Emden was born in St. Gallen, Switzerland, the eldest of three children. He studied mathematics and physics in Heidelberg and Berlin and completed his BS Physics in 1885, and his PhD in Physics in 1887 at the University of Strasbourg, France. His thesis was on the vapour pressure of salt solutions. He was appointed professor of physics at the Technical University of Munich in 1889. He became associate professor of physics and meteorology at the Technical University of Munich and in 1907 published the classical work Gaskugeln: Anwendungen der mechanischen Wärmetheorie auf kosmologische und meteorologische probleme. Emden was a member of the Bayerische Akademie der Wissenschaften from 1920 to 1933. In 1924 he became honorary professor of astrophysics at the University of Munich. In 1930 Emden assisted in the founding of Zeitschrift fur Astrophysik and served as the editor for six years. On 10 June 1932 he became an Associate of the Royal Astronomical Society. He retired in 1934.
Influence in physics and meteorology
Most of Emden's work related to thermodynamics applied to natural phenomena, while his published papers focused on geophysics and astrophysics. Emden's book Gaskugeln: Anwendungen der mechanischen Wärmetheorie auf kosmologische und meteorologische probleme presented a mathematical model to explain the expansion and compression of gas spheres. The book also includes a short section on Karl Schwarzschild's theory ofconvective equilibrium. Emden's work, in conjunction with Subrahmanyan Chandrasekhar, was named the Emden–Chandrasekhar equation. In a major advance over previous work, by introducing polytropic solutions, modelling of a much broader range of stellar objects was possible. His theories also suggested that stars have a boundary at a finite radius. This work, in conjunction with Jonathan Homer Lane, became known as the Lane-Emden equation. The Lane-Emden equation can be described as "a second-order ordinary differential equation that applies to polytropic profiles in density". The Lane-Emden equations were later studied by Ralph H. Fowler who developed a new set of solutions for different values of n and for all types of boundary conditions. These became known as Emden-Fowler-type differential equations. Emden's convective stellar models have been supplanted by radiative theory. Robert Emden also offered an hypothesis, which has since been discredited, to explain sunspots. The crater Emden on the Moon is named after him.
Personal life
Robert Emden married Klara Schwarzschild, the sister of German physicist and astronomer Karl Schwarzschild and the uncle of the German-American astrophysicist Martin Schwarzschild. They had six children of whom the names of five are known: Charlotte Schein; Emma Müller; Antonia Flach; Karl Emden, and Johanna Luise Berchtold-Emden. Although he married into a strongly scientific family, Robert Emden's children are not noted for any contributions to science. Emden was an avid balloonist and wrote a book on the principles of balloon navigation in 1910. He always had a practical attitude towards physics, as shown by his 1938 letter to Nature entitled "Why do we have winter heating?" Although he had retired in 1934, Jacob Robert Emden continued his scientific activities until he died in Zürich on 8 October 1940. His final paper on the temperature problems of lakes was in the press at the time of his death.
