleaned to a measured 4 spores/m2 against a 1000 spores/m2 requirement, but over more than 400 m2 of interior surface, so even a compliant fairing carries a large absolute count and recontamination after encapsulation is a real path [5]. Which reduction method was actually used is a separate question from which is specified: of 721 MER flight hardware line items, 48 percent went through dry heat microbial reduction and 35 percent were isopropyl alcohol wipe or rinse only [6]. That is counted by line item and explicitly not by surface area or bioburden allocation, so it says nothing about which hardware carried the burden [6].

Cleanliness and structural qualification share a schedule, not a chamber

Section titled “Cleanliness and structural qualification share a schedule, not a chamber”

Bioburden control competes for the same assembly, test and launch operations calendar as environmental qualification, and the MER program’s own accounting shows the two loads are comparable in size. Of 3,355 problem failure reports raised across MER development, 294 came out of environmental testing alone, with a per-test failure rate ranging from 0 percent for acoustics to 78 percent for EMC [9]; the same spacecraft went through 164 assemblies, 802 assembly and subsystem tests, 47 re-tests and 86 analyses before the bakeout and assay counts above were ever taken [9]. The environmental test laboratory campaign that produced those numbers ran flight-acceptance random vibration at 5.5 to 8.0 Grms, protoflight vibration and acoustic testing at 145 dB, and ten days of continuous solar-thermal-vacuum cruise simulation in the 1e-6 torr range, all before the vehicles that later returned the 101,000 and 209,000 spore totals were accepted for flight [10]. Bakeout and assay windows are scheduled around that qualification sequence, not instead of it.

Cleaning methods are characterized on coupons

Section titled “Cleaning methods are characterized on coupons”
MethodResultArticle
Laser induced plasma shockwave40 nm particles removed, up to 6-log spore reductioncoupons
Liquid boundary layer disruptionbetter than 4-log reduction at 99.9 percent confidencecoupons inoculated with 1e5 spores

Source: [5]. Both were measured at JPL. Neither has been demonstrated on flight hardware geometry, and laser plasma shockwave cleaning is not universally approved by the Planetary Protection Officer. Liquid boundary layer disruption removes microbes rather than killing them, which is the property that matters when the science requirement is organic detection at parts per billion.

The NASA Standard Assay takes more than 72 hours: sonication to dislodge, heat shock at 80 C for 15 minutes to select endospores, then plating on trypticase soy agar and 72 hours of incubation at 32 C [5][11]. Swabs cover 25 cm2 and polyester wipes about 1 m2 [5]. That turnaround is what makes assays a schedule driver during assembly, test and launch operations, because hardware waits on a result before the next access closes.

Faster methods exist with narrower coverage. A modified membrane filtration assay with ATP bioluminescence returns in under 8 hours at sensitivity measured as equivalent to the standard assay, both detecting one colony forming unit [5]. A Limulus amoebocyte lysate proxy returns in under an hour but detects only Gram-negative endotoxin and beta-glucan, about half the assembly-environment burden [5].

The assay is also a filter on what is known about the organisms themselves. JPL holds over 8000 strains isolated from missions carrying planetary protection requirements; 1249 of 1418 archived isolates revived within 72 hours in 2019, and 191 were sequenced across six missions from 1975 to 2012 [11]. Those 191 were selected for abundance and apparent novelty rather than at random, and anything unculturable under the standard assay is absent by construction [11]. An earlier pass over 188 archived MER isolates found the same skew toward two genera, Bacillus at 73.7 percent and Paenibacillus at 14.0 percent of the population, with 5 of 171 sequenced isolates falling below 97 percent homology to any known species [12]. Neither study reports a survival or resistance finding; both report what the culture-based assay happens to catch.

Cleanroom class does not order the airborne load

Section titled “Cleanroom class does not order the airborne load”

Real-time optical bioaerosol monitoring across five JPL assembly cleanrooms [13]:

RoomISO classVolumeBioaerosols
Facility 3793 m39,940,800 /m3
Facility 56117 m346,728 /m3
Facility 6698 m30 /m3
Facility 18417 m31,722 /m3
Facility 283,780 m3396 /m3

Source: [13]. Averages over triplicate 6 hour intervals at 28.3 L/min.

