Hertzsprung (right) andKarl Schwarzschild in front of the Göttingen Observatory building (1909)
Hertzsprung was born inFrederiksberg, Denmark, the son of Severin and Henriette. He studied chemical engineering atCopenhagen Polytechnic Institute, graduating in 1898. After spending two years working as a chemist in St. Petersburg, in 1901 he studiedphotochemistry atLeipzig University for a year.[1] His father was an amateur astronomer, which led to Ejnar's interest in the subject. He began making astronomical observations in Frederiksberg in 1902, and within a few years had noticed that stars with similarspectral type could have widely differentabsolute magnitudes. In 1909, he took a position at theGöttingen Observatory under directorKarl Schwarzschild.[2]
In 1913 Hertzsprung determined the distances to severalCepheid variable stars byparallax,[3] and was thus able to calibrate the relationship, discovered byHenrietta Leavitt, between Cepheid period andluminosity. In this determination he made a mistake, possibly a slip of the pen, putting the stars 10 times too close. He used this relationship to estimate the distance to theSmall Magellanic Cloud. From 1919 to 1946, Hertzsprung worked atLeiden Observatory in the Netherlands, from 1937 as director. Among his graduate students at Leiden wasGerard Kuiper.
Perhaps his greatest contribution to astronomy was the development of a classification system for stars to divide them by spectral type, stage in their development, and luminosity. He used the earlier classification system developed byAntonia Maury in his work.[4] The so-called "Hertzsprung–Russell Diagram" has been used ever since as a classification system to explain stellar types andstellar evolution. He also discovered twoasteroids, one of which is1627 Ivar, anAmor asteroid.[5]
His wife Henrietta (1881–1956) was a daughter of the Dutch astronomerJacobus Kapteyn. Hertzsprung died inRoskilde in 1967. The asteroid1693 Hertzsprung was named in his honour.[6]
^Hellyer, B. (October 1973). "Ejnar Hertzsprung, 1873–1967".Journal of the British Astronomical Association.83:460–461.Bibcode:1973JBAA...83..460H.
^Hertzsprung, E. (1913). "Über die räumliche Verteilung der Veränderlichen vom δ Cephei-Typus" [On the spatial distribution of variable [stars] of the δ Cephei type].Astronomische Nachrichten (in German).196 (4692):201–208.Bibcode:1913AN....196..201H.
^Hoffleit, Dorritt (1994). "Reminiscences on Antonia Maury and the c-Characteristic.". In Corbally, Christopher J.; Gray, Richard O.; Garrison, Robert F. (eds.).The MK Process at 50 Years. San Francisco: Astronomical Society of the Pacific. pp. 215–223.ISBN0-937707-79-1.