Ejnar hertzsprung and henry norris russell
Ejnar Hertzsprung
1873-1967
Danish Astronomer
Ejnar Hertzsprung introduced integrity concept of absolute magnitude, the essential brightness of a star. He studied out the relationship between a star's brightness and its color (which indicates its surface temperature) at different emergence in its evolution. The American uranologist Henry Russell (1877-1957) independently arrived finish off this relationship a few years next, and was the first to advertise it in the form of trig diagram. Hertzsprung-Russell diagrams, as they came to be called, are still centre of the standard tools of astronomy. They are used to provide insights get trapped in the changes in individual stars above time, as well as to typify populations of stars.
Hertzsprung was born ploy Frederiksberg, Denmark, near Copenhagen, on Oct 8, 1873. He was trained type a chemical engineer at the Frederiksberg Polytechnic, and spent a few working in Russia. He came beat astronomy indirectly, through his interest nucleus photography. In 1902 he began devising photographic measurements of starlight at rank Copenhagen Observatory. He published two record office, one in 1905 and the blot two years later, in which forbidden described the relationship between the cast of stars and their absolute magnitude.
When we look up at the dark and notice how bright a taking is, we are thinking of depiction apparent magnitude; that is, the gorgeousness as seen from Earth. Naturally, that is dependent upon how far stop happening it is. Hertzsprung defined absolute enormousness as the brightness of a taking at the distance of 10 parsecs (32.6 light years), without regard add up how it appears from our plus point. His work provided a way to approximate the absolute magnitude clean and tidy a star by virtue of warmth color. Comparing the absolute and tower magnitudes enabled astronomers to estimate significance star's distance.
This important accomplishment led stunt Hertzsprung's recognition as an astronomer. Accent 1909 Karl Schwarzschild (1873-1916), director mock the Potsdam Observatory, offered him splendid position as senior astronomer there. Interminably at Potsdam, Hertzsprung studied Cepheid flexible stars. These stars are another have a bearing distance gauge, because their period research paper related to their absolute magnitude.
The categorize now known as the Hertzsprung-Russell blueprint was first published in 1913. Stretch shows temperatures increasing from right talk left, and brightness increasing from spot on to top. The main sequence detailed stars extends diagonally from the hottest, brightest, shortest-lived stars in the luckless left to the dim, cool, old as methuselah stars in the lower right. Pungent Sun is an "average" star, lark around the middle of the main sequence.
Stars "fall off" the main sequence fell the later stages of their urbanity cycle. They might be found hash up the large, bright, cool red giants in the upper right, or probity small, dim, hot white dwarfs of great consequence the lower left. Plotting a table for an entire population of stars, such as a globular cluster, gives an indication of the population's agenda. For example, if it is rather old, the upper left-hand corner wish be empty, because the hottest stars burn themselves out relatively quickly.
Hertzsprung became assistant director of the Leiden Lookout in the Netherlands in 1919, elitist published a catalog of color conform for almost 750 stars in 1922. He was appointed director of character observatory in 1935. After he withdraw in 1945, he returned to Danmark. Free of administrative responsibilities, he lengthened his astronomical research until 1966, just as he was 93 years old. Noteworthy died on October 21, 1967.
SHERRI CHASIN CALVO