Inner Workings: Hunting for Microbial Life Throughout the Solar System
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20 Years Building Astrobiology
ASTROBIOLOGY Volume 20, Number 9, 2020 Special Collection Articles Mary Ann Liebert, Inc. DOI: 10.1089/ast.2020.0804 Introduction—Centro de Astrobiologı´a: 20 Years Building Astrobiology Vı´ctor Parro,1 J. Miguel Mas-Hesse,1 Javier Gomez-Elvira,1,2 A´ lvaro Gime´nez,1 and Juan Pe´rez-Mercader3 The Origins example of life, and we do not know how it was generated. It would require a team of scientists with a truly scientific he Centro de AstroBiologı´a (CAB) was founded in and professional knowledge and understanding of the TNovember 1999 as a joint institute between the Spanish various components of the puzzle. National Research Council (CSIC) and the National Institute That team began to emerge in Madrid, with scientists for Aerospace Technologies (INTA). Located in Madrid working in galactic astrophysics, planetary science, evolu- (Spain), CAB became the first astrobiology organization outside tion of life and of viruses, origins-of-life chemistry, meta- the United States to be associated with the NASA Astrobiology bolic processes in biochemistry, evolution of planets, Institute (NAI)—formally becoming an associate member in bioinformatics, extremophiles, and physics, together with the year 2000. Astrobiology considers life as a natural conse- engineers to design and produce instrumentation. This group, quence of the evolution of the Universe, and CAB aims to study from a variety of universities and government research cen- the origin, evolution, distribution, and future of life in the ters, such as INTA (Instituto Nacional de Te´cnica Aero- Universe, from an integrative transdisciplinary approach. espacial) and CSIC (Consejo Superior de Investigaciones CAB’s foundation was the result of a profound interest Cientı´ficas), started informal discussions; and a passion for in applying the scientific method to life—in the sense of the subject of astrobiology began to burn. -
Contamination Control Technology Study for Achieving the Science Objectives of Life-Detection Missions
Contamination Control Technology Study for Achieving the Science Objectives of Life-Detection Missions Study Team: Chris McKay, NASA ARC, (650)604-6864, [email protected] (submitting author) Alfonso Davila, NASA ARC, [email protected] Jennifer Eigenbrode, NASA GSFC, [email protected] Chris Lorentson, NASA GSFC, [email protected] Rob Gold, JHU/APL, [email protected] John Canham, Northrop Grumman/NASA GSFC, [email protected] Anthony Dazzo, KBR Inc./NASA GSFC, [email protected] Therese Errigo, NASA GSFC, [email protected] Faith Kujawa, JHU/APL, [email protected] Dave Kusnierkiewicz, JHU/APL, [email protected] Charles Sandy, ILC Dover, crsandy @ilcdover.com Erich Schulze, JHU/APL, Erich.Schulze@jhuapl Antonios Seas, NASA GSFC [email protected] Science Contamination Control Technology Study Summary: This white paper summaries technological advances in science-required contamination-control engineering for in situ and sample-return life-detection missions in the Solar System. Key study results are: 1) New spacecraft !arrier design that accommodates MMRT$s% is cleana!le% and is repaira!le. &) 'urge gas cleanliness of 1 part per trillion HC impurity limit is feasible. )) The !arrier reduces particle contamination *likely !iological) from fairing to spacecraft !y 1, -&-1,-). -) Spacecraft surfaces protected !y !arrier are 1,-&,. cleaner after launch than !efore launch. /) 0n-1ight !a+e-out of critical surfaces significantly reduced molecular contamination *!y 1,-3 to 1,-1&). 0mplementing a full spacecraft !arrier% collector cover and purge% and in-1ight cleaning steps will achieve cleanliness levels required of science instruments *down to femtomolar levels of !iomolecules). -
Periodic Habitability in Northern Plains Ground Ice: the Icebreaker Life Mission Plan