The ISO 7 room ran two to three orders of magnitude above every other room, including both ISO 6 rooms, and it was the smallest and the most crowded: 5 operators and a cumulative 23 plus or minus 6 operator-hours [13]. Operator activity tracks the load better than class does. In that room the biological share of total particle count ran 55 to 80 percent while work was underway and under 10 percent at rest, the only difference the study tested statistically, at p = 0.0264 with no correction for multiple comparisons [13]. About 91 percent of bioaerosols during work sat in the 0.5 and 1 um bins, which is where a conventional particle counter cannot separate biological from inert [13].

Two limits on reading that table. The counts are optically inferred from intrinsic fluorescence, not cultured organisms, so they are not colony forming units and not the spore bioburden requirements are written against. The ISO 6 zero is the instrument’s detection floor rather than a measurement, and with two rooms per class and three intervals per condition the study cannot separate class from room, volume or headcount [13]. Airborne count is also one step removed from what settles compliance, which is surface bioburden.

Sample return moves the requirement from forward to back contamination

Section titled “Sample return moves the requirement from forward to back contamination”

Everything above is a forward contamination requirement: keeping Earth life off another body. A mission that brings material back adds a second, harder requirement running the other way, and the design responses look different because the failure mode does.

Mars Sample Return’s science baseline once called for more than 500 g of returned sample, at least 1 km of surface mobility, sampling from at least 2 meters depth and at least 50 kg of lander science instruments; when the Mars Exploration Program’s budget was capped in 2001 to 2002, a science steering group deleted mobility, the drill, sample segregation and the in-situ science package to reach a floor-level stationary lander with a scoop, sieve and context camera [14]. Planetary protection requirements were part of what forced that descope, because a mission that returns unsterilized material must hold the probability of releasing a single viable organism to Earth’s biosphere below about 1e-6, several orders of magnitude tighter than the forward requirements above [14].

Mars 2020’s caching hardware shows what meeting a return requirement costs in hardware rather than in schedule. Sample-intimate surfaces are combustion cleaned at 350 C, coated in titanium nitride or gold, and protected by fluid mechanical particle barriers and molecular absorbers, with compliance argued through end-to-end particulate and molecular transport modeling rather than an end-to-end test, because no test article can be certified clean enough to stand in for the flight hardware [15]. The dominant contamination path the project modeled was not the caching hardware itself, which measured essentially zero on assay, a single colony forming unit on one hermetic seal and zero spore counts on the drill bits, but the rover as a whole: particles lofted by ambient Mars wind and redeposited where a sample is later taken [16]. The project’s conservative estimate for the probability of a single viable Earth organism riding home in a sample beat the requirement by more than an order of magnitude and its own best estimate by more than two [16].

Every dry heat and vapor hydrogen peroxide credit in the current specification rests on an assumed, not measured, fraction of heat-super-tolerant spores, stated as unknown and possibly varying with location, season and activity [5]. Mission bioburden totals for MSL and MER are accounting or worst-case estimates built from partial sampling and analytic credit, not direct counts, and every count above is culturable aerobic endospores by design, which bounds nothing about anaerobes, fungi, unculturable organisms, or the dead-but-chemically-detectable material an organic detection requirement is written against [5][6][11]. The 1973 critique of the underlying contamination probability model was never fully absorbed into a validated replacement; the category and special-region system that followed is a structural response to it, not a resolution of its statistics [3]. Novel cleaning methods are characterized on coupons at JPL, not on flight hardware geometry, and one of the two described here is not universally approved for flight use [5]. The bioaerosol monitoring behind the cleanroom table is a single-instrument, single-occasion measurement per facility, so facility, ISO class, room volume and operator count are confounded rather than separated [13]. And the sample-return contamination estimates for Mars 2020 are end-to-end models validated against near-zero hardware measurements, not against a returned sample, because no such sample yet exists to check them against [16].

