Johann Jakob Balmer

Johann Jakob Balmer (1 May 1825 – 12 March 1898) was a Swiss mathematician best known for his work in physics, the Balmer series of Hydrogen atom.

Johann Jakob Balmer
Born	1 May 1825 Lausen, Switzerland
Died	12 March 1898(1898-03-12) (aged 72) Basel, Switzerland
Nationality	Swiss
Alma mater	University of Basel
Scientific career
Fields	Mathematics

Biography

Balmer was born in Lausen, Switzerland, the son of a chief justice also named Johann Jakob Balmer. His mother was Elizabeth Rolle Balmer, and he was the oldest son. During his schooling he excelled in mathematics, and so decided to focus on that field when he attended university.

He studied at the University of Karlsruhe and the University of Berlin, then completed his Ph.D. from the University of Basel in 1849 with a dissertation on the cycloid. Johann then spent his entire life in Basel, where he taught at a school for girls. He also lectured at the University of Basel. In 1868 he married Christine Pauline Rinck at the age of 43. The couple had six children.

Despite being a mathematician, Balmer is best remembered for his work on spectral series. His major contribution (made at the age of sixty, in 1885) was an empirical formula for the visible spectral lines of the hydrogen atom, the study of which he took up at the suggestion of Eduard Hagenbach also of Basel.[1][2] Using Ångström's measurements of the hydrogen lines, he arrived at a formula for computing the wavelength as follows:

${\displaystyle \lambda \ =h\,{\frac {m^{2}}{m^{2}-n^{2}}}}$

for n = 2 and m = 3, 4, 5, 6, and so forth; h = 3.6456×10⁻⁷ m.[n and m need to be defined]

In his 1885 notice, he referred to h (now known as the Balmer constant) as the "fundamental number of hydrogen." Balmer then used this formula to predict the wavelength for m = 7 and Hagenbach informed him that Ångström had observed a line with wavelength 397 nm. Two of his colleagues, Hermann Wilhelm Vogel and William Huggins, were able to confirm the existence of other lines of the series in the spectrum of hydrogen in white stars.

Balmer's formula was later found to be a special case of the Rydberg formula, devised by Johannes Rydberg in 1888.

${\displaystyle {\frac {1}{\lambda }}\ ={\frac {4}{h}}\left({\frac {1}{n_{1}^{2}}}-{\frac {1}{n_{2}^{2}}}\right)=R_{H}\left({\frac {1}{n_{1}^{2}}}-{\frac {1}{n_{2}^{2}}}\right)}$

with ${\displaystyle R_{H}}$ being the Rydberg constant for hydrogen, ${\displaystyle n_{1}=2}$ for Balmer's formula, and ${\displaystyle n_{2}>n_{1}}$.

A full explanation of why these formulas worked, however, had to wait until the presentation of the Bohr model of the atom by Niels Bohr in 1913.

Johann Balmer died in Basel. He was 72 when he died.

Honors

• Balmer formula and Balmer constant h are named after him, as well as Balmer lines and Balmer series.
• The Balmer jump is useful in Astronomy for stellar classification.
• The crater Balmer on the Moon is named after him.
• Minor planet 12755 Balmer is named after him.[3]

References

1. Balmer, J. J. (1885). "Notiz über die Spectrallinien des Wasserstoffs" [Note on the spectral lines of hydrogen]. Annalen der Physik und Chemie. 3rd series (in German). 25: 80–87.
2. Magie, William Francis (1969). A Source Book in Physics. Cambridge, Massachusetts: Harvard University Press. p. 360
3. "12755 Balmer". JPL.

External links

• O'Connor, John J.; Robertson, Edmund F., "Johann Jakob Balmer", MacTutor History of Mathematics archive, University of St Andrews.