Astrobiology Science Conference 2017 (LPI Contrib. No. 1965) 3478.pdf PERIODIC HABITABILITY IN NORTHERN PLAINS GROUND ICE: THE ICEBREAKER LIFE MISSION PLAN. C. Stoker1, C. McKay1, A. Davila1 , B. Glass2, V. Parro3, 1 Space Science Division, NASA Ames Research Center, Moffett Field CA, 2Exploration Technology Division, NASA Ames Research Center, Moffett Field CA, 3Centro de Astrobiología (INTA-CSIC), Madrid, Spain Introduction:The results from the 2008 Phoenix and future proposals are planned. The mission returns mission that sampled ground ice at 68oN latitude, along to the well-characterized Phoenix landing site with a with climate modeling studies, indicate that the high N. payload designed to address the following science latitude ice-rich regolith at low elevations is likely to goals: (1) search for biomolecular evidence of life; (2) be a recently habitable place on Mars [1]. search for organic matter from either exogeneous or Habitable Conditions Evidence: Ice was found endogeneous sources using methods that are not within 3-5 cm of the surface. If warmer conditions spoiled by the presence of perchlorate; (3) characterize occur, the ice could provide a source of liquid water. oxidative species that produced reactivity of soils seen Phoenix found evidence for liquid water processes by Viking; and 4) assess the habitability of the ice including 1) beneath 3 -5 cm of dry soil, segregated bearing soils. The Icebreaker Life payload hosts a 1-m pure ice was discovered in patches covering 10% of drill that brings cuttings samples to the surface where the area explored, 2) calcite mineral was detected in they are delivered to three instruments. -
Space Biology Research and Biosensor Technologies: Past, Present, and Future †
biosensors Perspective Space Biology Research and Biosensor Technologies: Past, Present, and Future † Ada Kanapskyte 1,2, Elizabeth M. Hawkins 1,3,4, Lauren C. Liddell 5,6, Shilpa R. Bhardwaj 5,7, Diana Gentry 5 and Sergio R. Santa Maria 5,8,* 1 Space Life Sciences Training Program, NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (A.K.); [email protected] (E.M.H.) 2 Biomedical Engineering Department, The Ohio State University, Columbus, OH 43210, USA 3 KBR Wyle, Moffett Field, CA 94035, USA 4 Mammoth Biosciences, Inc., South San Francisco, CA 94080, USA 5 NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (L.C.L.); [email protected] (S.R.B.); [email protected] (D.G.) 6 Logyx, LLC, Mountain View, CA 94043, USA 7 The Bionetics Corporation, Yorktown, VA 23693, USA 8 COSMIAC Research Institute, University of New Mexico, Albuquerque, NM 87131, USA * Correspondence: [email protected]; Tel.: +1-650-604-1411 † Presented at the 1st International Electronic Conference on Biosensors, 2–17 November 2020; Available online: https://iecb2020.sciforum.net/. Abstract: In light of future missions beyond low Earth orbit (LEO) and the potential establishment of bases on the Moon and Mars, the effects of the deep space environment on biology need to be examined in order to develop protective countermeasures. Although many biological experiments have been performed in space since the 1960s, most have occurred in LEO and for only short periods of time. These LEO missions have studied many biological phenomena in a variety of model organisms, and have utilized a broad range of technologies. -
Uncorrected Proof
Planetary and Space Science xxx (xxxx) xxx-xxx Contents lists available at ScienceDirect Planetary and Space Science journal homepage: http://ees.elsevier.com Joint Europa Mission (JEM) a multi-scale study of Europa to characterize its habitability and search for extant life Michel Blanc a,∗, Nicolas André a, Olga Prieto-Ballesteros b, Javier Gomez-Elvira b, Geraint Jones c, Veerle Sterken d,e, William Desprats a,f, Leonid I. Gurvits g,p,ak, Krishan Khurana h, Aljona Blöcker i, Renaud Broquet j, Emma Bunce k, Cyril Cavel j, Gaël Choblet l, Geoffrey Colins m, Marcello Coradini n, John Cooper o, Dominic Dirkx p, Philippe Garnier a, David Gaudin f, Paul Hartogh q, Luciano Iess r, Adrian Jäggi d, Sascha Kempf s, Norbert Krupp q, Luisa Lara t, Jérémie LasuePROOFa, Valéry Lainey u, François Leblanc v, Jean-Pierre Lebreton w, Andrea Longobardo x, Ralph Lorenz y, Philippe Martins z, Zita Martins aa, Adam Masters ab,al, David Mimoun f, Ernesto Palumba x, Pascal Regnier j, Joachim Saur ac, Adriaan Schutte ad, Edward C. Sittler o, Tilman Spohn ae, Katrin Stephan ae, Károly Szegő af, Federico Tosi x, Steve Vance ag, Roland Wagner ae, Tim Van Hoolst ah, Martin Volwerk ai, Frances Westall aj a IRAP, France b INTA-CAB, Spain c MSSL/UCL, UK d University of Bern, Switzerland e ETH Zürich, Switzerland f ISAE, France g Joint Institute for VLBI ERIC, Dwingeloo, the Netherlands h UCLA, USA i Royal Institute of Technology KTH, Sweden j Airbus D&S, France k Univ. Leicester, UK l LPG, Univ. Nantes, France mWheaton College, USA n CSEO, USA o GSFC, USA p TU Delft, the Netherlands q MPS, Germany r Univ. -