References

  1. Pittendrigh, C. S., Vishniac, W. and Pearman, J. P. T. (1966). Biology and the Exploration of Mars . National Academy of Sciences, National Research Council, Publication 1296. Source
    BibTeX
    @book{pittendrigh1966biology,
      title = {Biology and the Exploration of Mars},
      author = {Pittendrigh, Colin S. and Vishniac, Wolf and Pearman, J. P. T.},
      editor = {Pittendrigh, Colin S. and Vishniac, Wolf and Pearman, J. P. T.},
      number = {Publication 1296},
      publisher = {National Academy of Sciences, National Research Council},
      address = {Washington, D.C.},
      year = {1966},
      url = {https://ntrs.nasa.gov/citations/19660027176},
      abstract = {Until recent years the origin of life and its possible occurrence elsewhere in the universe have been matters for speculation only. The rapid growth of molecular biology since 1940 has, to be sure, made it possible to discuss life's origins in far more precise and explicit terms than was possible earlier;
    and the subject entered a new experimental phase in the 1950's with successful abiogenic synthesis of important biochemical substances in conditions simulating the presumptive environment of the primitive Earth. But the real transformation that the subject has undergone stems from the spectacular growth of space technology in the last decade. The possibility of life's origin and occurrence on planets other than ours is no longer limited to idle speculation: it has entered the realm of the testable, of science in the strict sense. Given the rockets now available, and especially those available by 1969, it has become fully realistic to consider plans for the biological exploration of Mars.
    
    The study that this report seeks to interpret was initiated in June, 1964, by the Space Science Board of the National Academy of Sciences to examine this possibility. The working group comprised 36 people representing a broad spectrum of scientific interests: evolutionary biology, genetics, microbiology, biochemistry and molecular biology, animal physiology, soil chemistry, organic chemistry, planetary astronomy, geochemistry, and theoretical physics. The participants included some with considerable prior involvement in problems of space exploration and others with none.  Advice was also sought outside the group of immediate participants on the potentialities of selected analytical methods for the experimental study of extraterrestrial life and its environment. More than 30 individuals contributed in this fashion written assessments of techniques in which they were particularly well versed.
    
    Our task was to examine the scientific foundations and merits of the proposal to undertake a biological exploration of Mars. What are the potential scientific yields? How valuable, if attained, would they be? What, in fact, is the possibility of life occurring on Mars? And of our detecting it with available and foreseeable technology? What could be achieved by further astronomical work from Earth? by Martian fly-by missions? by Martian orbiters? and Martian Landers? What payloads would we recommend for planetary missions? What timing and over-all strategy would we recommend for Martian exploration were we to consider it worthwhile at all?
    
