Ejnar Hertzsprung

Citation metadata

Date: 2006
Publisher: Gale, a Cengage Company
Document Type: Biography
Length: 401 words
Content Level: (Level 4)
Lexile Measure: 1280L

Document controls

Main content

About this Person
Born: October 08, 1873 in Frederiksberg, Denmark
Died: October 21, 1967 in Roskilde, Denmark
Nationality: Danish
Occupation: Astronomer
Updated:Jan. 1, 2006
Full Text: 

Born in Frederiksberg, Denmark on October 8, 1873, Hertzsprung was trained as a chemical engineer, but he was also an amateur astronomer and so impressed Karl Schwarzschild (1877-1916) with his knowledge that Schwarzchild offered him a professorship in Göttingen, Germany in 1909.

Hertzsprung thought there should be a standard by which the brightness of stars could be compared. A given star might be very luminous but appear dim to observers on the earth because of its distance. Likewise, a dim star might appear bright because it is closer. If all stars could be placed at exactly the same distance, their relative luminosity would be readily apparent.

In 1905, Hertzsprung set up a standard that he called the "absolute magnitude" of a star, defining the quantity as what a star's brightness would be at a distance of ten parsecs from the earth (one parsec is equivalent to 3.26 light-years). Once he had determined the intrinsic brightness of a number of stars, it became apparent to him that there was a relationship between a star's color and its luminosity. He found that red stars, generally, are not as bright as blue stars, while yellow stars fall somewhere between the two. Furthermore, since the color of a star is related to its temperature, Hertzsprung concluded that a star's temperature and brightness were correlated. But he published his findings in a journal of photography and timidly kept his diagrams to himself.

Nearly ten years passed before Hertzsprung's important contribution was finally recognized, when American astronomer Henry Norris Russell independently came to the same conclusions. Today the graph depicting the relationship between luminosity and temperature is called the Hertzsprung-Russell diagram. The diagram has played an important role in providing clues to astronomers about stellar evolution.

In 1913 Hertzsprung began another important line of research. With the help of Henrietta Leavitt, he found a method to determine the distances to Cepheid variable stars. Their exploration of this Cepheid "yardstick" led Hertzsprung to make the first credible estimate for the distance of an extragalactic object--the Small Magellanic Cloud. Their method, in turn, was used by Harlow Shapley to determine the size and dimensions of our galaxy, as well as to conclude that spiral nebulas are actually distant galactic systems.

Hertzsprung became director of the observatory at Leiden, Germany in 1935 and retired ten years later. He died in Denmark on October 21, 1967, at the age of 94.

Source Citation

Source Citation   

Gale Document Number: GALE|K1648000307