Carbon Monoxide As a Metabolic Energy Source for Extremely Halophilic Microbes: Implications for Microbial Activity in Mars Regolith
Carbon monoxide as a metabolic energy source for extremely halophilic microbes: Implications for microbial activity in Mars regolith Gary M. King1 Department of Biological Sciences, Louisiana State University, Baton Rouge, LA 70803 Edited by David M. Karl, University of Hawaii, Honolulu, HI, and approved March 5, 2015 (received for review December 31, 2014) Carbon monoxide occurs at relatively high concentrations (≥800 that low organic matter levels might indeed occur in some deposits parts per million) in Mars’ atmosphere, where it represents a poten- (e.g., 12). Even so, it is uncertain whether this material exists in a tially significant energy source that could fuel metabolism by a local- form or concentrations suitable for microbial use. ized putative surface or near-surface microbiota. However, the The Martian atmosphere has largely been ignored as a potential plausibility of CO oxidation under conditions relevant for Mars in energy source, because it is dominated by CO2 (24, 25). Ironically, its past or at present has not been evaluated. Results from diverse UV photolysis of CO2 forms carbon monoxide (CO), a potential terrestrial brines and saline soils provide the first documentation, to bacterial substrate that occurs at relatively high concentrations: our knowledge, of active CO uptake at water potentials (−41 MPa to about 800 ppm on average, with significantly higher levels for −117 MPa) that might occur in putative brines at recurrent slope some sites and times (26, 27). In addition, molecular oxygen lineae (RSL) on Mars. Results from two extremely halophilic iso- (O2), which can serve as a biological CO oxidant, occurs at lates complement the field observations. -
Robotics and Automation for “Icebreaker” B.J
ROBOTICS AND AUTOMATION FOR “ICEBREAKER” B.J. Glass (1), G. Paulsen(2), A. Dave (1), C. McKay(1) (1) NASA Ames Research Center, Moffett Field, CA 94035 USA; Email: [email protected] (2) Honeybee Robotics, Pasadena, CA 91103 USA; Email: [email protected] ABSTRACT components that will penetrate below the ground, and place these inside a biobarrier. To prevent The proposed “Icebreaker” mission is a return to spores from traveling onto the drill auger/bit via the Mars polar latitudes first visited by the Phoenix sample transfer, there must be an air gap between mission in 2007-08. Exploring and interrogating the sterilized drill and a less-sterilized robotic the shallow subsurface of Mars from the surface sample delivery subsystem that could contact the will require some form of excavation and “dirty” spacecraft instruments (which will not be penetration, with drilling being the most mature heat sterilized to Viking standards). approach. A series of 0.5-5m automated rotary and rotary-percussive drills developed over the past Since 2006, NASA has developed a Discovery- decade by NASA Ames and Honeybee Robotics class mission concept, called "Icebreaker" (Fig. 1), provide a capability that could fly on a Mars which is a Lockheed-Martin (Phoenix-derived) surface mission within the next decade. Surface Mars polar lander with life and organics detection robotics have been integrated for sample transfer to instruments and a 1m sampling drill [4]. The deck instruments, and the Icebreaker sample Icebreaker science payload has since 2010 also acquisition system has been tested successfully in been the baseline science payload for developing a Mars chambers and analog field sites to depths joint NASA-commercial Mars astrobiology between 1-3m. -
Contamination Control Technology Study for Achieving the Science Objectives of Life-Detection Missions
