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Jeffrey L. Bada

Jeffrey L. Bada

American chemist
Jeffrey L. Bada
The basics

Quick Facts

Intro American chemist
Is Chemist
From United States of America
Type Science
Gender male
Birth 10 September 1942, San Diego, San Diego County, California, U.S.A.
Age 78 years
Star sign Virgo
Peoplepill ID jeffrey-l-bada
The details


Jeffrey L. Bada (born September 10, 1942) is an American chemist well known for his works in the study of the origin of life. He is Distinguished Research Professor of Marine Chemistry and former Director of the NASA Specialized Center of Research and Training (NSCORT) in Exobiology at the Scripps Institution of Oceanography, University of California at San Diego. Bada has played a pioneering role in the development of the Mars Organic Detector (MOD) instrument package that is designed to search for amino acids and other organic compounds directly on the surface of Mars during future ESA and NASA missions.

Education and career

Jeffrey Bada studied at the San Diego State University and obtained BS in chemistry in 1965. He wanted to become a theoretical chemist, applying quantum mechanics to chemistry and had no prior interest in prebiotic chemistry. Then he met Stanley Miller at the University of California at San Diego (UCSD) who inspired him to take up the spark discharge experiment a step forward by studying amino acid stability. Bada completed PhD in Chemistry in 1968 under Miller's supervision. He worked as Research Fellow at the Hoffman Labs of the Department of Geological Science at Harvard University for one year. In 1968 he joined the UCSD Department of Chemistry as Instructor, and became Assistant Professor of Marine Chemistry in 1969. He became Associate Professor in 1974 and full professor in 1980. Between 1980 and 2009 he was Director of NASA Specialized Center of Research and Training (NSCORT) in Exobiology. In 2009 he was promoted to Distinguished Professor, and in 2010 to Distinguished Research Professor. He has more than 200 technical publications.

Professional achievements


As a marine geochemist, Jeffrey Bada made significant research in geochronology. During the 1970s and 1980s he developed an important technique of marine sediment dating through the measurement of the racemisation rates of amino acids. This method is useful for dating a large span in geological time scale. This is useful in marine biology, palaeontology and archaeology for dating millions of years old organic materials based on their amino acid content.


Jeffrey Bada is a leading scientist in the study of organic compounds outside of the Earth. Among the most interesting works was his analysis of the Martian meteorite Nakhla, which fell in Egypt in 1911. His team found aspartic acid, glutamic acids, glycine, alanine, beta-alanine, and gamma-aminobutyric acid as the most abundant amino acids in the meteorite. This a supports the notion that the organic building blocks of life could be naturally synthesized and were present in the making of the solar system. He and his team also developed a Mars Organic Analyzer (MOA), which is a microfabricated capillary electrophoresis (CE) instrument for sensitive amino acid biomarker analysis. The device is useful in planetary exploration such as for the analysis of even trace amounts of amino acids, mono- and diaminoalkanes, amino sugars, nucleobases, and nucleobase degradation products from living and non-living materials.

Prebiotic chemistry

Jeffrey Bada is most familiar with his research on the origin of life, following his mentor Miller, whose laboratory he inherited. In fact his most famous works, perhaps, are his reassessment and validation of the original Miller's experiments. In 1999, Miller had a stroke and on thinking of his medical condition, he donated everything in his office to Bada's laboratory. Just before Miller's death in 2007, several cardboard boxes containing vials of dried residues were found in his laboratory at UCSD. The labels indicated that some were from Miller's original 1952–1954 experiments, produced by using three different apparatuses, and one from 1958, which included H2S in the gaseous mixture for the first time and the result never published. In 2008 Bada and his team reported a re-analysis of the 1952 samples using more sensitive techniques, such as high-performance liquid chromatography and liquid chromatography–time of flight mass spectrometry. Their result showed the synthesis of 22 amino acids and 5 amines, revealing that the original Miller experiment produced much more compounds than actually known. Miller's report of 1953 mentioned synthesis of only glycine, α- and β-alanine, with uncertain aspartic acid and GABA. In addition Bada also analysed the unreported 1958 samples in 2011, from which 23 amino acids and 4 amines, including 7 organosulfur compounds, were detected.

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