    In brief, the over-all purpose was to recommend to. the government, through the Academy's Space Science Board, whether or not a biological exploration of Mars should be included in the nation's space program over the next few decades; and, further, to outline what that program, if any, should be.}
    }
  2. Sagan, C., Levinthal, E. C. and Lederberg, J. (1967). Contamination of Mars . Smithsonian Institution Astrophysical Observatory, Cambridge, Massachusetts, NASA CR-89768; NGR-09-015-023. Source
    BibTeX
    @techreport{sagan1967contamination,
      title = {Contamination of Mars},
      author = {Sagan, Carl and Levinthal, Elliott C. and Lederberg, Joshua},
      volume = {159},
      number = {NASA CR-89768; NGR-09-015-023},
      pages = {1191-1196},
      institution = {Smithsonian Institution Astrophysical Observatory, Cambridge, Massachusetts},
      month = {6},
      year = {1967},
      doi = {10.1126/science.159.3820.1191},
      abstract = {Spacecraft sterilization standards and microbial contamination of Mars}
    }
  3. Harrison, J. M. and North, D. W. (1973). The Probabilistic Structure of Planetary Contamination Models . Stanford Research Institute, NASA CR-130558; SRI Project 2274, Project Memo 1. Source
    BibTeX
    @techreport{harrison1973probabilistic,
      title = {The Probabilistic Structure of Planetary Contamination Models},
      author = {Harrison, J. Michael and North, D. Warner},
      number = {NASA CR-130558; SRI Project 2274, Project Memo 1},
      institution = {Stanford Research Institute},
      month = {1},
      year = {1973},
      url = {https://ntrs.nasa.gov/citations/19730008376},
      abstract = {The analytical basis for planetary quarantine standards and procedures is presented. The heirarchy of planetary quarantine decisions is explained and emphasis is placed on the determination of mission specifications to include sterilization. The influence of the Sagan-Coleman probabilistic model of planetary contamination on current standards and procedures is analyzed. A classical problem in probability theory which provides a close conceptual parallel to the type of dependence present in the contamination problem is presented.}
    }
  4. Ezell, E. C. and Ezell, L. N. (1984). Viking Lander: Building a Complex Spacecraft . On Mars: Exploration of the Red Planet, -, NASA SP-4212, NASA-SP-4212. Source
    BibTeX
    @incollection{ezell1984viking,
      title = {Viking Lander: Building a Complex Spacecraft},
      author = {Ezell, Edward Clinton and Ezell, Linda Neuman},
      booktitle = {On Mars: Exploration of the Red Planet, -, NASA SP-4212},
      number = {NASA-SP-4212},
      publisher = {NASA},
      year = {1984},
      url = {https://ntrs.nasa.gov/citations/19840027185},
      abstract = {Various aspects of the design, testing, and preparation of the Viking lander spacecraft for Mars exploration are considered. The mission profile is given, including the entry into the Martian atmosphere and landing on the planet's surface. The return of scientific data to Earth is discussed. The top ten problem areas in the Viking lander project are enumerated, as are project costs. Pre-launch performance tests and preparation procedures are also addressed.}
    }
  5. Kazarians, G. A., Benardini, J. N., Stricker, M. C., Schubert, W. W., Chen, F., Vaishampayan, P., Jones, M. A., Barengoltz, J. and Koukol, R. (2017). The Evolution of Planetary Protection Implementation on Mars Landed Missions . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{kazarians2017evoluation,
      title = {The Evolution of Planetary Protection Implementation on Mars Landed Missions},
      author = {Kazarians, Gayane A. and Benardini, James N. and Stricker, Moogega C. and Schubert, Wayne W. and Chen, Fei and Vaishampayan, Parag and Jones, Melissa A. and Barengoltz, Jack and Koukol, Robert},
      booktitle = {IEEE Aerospace Conference},
      pages = {1-20},
      publisher = {IEEE},
      year = {2017},
      doi = {10.1109/aero.2017.7943576},
      abstract = {NASA has developed requirements dedicated to the prevention of forward and backward contamination during space exploration. Historically, international agreements provided guidelines to prevent contamination of the Moon and other celestial bodies, as well as the Earth (e.g., sample return missions). The UN Outer Space Treaty was established in 1967 and the Committee on Space Research (COSPAR) maintains a planetary protection policy complying with Article IX of this treaty. By avoiding forward contamination, the integrity of scientific exploration is preserved. Planetary Protection mission requirements are levied on missions to control contamination. These requirements are dependent on the science of the mission and on the celestial bodies encountered or targeted along the