NASA/TM-20205008709 Contamination Control Technology Study for Achieving the Science Objectives of Life-Detection Missions Chris McKay, Alfonso Davila, Jennifer Eigenbrode, Chris Lorentson, Rob Gold, John Canham, Northrop Grumman, Anthony Dazzo, Therese Errigo, Faith Kujawa, Dave Kusnierkiewicz, Charles Sandy, Erich Schulze and Antonios Seas, October 2020 NASA STI Program ... in Profile Since its founding, NASA has been dedicated CONFERENCE PUBLICATION. to the advancement of aeronautics and space Collected papers from scientific and science. The NASA scientific and technical technical conferences, symposia, seminars, information (STI) program plays a key part in or other meetings sponsored or helping NASA maintain this important role. co-sponsored by NASA. The NASA STI program operates under the SPECIAL PUBLICATION. Scientific, auspices of the Agency Chief Information Officer. technical, or historical information from It collects, organizes, provides for archiving, and NASA programs, projects, and missions, disseminates NASA’s STI. The NASA STI often concerned with subjects having program provides access to the NTRS Registered substantial public interest. and its public interface, the NASA Technical Reports Server, thus providing one of the largest TECHNICAL TRANSLATION. collections of aeronautical and space science STI English-language translations of foreign in the world. Results are published in both non- scientific and technical material pertinent to NASA channels and by NASA in the NASA STI NASA’s mission. Report Series, which includes the following report types: Specialized services also include organizing and publishing research results, distributing TECHNICAL PUBLICATION. Reports of specialized research announcements and completed research or a major significant feeds, providing information desk and personal phase of research that present the results of search support, and enabling data exchange NASA Programs and include extensive data services. -
Figure 1 (Left) SOLID Instrument Block Diagram Showing 3 Main Modules. Power Is Provided by ICU, Which Collects Internal Senso
Eighth International Conference on Mars (2014) 1069.pdf THE SIGNS OF LIFE DETECTOR (SOLID): AN INSTRUMENT TO DETECT MOLECULAR BIOSIGNATURES ON MARS. V. Parro1, C. Stoker2, A.F. Davila3, R. Quinn4., Javier Gomez-Elvira1 1Centro de Astrobiología ([email protected]), 2NASA Ames Research Center ([email protected]), 3Carl Sagan Center at the SETI Institiute ([email protected]), 4Carl Sagan Center at the SETI Institiute ([email protected]). Introduction: The case for life on Mars grows fluorescence images with the results of the immunoas- stronger. Investigations at Gale Crater by Curiosity say. have revealed fine-grained sedimentary rocks inferred Conceptually, immunoassays mimic our immune to represent an ancient lake environment suited to sup- system in that a fleet of antibodies (Ab) is designed to port life [1]. In addition, Curiosity tentatively found a chemically capture desired organic compounds termed heterogeneous distribution of organic carbon within antigens (Ag) in solution. Antibodies possess high these sediments [2], consistent with the detection of specificity and affinity for their respective Ag, making native organic C in Mars meteorites. Futhermore, immunoassays both reliable and sensitive, with con- modern potentially habitable environments have been firmed detection limits of a few ppb for specific com- recognized on Mars including the N. Polar region vis- pounds. For analysis, the liquid extract obtained in the ited by Phoenix [3], gully featuers suggesting modern SPU is exposed to a fleet of Ab’s designed to anchor to water flows [4], and RSLs that occur seasonally sug- a specific region of the target organic compound. Spe- gest liquid processes[5]. -
It's Life… Isn't
It’s life… isn’t it? Scientists find it hard enough to pin down evidence of early life on our own planet. How on Earth do we plan to determine whether life exists elsewhere? John Whitfield finds out. e can, it’s fair to say, be confident their research agendas towards looking for As a control,the landers did the same tests on that there’s life on Earth — but life,says chemist Richard Mathies of the Uni- a heat-sterilized sample of martian soil. ASA/SPL Wproving it is a different matter. In versity of California,Berkeley.“Exobiology is Remarkably, every test gave a positive N December 1990, the Galileo spacecraft becoming more prominent,” he says. NASA result. The soil samples released oxygen and pointed its sensors back at Earth before and the European Space Agency (ESA) are compounds made from ingredients in the setting off for Jupiter. The probe reported moving from rock and mineral experiments nutrient solution, and carbon in the experi- an atmosphere abundant in oxygen and to biological ones, he explains. In 2009, both ment seemed to be incorporated into unusually rich in methane. It also detected a agencies will send landers to Mars that, organic molecules. Unfortunately, most of mysterious pigment that was unlikely to be unlike the Spirit and Opportunity rovers the controls — except the experiments of mineral origin: something earthlings call now on the planet, will be designed to look designed to detect nutrient uptake — also chlorophyll. Yet the astrophysicist Carl for the chemistry of life. gave positive results. At the same time, two Sagan and his colleagues were still cautious Astrobiologists are currently working out instruments designed to analyse the planet’s in their conclusions based on these results. -
