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Gilbert Levin
Gilbert Levin
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Gilbert Victor Levin (April 23, 1924 – July 26, 2021) was an American engineer, the founder of Biospherics and the principal investigator of the Viking mission Labeled Release experiment.[1] He was born in Baltimore, Maryland, to a Jewish family; his father was an immigrant from Lithuania.[2][3]

In 1997, Levin published his conclusion that a 1976 Viking lander had discovered living microorganisms on Mars.[1][4] He is noted for still claiming that his experiment on board the 1976 Viking Mars landers to detect microscopic life on Mars rendered a true positive result. On April 12, 2012, an international team including Levin reported their analysis "support the interpretation that the Viking LR experiment did detect extant microbial life on Mars." The team used cluster analysis of the Labeled Release experiments of the Viking program.[5][6][7]

He was one of the science advisers of the International Committee Against Mars Sample Return.[8][9]

He also patented an inexpensive method to make tagatose, an artificial sweetener, in 1988.[10]

Levin died in Bethesda, Maryland after an aortic dissection on July 26, 2021, at the age of 97.[2][11]

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References

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from Grokipedia
Gilbert Levin is an American engineer and scientist known for his role as principal investigator of the Labeled Release (LR) experiment on NASA's twin Viking landers in 1976, which produced results he interpreted as evidence of microbial life on Mars. The LR experiment, based on his patented radiospirometry technique originally developed to detect microbial activity in clinical samples, supplied radioactively labeled nutrients to Martian soil and detected gas releases consistent with metabolism on both landers. Despite the absence of organic molecules detected by other Viking instruments and prevailing scientific explanations attributing the results to non-biological chemical reactions, Levin maintained that the data indicated extant life, continuing to publish defenses of this view for decades. Born in 1924, Levin founded Biospherics Incorporated in Rockville, Maryland, where he directed biotechnology research and information services on health and public interest topics. He served on NASA's planetary quarantine advisory panel from 1967 to 1973 and contributed to early Mars sample return studies. In 1999 he became a founding member and scientific advisor to the International Committee Against Mars Sample Return, citing concerns over potential contamination risks. Levin received awards from NASA and Johns Hopkins University, where he served on national engineering and library advisory councils. He died on July 26, 2021, in Bethesda, Maryland, at the age of 97.

Early life and education

Family background and childhood

Gilbert Victor Levin was born on April 23, 1924, in Baltimore, Maryland, to Jewish parents. His father, a Jewish immigrant from Lithuania, operated an antiques business. Levin grew up in Baltimore and graduated from Forest Park High School. He later entered the Johns Hopkins University School of Engineering in 1941.

Education and World War II service

Gilbert Levin entered the Johns Hopkins University School of Engineering in 1941. His studies were interrupted in 1944 during World War II, in his junior year, when he joined the U.S. Maritime Service and trained as a shipboard radio operator. He served on merchant ships in combat zones across the Atlantic, North Atlantic, Mediterranean, Pacific, and Indian Oceans until leaving the service in 1946. In a personal account, Levin described becoming a shipboard radio operator in the Merchant Marine, sailing around the world for over two years during the war. After returning to Johns Hopkins in 1946, Levin earned his B.E. in Civil Engineering in 1947 and his M.S. in Sanitary Engineering in 1948. He later returned to the university as a full-time student while working professionally and obtained his Ph.D. in Environmental Engineering in 1963.

Environmental engineering career

Public health engineering roles

After earning his master's degree in sanitary engineering in 1948, Gilbert Levin worked as a public health engineer in the health departments of Maryland, California, and the District of Columbia. In Maryland, he served as a sanitary engineer focused on public health concerns related to water and environmental quality. His subsequent role in California around 1951 involved assessing sewage pollution in Santa Monica Bay, where he collected water samples twice weekly to track bacterial contamination stemming from approximately 300 million gallons per day of partially treated sewage discharged into the bay, with the aim of determining quarantine limits for swimmers. The standard bacteriological testing methods available at the time required up to three days for microorganisms to produce detectable gases in test tubes, followed by additional reporting delays, making results outdated for urgent public health responses. In 1952, while employed as a public health engineer in the District of Columbia, Levin developed a faster approach by incorporating carbon-14 labeled nutrients into microbiological test media, allowing detection of contaminating bacteria through measurement of minute amounts of radioactive gas in about one hour. This technique was pursued with a grant from the Atomic Energy Commission and conducted at the Georgetown School of Medicine under the approval of the D.C. Department of Public Health director. In 1955, Levin co-founded Resources Research Inc. with Dr. Louis McCabe, formerly director of the Los Angeles County Air Pollution Control District, to operate as an environmental consulting and research firm. His earlier development of radioisotope-based microbial detection methods during his public health roles later attracted NASA interest for potential extraterrestrial applications.

