Template:Short description {{#invoke:Other people|otherPeople}} Template:Infobox scientist Walter Sydney Adams (December 20, 1876 – May 11, 1956) was an American astronomer.<ref name="frs"/><ref name="nas">Template:Biographical Memoirs</ref><ref name="obitmnras">MNRAS 117 (1957) 243</ref><ref name="obitobs">Obs 76 (1956) 139</ref><ref name="obitpaps">PASP 68 (1956) 285</ref><ref>Template:Cite encyclopedia</ref> He is renowned for his pioneering work in spectroscopy.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

Life and workEdit

Adams was born in Antioch, Ottoman Empire, to Lucien Harper Adams and Nancy Dorrance Francis Adams, missionary parents,<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> and was brought to the U.S. in 1885<ref name="frs"/> He graduated from Dartmouth College in 1898, then continued his education in Chicago and in Germany. After returning to the U.S., he began a career in Astronomy that culminated when he became director of the Mount Wilson Observatory.

His primary interest was the study of stellar spectra. He worked on solar spectroscopy and co-discovered a relationship between the relative intensities of certain spectral lines and the absolute magnitude of a star. He was able to demonstrate that spectra could be used to determine whether a star was a giant or a dwarf. In 1915 he began a study of the companion of Sirius and found that despite a size only slightly larger than the Earth, the surface of the star was brighter per unit area than the Sun and it was about as massive.<ref name="sirius">F. Wesemael, A comment on Adams's measurement of the gravitational redshift of Sirius B Royal Astronomical Society, Quarterly Journal ({{#if:0035-8738|Template:Catalog lookup link{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}{{#if:Template:Trim|{{#ifeq:Template:Yesno-no|yes|Template:Main other|{{#invoke:check isxn|check_issn|Template:Trim|error=Template:Error-smallTemplate:Main other}}}}}}}}}}}}}}}}}}}}}}|Template:Error-small}}), 26, Sept. 1985, 273-278</ref> Such a star later came to be known as a white dwarf. In 1925, he reported a gravitational redshift caused by Sirius B; this was regarded as significant confirmation of Albert Einstein's theory of General Relativity. It is now known that his reported measurements were incorrect. Along with Theodore Dunham, he discovered the strong presence of carbon dioxide in the infrared spectrum of Venus.

Adams died at the age of 79 in Pasadena, California.

Awards and honorsEdit

Awards and honors

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Named after him

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ReferencesEdit

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Further readingEdit

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