Biography:William Coblentz

Short description: American physicist

William Coblentz
William Coblentz in 1922
Born	November 20, 1873 North Lima, Ohio, U.S.
Died	September 15, 1962 (1962-09-16) (aged 88) Washington, D.C., U.S.
Alma mater	Cornell University Case Western Reserve
Known for	Infrared radiometry and spectroscopy
Spouse(s)	Catherine Cate Coblentz (m. 1924; died 1951)
Awards	Howard N. Potts Medal 1911 Physics Janssen Medal 1920 Work on infrared rays Rumford Prize 1937 Improving measurement Frederic Ives Medal 1945 Optics
Scientific career
Fields	Physics
Institutions	National Bureau of Standards

William Weber Coblentz (November 20, 1873 – September 15, 1962) was an American physicist notable for his contributions to infrared radiometry and spectroscopy.

Early life, education, and employment

William Coblentz was born in North Lima, Ohio to parents of German and Swiss descent. His mother (Catherine) died when Coblentz was just under three, leaving him temporarily with a family of just his younger brother (Oscar) and their father (David). However, the father remarried about 2 years later, and Coblentz appears to have admired his second mother (Amelia). Throughout Coblentz's childhood and adolescence, his family lived on farms, but apparently were never able to buy one of their own. The family's extremely modest circumstances led to a somewhat-delayed education for Coblentz, who did not finish high school (Youngstown, Ohio) until 1896, when he was 22 years old.

Coblentz entered the Case School of Applied Science, now Case Western Reserve University in the fall of 1896, and received his Bachelor of Science degree in physics in June, 1900. He went on to earn MS (1901) and PhD (1903) degrees from Cornell University in Ithaca, New York, staying two years beyond his doctoral time by working as a Research Fellow with support from the Carnegie Institution. In the spring of 1905, Coblentz accepted a position with the newly founded National Bureau of Standards (now the National Institute of Standards and Technology, NIST) in Washington, DC, where he spent his entire career. In 1905 he founded the Bureau's radiometry section, and headed it for 40 years until his retirement in 1945.

Scientific work

Coblentz at the 1910 Fourth Conference International Union for Cooperation in Solar Research at Mount Wilson Observatory

During the course of a long and productive career, Coblentz made many scientific contributions both of a pure and applied nature. Bibliographies of his work show that he had hundreds of scientific publications, talks, and abstracts to his credit. He received a total of ten patents during his lifetime, the first being US Patent 1,077,219 for a solar cell invention to convert sunlight to electricity.

Coblentz's first publication, "Some Optical Properties of Iodine", was based on his PhD research. On acquiring his doctorate, he soon began publishing regularly on problems related to infrared (IR) radiation, both those concerning spectroscopy and those concerning radiometry. For example, Coblentz was among the first, if not the very first, to verify Planck's Law.

Infrared studies

Spectrometer used at Cornell University by W. W. Coblentz

When Coblentz entered Cornell University, infrared spectroscopy was in what today would be considered an extremely primitive state. As a young Cornell researcher, Coblentz assembled and calibrated his own IR equipment, and extended the range of IR measurements to longer wavelengths than had ever been reached. By 1905 he had acquired hundreds of spectra by tedious point-by-point measurements with a prism instrument of his own construction. These were published in 1905 with large fold-outs charts (not available in the later reprints), and tables of wavelengths at which various materials absorbed IR light. While such a massive spectral compilation itself was something of a tour de force, it is perhaps not the most important part of Coblentz's 1905 book. Instead, that honor probably goes to his generalization that certain molecular groupings, or functional groups in modern parlance, appeared to absorb specific and characteristic IR wavelengths. In time this would allow scientists to use a molecule's IR spectrum as a type of molecular fingerprint. This generalization had been hinted at in earlier work by others, but not with such a large amount of supporting data as Coblentz presented. Today, IR spectra are used in thousands of laboratories around the globe by scientists in many fields.

