Timeline (nonfiction): Difference between revisions

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File:George Gabriel Stokes.jpg|link=Sir George Stokes, 1st Baronet (nonfiction)|1903 Feb. 1:  Physicist and mathematician [[Sir George Stokes, 1st Baronet (nonfiction)|Sir George Stokes, 1st Baronet]] dies. He made seminal contributions to fluid dynamics (including the Navier–Stokes equations) and to physical optics.  
File:George Gabriel Stokes.jpg|link=Sir George Stokes, 1st Baronet (nonfiction)|1903 Feb. 1:  Physicist and mathematician [[Sir George Stokes, 1st Baronet (nonfiction)|Sir George Stokes, 1st Baronet]] dies. He made seminal contributions to fluid dynamics (including the Navier–Stokes equations) and to physical optics.  
File:J. Robert Oppenheimer.jpg|link=J. Robert Oppenheimer (nonfiction)|1904 Apr. 22: American physicist and academic [[J. Robert Oppenheimer (nonfiction)|J. Robert Oppenheimer]] born. His achievements in physics will include the Born–Oppenheimer approximation for molecular wavefunctions, work on the theory of electrons and positrons, the Oppenheimer–Phillips process in nuclear fusion, and the first prediction of quantum tunneling.
File:J. Robert Oppenheimer.jpg|link=J. Robert Oppenheimer (nonfiction)|1904 Apr. 22: American physicist and academic [[J. Robert Oppenheimer (nonfiction)|J. Robert Oppenheimer]] born. His achievements in physics will include the Born–Oppenheimer approximation for molecular wavefunctions, work on the theory of electrons and positrons, the Oppenheimer–Phillips process in nuclear fusion, and the first prediction of quantum tunneling.
File:Heike Kamerlingh Onnes.jpg|link=Heike Kamerlingh Onnes (nonfiction)|1911 Apr. 8: Physicist [[Heike Kamerlingh Onnes (nonfiction)|Heike Kamerlingh Onnes]] discovers superconductivity.
File:Gustav Hahn - 1913 Great Meteor Procession.jpg|link=1913 Great Meteor Procession (nonfiction)|1913: A [[1913 Great Meteor Procession (nonfiction)|group of meteors is visible across much of the eastern seaboard of North and South America]], leading astronomers to conclude the source had been a small, short-lived natural satellite of the Earth.
File:Gustav Hahn - 1913 Great Meteor Procession.jpg|link=1913 Great Meteor Procession (nonfiction)|1913: A [[1913 Great Meteor Procession (nonfiction)|group of meteors is visible across much of the eastern seaboard of North and South America]], leading astronomers to conclude the source had been a small, short-lived natural satellite of the Earth.
File:Heike Kamerlingh Onnes.jpg|link=Heike Kamerlingh Onnes (nonfiction)|1926 Feb. 21: Physicist and academic [[Heike Kamerlingh Onnes (nonfiction)|Heike Kamerlingh Onnes]] dies. He received widespread recognition for his work, including the 1913 Nobel Prize in Physics for (in the words of the committee) "his investigations on the properties of matter at low temperatures which led, ''inter alia'', to the production of liquid helium".
File:Heike Kamerlingh Onnes.jpg|link=Heike Kamerlingh Onnes (nonfiction)|1926 Feb. 21: Physicist and academic [[Heike Kamerlingh Onnes (nonfiction)|Heike Kamerlingh Onnes]] dies. He received widespread recognition for his work, including the 1913 Nobel Prize in Physics for (in the words of the committee) "his investigations on the properties of matter at low temperatures which led, ''inter alia'', to the production of liquid helium".

Revision as of 17:58, 4 February 2017