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Russell, Henry Norris

The Danish astronomer Ejnar Hertzsprung and the American astronomer Henry Norris Russell independently observed a very well defined correlation between the luminosity and surface temperature of stars. That correlation is shown in Figure 12.7 and is called a Hertzsprung-Russell, or H-R, diagram. Most stars, such as our sun, fall in a narrow band on this diagram called the main sequence. Stars in this main sequence have luminosities L that are approximately proportional to 7 s5u3face, or in terms of their mass, M, L °c M3 5. How long a star stays on the main sequence will depend on its mass, which, in ton, is related to the reaction rates in its interior. [Pg.340]

In 1977 she received the prestigious Henry Norris Russell Prize from the American Astronomical Society. In her acceptance speech, she discussed her excitement for science ... [Pg.55]

Henry Norris Russell (1877-1957). Frederick Albert Saunders (1875-1963). [Pg.193]


See other pages where Russell, Henry Norris is mentioned: [Pg.106]    [Pg.177]    [Pg.8]    [Pg.322]    [Pg.320]    [Pg.201]    [Pg.52]    [Pg.723]    [Pg.194]    [Pg.7]   
See also in sourсe #XX -- [ Pg.106 ]

See also in sourсe #XX -- [ Pg.177 ]

See also in sourсe #XX -- [ Pg.320 ]




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Russell, Henry

Russell, Henry Norri

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