As an aside, Coblentz's early work on molecular spectra was not given the eager reception that hindsight might suggest. The reasons are numerous and have been explored by several authors.

Astronomical studies

Coblentz had a long interest in astronomical problems. In 1913, he developed thermopile detectors and used them at Lick Observatory to measure IR radiation from 110 stars, and the planets Mars, Venus, and Jupiter. In this work he was assisted by Seth Nicholson, later of the Mt. Wilson Observatory. Extending this work, Coblentz and Carl Lampland, of the Lowell Observatory, measured large differences between the day and night temperatures on Mars, which implied a thin Martian atmosphere.

For his applications of IR detectors to astronomy, Coblentz is regarded as the founder of astronomical infrared spectroscopy. In recognition of his astronomical contributions, craters on the moon and Mars were named after him by the International Astronomical Union.

Coblentz also made observations of solar eclipses, and published papers describing his work.

Other research

An inspection of Coblentz's bibliography shows that from about 1930 his research turned more toward measurements involving the ultraviolet (UV) region and away from infrared work. Much of this research had a distinctly bio-medical slant, such as his investigations of ultraviolet therapy (1938) and the production of skin cancer by UV exposure (1948).

Although Coblentz is remembered today mainly for his contributions to physics and astronomy, he also had interests in bioluminescence, atmospheric ozone, and, perhaps surprisingly, parapsychology. He appears to have brought the same energy to the latter field as he did to his other areas of interest.

Honors

Coblentz was elected a member of the National Academy of Sciences in 1930.

Among the awards Coblentz received were the 1911 Howard N. Potts Medal from the Franklin Institute, the 1920 Janssen Medal from the French Academy of Sciences, and the 1937 Rumford Prize from the American Academy of Arts and Sciences. In 1945, shortly after retiring, Coblentz received the Frederic Ives Medal from the Optical Society of America.

The Coblentz Society, dedicated to the understanding and application of vibrational spectroscopy, is named in his honor, as is the Coblentz Medal. Coblentz was given membership card number 1 from the Society. Coblentz died just before his 1905 work on infrared spectroscopy was reprinted, nearly 60 years after its first publication.

Family and personal life

Marker for the Coblentz family

In his autobiography, From the Life of a Researcher (1951), William Coblentz described his typical day as long hours of laboratory research followed by evenings spent on data analysis and writing papers. This left little time for socializing, and so it is not unexpected that Coblentz was over 50 before ever marrying. He wed Catherine Emma Cate of Vermont on June 10, 1924, and it is said that they spent their honeymoon in Flagstaff, Arizona while Coblentz was at the Lowell Observatory measuring planetary temperatures. Catherine Cate Coblentz achieved success as a writer of children's book, worked for a time at the National Bureau of Standards, and was instrumental in raising money to build the Cleveland Park Neighborhood Library in Washington, DC.

William Coblentz reportedly was plagued by periods of poor health, but he lived nearly 90 years. He is buried in Rock Creek Cemetery in Washington, DC alongside his wife and an infant daughter.

Further reading

• A Physical Study of the Firefly, by William W. Coblentz, 1912
• Man's Place in a Superphysical World, by William W. Coblentz, 1955 (concerning parapsychology)
• Journal of the Optical Society of America, 1936, volume 36, number 2, pp. 61 – 71 (The presentation ceremony, and Coblentz's accompanying lecture, for the Ives Medal, along with a list of Coblentz's scientific publications.)
• Applied Optics (November, 1963), commemorative issue with extensive material on Coblentz's scientific work
• Coblentz, W. W. "Present Status of the Determination of the Constant of Total Radiation from a Black Body," Bulletin of the Bureau of Standards 12 (553-582) 1916.

Copies of most of Coblentz's books are listed as being in the libraries of the University of Maryland and the American Institute of Physics, both in College Park, Maryland (USA), not far from where Coblentz lived, worked, and died.

External links

• The Coblentz Society
• National Academy of Sciences Biographical Memoir