way. Consequently, categories are assigned to missions, and specific implementation plans are developed to meet the planetary protection requirements. NASA missions have evolved over time with increasingly more demanding scientific objectives and more complex flight systems to achieve those objectives and, thus, planetary protection methods and processes used for implementation have become much more intricate, complicated, and challenging. Here, we will portray the evolution of planetary protection implementation at JPL in several important areas throughout the course of NASA sponsored robotic Mars lander or rover missions, starting from Mars Pathfinder through the beginning of Mars 2020. Highlighted in the discussion will be process changes in planetary protection requirements development and flow down. Development and implementation of new and improved methods used in the reduction of spacecraft bioburden will be discussed as well as approaches and challenges that come along with setting up remote laboratories to perform bioassays. The consequences and forward planning of delays on missions will be highlighted as well as lessons learned on the impact of communication and training in achieving planetary protection requirements. The evolution of methods used for the detection of microbial bioburden on spacecraft hardware will be considered. These methods use standard microbiology as well as the adaptation of advances in biotechnology, molecular biology, and bioinformatics. Technical approaches developed for the prevention of contamination and recontamination of hardware during Assembly, Test, and Launch Operations will be discussed.}
    }
  6. Newlin, L. (2005). Planetary protection and its application to the Mars Exploration Rover (MER) Project . AIAA Aviation and Aeronautics Forum and Exposition. Source
    BibTeX
    @inproceedings{newlin2005planetary,
      title = {Planetary protection and its application to the Mars Exploration Rover (MER) Project},
      author = {Newlin, L.},
      booktitle = {AIAA Aviation and Aeronautics Forum and Exposition},
      publisher = {JPL Open Repository},
      year = {2005},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/37702}
    }
  7. Hand, K. P., Murray, A. E., Garvin, J. B., Brinckerhoff, W. B., Christner, B. C., Edgett, K. S., Ehlmann, B. L., German, C. R., Hayes, A. G., Hoehler, T. M., Horst, S. M., Lunine, J. I., Nealson, K. H., Paranicas, C., Schmidt, B. E., Smith, D. E., Rhoden, A. R., Russell, M. J., Templeton, A. S., Willis, P. A., Yingst, R. A., Phillips, C. B., Cable, M. L., Craft, K. L., Hofmann, A. E., Nordheim, T. A. and Pappalardo, R. P. (2017). Report of the Europa Lander Science Definition Team . NASA Jet Propulsion Laboratory, JPL D-97667. [no online locator recorded]
    BibTeX
    @techreport{europa2017lander,
      title = {Report of the Europa Lander Science Definition Team},
      author = {Hand, Kevin P. and Murray, A. E. and Garvin, James B. and Brinckerhoff, William B. and Christner, B. C. and Edgett, Kenneth S. and Ehlmann, Bethany L. and German, Christopher R. and Hayes, Alexander G. and Hoehler, T. M. and Horst, S. M. and Lunine, Jonathan I. and Nealson, Kenneth H. and Paranicas, C. and Schmidt, B. E. and Smith, David E. and Rhoden, A. R. and Russell, M. J. and Templeton, A. S. and Willis, Peter A. and Yingst, R. Aileen and Phillips, Cynthia B. and Cable, M. L. and Craft, Kathleen L. and Hofmann, Amy E. and Nordheim, T. A. and Pappalardo, R. P.},
      number = {JPL D-97667},
      institution = {NASA Jet Propulsion Laboratory},
      year = {2017}
    }
  8. Newlin, L., Barengoltz, J., Chung, S., Kirschner, L., Koukol, R. and Morales, F. (2002). Microbiological cleanliness of the Mars Exploration Rover spacecraft. dataverse.jpl.nasa.gov/dataset.xhtml
    BibTeX
    @misc{newlin2002microbiological,
      title = {Microbiological cleanliness of the Mars Exploration Rover spacecraft},
      author = {Newlin, L. and Barengoltz, J. and Chung, S. and Kirschner, L. and Koukol, R. and Morales, F.},
      year = {2002},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/9627}
    }
  9. Man, K. F., Farguson, C. T. and Hoffman, A. R. (2004). Mars Exploration Rover (MER) project environmental assurance program . The International Symposium on Artificial Intelligence, Robotics, and Automation in Space. Source
    BibTeX
    @inproceedings{man2004mars,
      title = {Mars Exploration Rover (MER) project environmental assurance program},
      author = {Man, Kin F. and Farguson, Christine T. and Hoffman, Alan R},
      booktitle = {The International Symposium on Artificial Intelligence, Robotics, and Automation in Space},
      publisher = {JPL Open Repository},
      year = {2004},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/39028}
    }