Founding and leadership of Biospherics

In 1967, Gilbert Levin founded Biospherics Research Inc., a bioengineering firm specializing in environmental and health-related technologies that was later renamed Spherix Incorporated. He served as the company's CEO and President until 2003, remained as Chairman of the Board until 2007, and retired from the company in 2008. Under Levin's leadership, Biospherics/Spherix secured over 50 patents across diverse areas including therapeutics, pesticides, and wastewater treatment. A key development was the company's work on D-tagatose, including an inexpensive production method patented in 1988 and its use as a naturally occurring low-calorie carbohydrate sweetener and bulking agent. The company advanced D-tagatose commercially as Naturlose and pursued its therapeutic potential, including completion of Phase 3 clinical trials for treatment of type 2 diabetes. Biospherics' early development of radioisotope-based microbial detection methods helped attract initial NASA contracts.

Contributions to space science

Early NASA contracts and research

Gilbert Levin's engagement with NASA began in the late 1950s following his development of radiorespirometry, a highly sensitive technique that used radioactive-labeled nutrients to detect microorganisms by measuring radioactive gas produced during metabolism, capable of detecting as few as ten bacterial cells in about half an hour. Originally applied to public health tasks such as water quality analysis and pathogen identification, the method attracted NASA's interest for potential extraterrestrial applications. In 1958, Levin discussed the possibility of searching for life on Mars with NASA's first administrator, T. Keith Glennan, at a social event, prompting Glennan to direct him to NASA's emerging biology program. By 1959, NASA funded Levin's proposal to adapt radiorespirometry for Mars, resulting in the creation of the Gulliver experiment, which incorporated radioactive carbon-labeled nutrients and a mechanical design to collect and test soil samples for metabolic activity. Under these early contracts, Levin's team developed a working instrument prototype, conducted successful field tests detecting microorganisms in soil, and also pursued related concepts including the Dark Release experiment for photosynthetic organisms and Diogenes for ATP detection using firefly luciferase. Through his firm Biospherics Research Inc., founded in 1967, Levin secured a series of NASA contracts to refine radioisotope-based methods for detecting extraterrestrial life in support of spacecraft missions. These efforts built on his sensitive microbial detection techniques and positioned his work as a prominent component of NASA's early exobiology program. NASA appointed Levin to a committee tasked with recommending experiments for the Biosatellite Mission. He also served on the Planetary Quarantine Advisory Panel from 1967 to 1973, advising on measures to prevent biological contamination of other planets. In 1971, Levin contributed as a team member on the Infrared Interferometer Spectrometer (IRIS) experiment conducted by NASA's Goddard Space Flight Center aboard Mariner 9, which analyzed the atmosphere of Mars. His pre-Viking NASA-funded research and committee roles laid the groundwork for his later selection as Principal Investigator on the Viking program's Labeled Release life-detection experiment.

Role in the Viking Mars program

Gilbert V. Levin served as the principal investigator and experimenter for the Labeled Release (LR) life-detection experiment aboard NASA's Viking 1 and Viking 2 landers, which were designed to search for signs of microbial life on Mars. He was one of three principal investigators selected by NASA for the biology instruments flown on the twin Viking landers. The Viking 1 lander touched down on July 20, 1976, in Chryse Planitia, while Viking 2 landed on September 3, 1976, in Utopia Planitia. The LR experiment functioned by collecting Martian soil samples with the lander's robotic arm and adding a nutrient solution containing carbon-14-labeled organic compounds to the samples. The instrument then monitored the samples for the release of radioactive ^{14}C-labeled gas, which would indicate metabolic activity if living organisms were present. The experiment was conducted at both Viking landing sites.