Planetary & Solar System Sciences
EGU General Assembly 2012 EGU General Assembly 2012 Programme Group Programme PS – Planetary & Solar System Sciences Monday, 23 April ........................................................................................................................................................................ 2 PS1.1 ........................................................................................................................................................................................ 2 PS2.2 ........................................................................................................................................................................................ 2 GD1.1/PS2.7 .............................................................................................................................................................................. 3 PS3.3 ........................................................................................................................................................................................ 4 PS5.3/ST6.4 ............................................................................................................................................................................... 4 ST2.4/PS5.4 ............................................................................................................................................................................... 6 Tuesday, 24 April ...................................................................................................................................................................... -
Presentación De Powerpoint
Center for Astrobiology The origin of life and the evolution of the Universe CAB: Center for Astrobiology Understanding the origin and evolution of life along the history of the Universe • How, where and when did life emerge? • How did it evolve towards intelligence and consciousness? • What is the future of life on Earth and beyond? 10 billion ~13 years billion years 92% Hydrogen Formation of elements Emergence of life Complex life and first exoplanets Intelligence CAB: Center for Astrobiology Transdisciplinary approach − Astrophysics − Geology/Planetology − Biology/Biochemistry − Planetary exploration − Simulation chambers − Engineering 3 CAB: Center for Astrobiology • Founded in 1999 as a joint institute INTA + CSIC – Close collaboration with the INTA technical laboratories, specially for the development of space missions. – Multidisciplinary scientists formed within CSIC. • Since 2000 associated to the NASA Astrobiology Institute 4 Departments and groups • Astrophysics: – Formation and evolution of galaxies – Interstellar and circumstellar medium – Formation and evolution of stars, brown dwarfs and planets – Virtual Observatory and astronomical archives • Planetology and habitability: – Planetary geology and atmospheres – Habitability – Extremophiles and extreme environments 5 Departments and groups • Molecular evolution: – Biomolecules in planetary exploration – Molecular evolution and genomics – Prebiotic chemistry – Molecular mechanisms of the biological adaptation • Instrumentation: – Space instrumentation – Simulation chambers 6 Simulation chambers • Mars environment simulation chamber • High pressure planetary chambers • Planetary atmosphere and surface chamber • Interstellar astrochemistry chamber • Cryogenic vacuum chamber for detector testing • Projectile impact facility 8 Space missions • Astrophysics (in development) − PLATO (M3 ESA): exoplanets characterization − X-IFU/Athena (L2 ESA): X-rays − Safari/SPICA (ESA-JAXA): Far Infrared 9 Space missions • Planetary exploration − REMS (NASA MSL Curiosity): In operation since August 2012.