  10. Fisher, T. C. and Van Velzer, P. L. (2004). Environmental test program for the Mars Exploration Rover Project . International Symposium on Environmental Testing for Space Programs. Source
    BibTeX
    @inproceedings{fisher2004environmental,
      title = {Environmental test program for the Mars Exploration Rover Project},
      author = {Fisher, Terry C. and Van Velzer, Paul L.},
      booktitle = {International Symposium on Environmental Testing for Space Programs},
      publisher = {JPL Open Repository},
      year = {2004},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/38001}
    }
  11. Tran, M. T., Seuylemezian, A., Wright, A., Coil, D., Eisen, J. and Guan, L. (2023). Draft Genome Sequence of Spacecraft Associated Microbes Isolated from 6 NASA missions (Viking, Mars Pathfinder, Mars Odyssey, MER, Phoenix, and MSL) . International Symposium on Robotics and Applications. Source
    BibTeX
    @inproceedings{tran2023draft,
      title = {Draft Genome Sequence of Spacecraft Associated Microbes Isolated from 6 NASA missions (Viking, Mars Pathfinder, Mars Odyssey, MER, Phoenix, and MSL)},
      author = {Tran, Michelle T. and Seuylemezian, Arman and Wright, Alonna and Coil, David and Eisen, Jonathan and Guan, Lisa},
      booktitle = {International Symposium on Robotics and Applications},
      publisher = {JPL Open Repository},
      year = {2023},
      doi = {10.48577/jpl.1kyqqc},
      abstract = {Whole-genome sequencing can be used to better understand and assess functional abilities of microorganisms isolated from spacecraft hardware and associated surfaces for planetary protection purposes. We sequenced 190 isolates from 6 spaceflight missions with PP requirements and identified them using Illumina-based sequencing, 16S rRNA, MALDI-TOF MS and GTDB-Tk.}
    }
  12. Arora-Williams, K. (2012). Genotypic & phenotypic diversity of microbial isolates from the Mars Exploration Rovers . NASA Experimental Program to Stimulate Competitive Research and Amgen Scholar Program. Source
    BibTeX
    @techreport{arorawilliams2012genotypic,
      title = {Genotypic & phenotypic diversity of microbial isolates from the Mars Exploration Rovers},
      author = {Arora-Williams, Keith},
      booktitle = {NASA Experimental Program to Stimulate Competitive Research and Amgen Scholar Program},
      publisher = {JPL Open Repository},
      institution = {NASA Experimental Program to Stimulate Competitive Research (EPSCoR) and Amgen Scholar Program, Pasadena, California},
      year = {2012},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/44141}
    }
  13. Yearicks, S., Ahmed, M., Rivera, A. and Vaishampayan, P. (2023). Real-time Quantification of Size-Resolved Bioaerosols and Inert Particles in Spacecraft Assembly Facilities at the NASA Jet Propulsion Laboratory . Astrobiology. Source
    BibTeX
    @inproceedings{yearicks2023real,
      title = {Real-time Quantification of Size-Resolved Bioaerosols and Inert Particles in Spacecraft Assembly Facilities at the NASA Jet Propulsion Laboratory},
      author = {Yearicks, Sarah and Ahmed, Mahjabeen and Rivera, Angie and Vaishampayan, Parag},
      booktitle = {Astrobiology},
      publisher = {JPL Open Repository},
      year = {2023},
      doi = {10.48577/jpl.ablflh},
      abstract = {Responsible space exploration is a cornerstone of planetary protection, particularly at sites in the solar system with a high potential for the existence of extant life. To limit bioburden, spacecraft assembly occurs in cleanrooms facilities. Cleanroom levels are established through air particulate counters; which can assess particle size distribution and concentration but cannot detect bioaerosols. Additionally, these devices do not detect in real-time, posing a risk to critical flight hardware assemblies or even mission timelines. A first-of-its-kind study was conducted to simultaneously detect bioaerosols, inert particles, and their size distribution in real-time, in operational spacecraft assembly cleanrooms at NASA’s Jet Propulsion Laboratory in Pasadena, CA, USA, using the BioVigilant IMD-A® 350 (Azbil Corporation, Tucson AZ, USA). The IMD-350A continuously sampled during operations and no-operation six-hour intervals in two facilities per cleanroom class: ISO-6, ISO-7, and ISO-8. A positive correlation was established between human presence in the cleanroom and elevated bioaerosol counts. Smaller particles of sizes 0.5 µm and 1 µm constituted an average ~91% of the total bioaerosols detected in "At Work" intervals across all ISO classes observed. The results of this study were used to establish bioburden particulate thresholds for the most stringent JPL cleanrooms used in the assembly of the Sample Caching System for the Mars 2020 Perseverance rover.}
    }