Labeled Release experiment

Design and implementation

The Labeled Release (LR) experiment was one of three biology instruments aboard each Viking lander, designed to detect metabolic activity through the addition of a carbon-14 labeled nutrient to Martian soil samples and subsequent monitoring of evolved radioactive gas. The LR instrument incorporated a carousel containing four incubation cells, each a 3.5 cc cylindrical test chamber (2 cm diameter) capable of receiving soil from the lander's sample distribution box. After soil delivery, the carousel rotated to seal the cell under a head-end assembly equipped with heaters and a temperature sensor for environmental control and sterilization procedures. Martian soil was collected by the lander's robotic sampling arm, which dredged material to a depth of approximately 4 cm, providing a sample volume of about 0.5 cc for each test. Samples were sometimes stored in the distribution box at around 10°C for periods ranging from hours to many sols before analysis. A 0.115 mL aliquot of aqueous nutrient solution was injected onto the soil, moistening it and establishing a moisture gradient from the injection site at the center to drier conditions at the periphery. The nutrient comprised Miller-Urey-type organic compounds—sodium formate, sodium lactate, glycine, alanine (both L- and D-isomers), and calcium glycolate—each at a concentration of 2.5 × 10^{-4} molar, with all carbon atoms uniformly labeled with ^{14}C at a specific radioactivity of 2 μCi/mL. The test chamber was maintained at 10°C ± 2°C under the Martian atmosphere supplemented by 85 mbar helium overpressure to ensure nutrient liquidity. Radioactive gas evolved from the moistened soil diffused through a 13-inch swan-neck tube, which prevented carryover of aerosol or dust particles, before entering a detector chamber where radioactivity was measured continuously by solid-state beta particle counters. In some runs, a second nutrient injection was performed days later to assess response to additional substrate. Control tests involved heating samples to 160°C for 3 hours (or attempting lower temperatures around 50°C in select cases) prior to nutrient addition to deactivate potential biological activity. The experiment was implemented on both Viking 1 and Viking 2 landers, with Viking 1 conducting four analysis cycles and Viking 2 conducting five, all during 1976. The LR experiments produced positive gas release signals at both landing sites.

Mission results and data

The Labeled Release (LR) experiment aboard NASA's Viking 1 and Viking 2 landers produced positive results at both Martian landing sites in 1976. The initial positive response was returned on July 30, 1976, with a total of four positive results obtained across the two spacecraft, supported by five varied control experiments. These findings came from sites approximately 4,000 miles apart and involved experiments that each ran for 7 days. The LR data showed a rapid release of labeled gas amounting to about 10–15% of the added radioactive counts upon nutrient injection, followed by a very slow continued release over periods of up to several weeks. The rapid evolution of labeled gas was abolished when samples were sterilized at temperatures between 145 °C and 175 °C, and it was reduced by approximately 70% after prior heating at about 45 °C. The response was also lost when samples were stored at spacecraft temperatures. These results were duplicated at both Viking landing sites and were documented in NASA technical reports, as well as in scientific publications including interim findings reported in Science. The positive LR responses formed the basis for Levin's later interpretation of a biological origin.

Claims of life on Mars

Levin's conclusions from 1997 onward

Gilbert Levin has publicly maintained since 1997 that the Viking Labeled Release (LR) experiment detected living microorganisms on Mars. In 2012, he co-authored a paper that applied cluster analysis to the Viking LR data, finding patterns consistent with a biological response rather than chemical reactions. This analysis supported his ongoing interpretation of the original Viking results as evidence of extant life. In a 2019 article published in Scientific American, Levin reiterated his conviction, writing that he is “Convinced We Found Evidence of Life on Mars in the 1970s” based on the LR experiment's positive results from July 30, 1976, including four positive responses supported by five varied controls. He noted that the data curves from Mars resembled those produced by LR tests of terrestrial soils, signaling microbial respiration, with duplication at both Viking landing sites and replication of the experiment. Levin emphasized that no definitive nonbiological explanation has accounted for the results over more than four decades. He has proposed a follow-up experiment called the Chiral LR (CLR), an amended version of the original LR test incorporating the ability to detect chiral metabolism to confirm biological activity and distinguish whether any detected life shares chirality with terrestrial organisms or represents a separate genesis. A small, lightweight Chiral LR has been designed, and its principle has been verified through tests, making it feasible for future Mars missions. These conclusions represent Levin's minority view within the scientific community, grounded in his interpretation of the Viking LR data.

Scientific controversy and mainstream rejection

The mainstream scientific community has largely rejected Gilbert Levin's interpretation of the Labeled Release (LR) experiment results as evidence for extant life on Mars. The general consensus holds that the Viking landers found no conclusive evidence of life, primarily due to the Gas Chromatograph–Mass Spectrometer (GCMS) detecting no trace of organic material in the Martian soil—a finding widely viewed as inconsistent with biological activity. The majority view attributes the LR experiment's positive responses, which resembled metabolic activity, to non-biological chemical processes involving strong oxidants in the regolith. Reactive chemicals such as perchlorates, later confirmed by the Phoenix lander in 2008, provide a plausible abiotic mechanism for the observed release of labeled gas when nutrients were added. These explanations align with the negative outcomes from the other Viking biology experiments and the GCMS data, leading most scientists to conclude that the LR signals were chemical rather than biological in origin. As a result, the claim of life detection via the LR experiment remains a minority position without broad acceptance. Levin's advocacy for a biological interpretation persisted as controversial until his death in 2021.

Later career and advocacy

Academic appointments and proposals

In his later career, Gilbert Levin held academic appointments focused on astrobiology and related fields. He was appointed Adjunct Professor at the Beyond Center for Fundamental Concepts in Science at Arizona State University in 2007. In 2011, he was named Honorary Professor at the Buckingham Centre for Astrobiology at the University of Buckingham. Levin also served as a science adviser to the International Committee Against Mars Sample Return (ICAMSR), an organization advocating caution regarding the potential risks of returning Martian samples to Earth. Levin continued to advocate for follow-up experiments based on his Labeled Release results, proposing improved versions of the LR instrument for future Mars missions that would incorporate controls and additional nutrients to further test for biological activity. These proposals were not accepted or implemented by NASA or other space agencies for any subsequent missions to Mars. Levin's ongoing work in this area emphasized the need for additional in-situ testing to resolve the ambiguity of the Viking results.

Publications, patents, and media appearances

Gilbert Levin published over 150 scientific papers in peer-reviewed journals throughout his career, covering topics in environmental engineering, microbiology, and astrobiology, with a significant focus on his interpretations of the Viking Labeled Release experiment data. He was awarded more than 50 patents, many related to microbial detection methods, wastewater treatment processes, and innovative biotechnological applications. His scientific contributions earned recognition through several prestigious awards, including the NASA Public Service Medal for his role in the Viking program, the AAAS Newcomb-Cleveland Award from the American Association for the Advancement of Science, and the Johns Hopkins Distinguished Alumnus Medal from his alma mater. Levin occasionally appeared in media to discuss his Viking findings and claims regarding evidence of life on Mars. He featured as himself in a 2002 episode of the television series In Search of and in a 2014 episode of NASA's Unexplained Files, where he was credited as a professor and Viking mission scientist.

Personal life and death

Family and personal details

Gilbert V. Levin married Marian "Karen" Bloomquist on October 25, 1953. They were married for over 66 years until her death on December 6, 2019. The couple had three children: sons Ron Levin and Henry Levin, and daughter Carol Sanchez. In his later years, Levin lived in Bethesda, Maryland. He died there on July 26, 2021.

Death and immediate legacy

Gilbert V. Levin died on July 26, 2021, at a hospital in Bethesda, Maryland, at the age of 97. The cause of death was aortic dissection, a tear in the blood vessel leading from the heart. Levin is primarily remembered for designing and interpreting the labeled release (LR) experiment aboard NASA's Viking landers, which he concluded provided evidence of microbial life on Mars—a claim he maintained steadfastly until the end of his life despite strong opposition from most planetary scientists. He continued to advocate for this interpretation in his final years, insisting that the positive results from both Viking landing sites in 1976 had resolved the question of life on the planet. His persistent view remains a minority position in astrobiology, with the scientific consensus attributing the LR experiment's outcomes to non-biological chemical processes rather than biology.

References

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