  14. Mattingly, R., Matovsek, S. and Jordan, F. (2002). Mars sample return, updated to a groundbreaking approach . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{mattingly2002mars,
      title = {Mars sample return, updated to a groundbreaking approach},
      author = {Mattingly, Richard and Matovsek, S. and Jordan, Frank},
      booktitle = {IEEE Aerospace Conference},
      volume = {2},
      pages = {2_745-2_758},
      publisher = {IEEE},
      year = {2002},
      doi = {10.1109/aero.2003.1235485},
      abstract = {A Mars Sample Return (MSR) mission is a goal of the Mars Program. Recently, NASA and JPL have been studying the possibility of a Mars Sample Return some time in the next decade of Mars exploration. In 2001, JPL commissioned four industry teams to make a fresh examination of MSR architectures. Six papers on these studies were presented at last year's conference. As new fiscal realities of a cost-capped Mars Exploration Program unfolded, it was evident that these MSR concepts, which included mobility and subsurface sample acquisition, did not fit reasonably within a balanced program. Therefore, at the request of NASA and the science community, JPL asked the four industry teams plus JPL's Team X to explore ways to reduce the cost of a MSR. A NASA-created MSR Science Steering Group (SSG) established a reduced set of requirements for these new studies that built upon the previous year's work. As a result, a new 'Groundbreaking' approach to MSR was established that is well understood based on the studies and independent cost assessments by Aerospace Corporation and SAIC. The Groundbreaking approach appears to be what a contemporary, balanced Mars Exploration Program can afford, has turned out to be justifiable by the MSR Science Steering Group, and has been endorsed by the Mars science community at large. This paper gives a brief overview of the original 2001 study results and discusses the process leading to the new studies, the studies themselves, and the results.}
    }
  15. White, L., Anderson, M., Blakkolb, B., Kipp, K., Stricker, M., Benardini, J. N., Mikellides, I., Katz, I., Bernard, D., Jandura, L., Rosette, K., Rainen, R. and Steltzner, A. (2019). Organic and inorganic contamination control approaches for return sample investigation on Mars 2020 . International Astronautical Congress. Source
    BibTeX
    @inproceedings{white2019organic,
      title = {Organic and inorganic contamination control approaches for return sample investigation on Mars 2020},
      author = {White, Lauren and Anderson, Mark and Blakkolb, Brian and Kipp, Kristina and Stricker, Moogega and Benardini, James N. and Mikellides, Ioannis and Katz, Ira and Bernard, Doug and Jandura, Louise and Rosette, Keith and Rainen, Richard and Steltzner, Adam},
      booktitle = {International Astronautical Congress},
      publisher = {JPL Open Repository},
      year = {2019},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/51011}
    }
  16. Chen, F., Ly, C., Mikellides, I., Bernard, D. and Cooper, M. (2023). Mars 2020 Mission Biological Return Sample Contamination Control Approach and Verification . International Symposium on Artificial Intelligence, Robotics and Automation in Space (i-SAIRAS). Source
    BibTeX
    @inproceedings{chen2023mars,
      title = {Mars 2020 Mission Biological Return Sample Contamination Control Approach and Verification},
      author = {Chen, Fei and Ly, Cynthia and Mikellides, Ioannis and Bernard, Douglas and Cooper, Moogega},
      booktitle = {International Symposium on Artificial Intelligence, Robotics and Automation in Space (i-SAIRAS)},
      publisher = {JPL Open Repository},
      year = {2023},
      doi = {10.48577/jpl.uhgyrr},
      abstract = {The Mars 2020 Perseverance rover is equipped with a Sample Caching System (SCS) designed to collect and cache Martian core and regolith samples for potential return to Earth. To ensure the integrity of these samples, the mission requirements for each encapsulated sample for return is less than one Earth-sourced viable organism (VO) and more than a 99.9% probability of being free of any Earth-sourced VO. To satisfy the stringent biological contamination requirements in support of return sample science (RSS) investigations, special bioburden mitigation and reduction approaches were developed and implemented for SCS hardware that would directly contact or be in close proximity to the Martian samples. Here, we describe the implemented approaches for microbiological contamination reduction and mitigation, detail the processes of the SCS aseptic assembly, and report the estimated VO for each returned sample. We found that our conservative estimate (CE) of the computed probability of a single VO in the returned sample is more than one order of magnitude lower than the biological contamination requirement while the best estimate (BE) exceeds two orders of magnitude.}
    }