Svante August Arrhenius (19 February 1859 – 2
October 1927) was a Swedish
scientist,
originally a
physicist, but often referred
to as a
chemist, and one of the founders of
the science of
physical
chemistry.
The Arrhenius
equation, lunar crater Arrhenius
and the Arrhenius Labs at Stockholm
University
are named after him.
Biography
Early years
Arrhenius
was born on February 19, 1859 at Vik (also spelled Wik or Wijk),
near Uppsala
, Sweden, the
son of Svante Gustav and Carolina Thunberg Arrhenius.
His father
had been a land surveyor for Uppsala
University
, moving up to a supervisory position. At the
age of three, Arrhenius taught himself to read without the
encouragement of his parents, and by watching his father's addition
of numbers in his account books, became an
arithmetical prodigy.
In later life, Arrhenius enjoyed using masses of data to discover
mathematical relationships and laws. At age 8, he entered the local
cathedral school, starting in the
fifth
grade, distinguishing himself in
physics
and
mathematics, and graduating as the
youngest and most able student in 1876.
At the
University of Uppsala, he was unsatisfied with the chief instructor
of physics and the only faculty member who could have supervised
him in chemistry, Per Teodor Cleve,
so he left to study at the Physical Institute of the Swedish
Academy of Sciences in Stockholm
under the physicist Erik
Edlund in 1881. His work focused on the
conductivities of
electrolytes. In 1884, based on this work, he
submitted a 150-page dissertation on electrolytic conductivity to
Uppsala for the
doctorate. It
did not impress the professors, like
Per Teodor Cleve, and he received a fourth
class degree, but upon his defence it was reclassified as third
class. Later, extensions of this very work would earn him the
Nobel Prize in
Chemistry.
There were 56 theses put forth in the 1884 dissertation, and most
would still be accepted today unchanged or with minor
modifications.The most important idea in the dissertation was his
explanation of the fact that neither pure
salts
nor pure
water is a
conductor, but solutions of salts in
water are.
Arrhenius' explanation was that in forming a solution, the salt
dissociates into charged particles (which
Michael Faraday had given the name
ions many years earlier). Faraday's belief had been that
ions were produced in the process of
electrolysis; Arrhenius proposed that, even in
the absence of an electric current, solutions of salts contained
ions.He thus proposed that chemical reactions in solution were
reactions between ions. For weak electrolytes this is still
believed to be the case, but modifications (by
Peter J. W. Debye and
Erich
Hückel) were found necessary to account for the behavior of
strong electrolytes.
The dissertation was not very impressive to the professors at
Uppsala, but Arrhenius sent it to a number of scientists in Europe
who were developing the new science of
physical chemistry, such as
Rudolf Clausius,
Wilhelm Ostwald, and
J. H. van 't
Hoff.They were far more impressed, and Ostwald even came to
Uppsala to persuade Arrhenius to join his research team. Arrhenius
declined, however, as he preferred to stay in Sweden for a while
(his father was very ill and would die in 1885) and had received an
appointment at Uppsala.
Middle period
Arrhenius
next received a travel grant from the Swedish Academy of Sciences,
which enabled him to study with Ostwald in Riga
(now in
Latvia
), with Friedrich
Kohlrausch in Würzburg
, Germany,
with Ludwig Boltzmann in Graz, Austria
, and with van 't Hoff in Amsterdam
.
In 1889 Arrhenius explained the fact that most reactions require
added heat energy to proceed by formulating the concept of
activation energy, an energy barrier that
must be overcome before two molecules will react.The
Arrhenius equation gives the quantitative
basis of the relationship between the activation energy and the
rate at which a reaction proceeds.
In 1891 he
became a lecturer at the Stockholm University College
(Stockholms Högskola, now Stockholm University
), being promoted to professor of physics (with much
opposition) in 1895, and rector in
1896.
He was married twice, to Sofia Rudbeck (his former pupil), who bore
him one son, although the marriage only lasted two years from 1894
to 1896, and to Maria Johansson (who bore him two daughters and a
son), from 1905 until his death.
About 1900, Arrehenius became involved in setting up the Nobel
Institutes and the
Nobel Prizes. He was
elected a member of the
Royal Swedish Academy of
Sciences in 1901. For the rest of his life, he would be a
member of the
Nobel Committee on
Physics and a de facto member of the Nobel Committee on Chemistry.
He used his positions to arrange prizes for his friends (
Jacobus van't Hoff,
Wilhelm Ostwald,
Theodore Richards) and to attempt to deny
them to his enemies (
Paul Ehrlich,
Walther Nernst). In 1901 Arrhenius
was elected to the Swedish Academy of Sciences, against strong
opposition. In 1903 he became the first Swede to be awarded the
Nobel Prize in chemistry.In
1905, upon the founding of the Nobel Institute for Physical
Research at Stockholm, he was appointed
rector of the institute, the position where he
remained until retirement in 1927. He became a Fellow of the Royal
Society in 1910.
Later years
Eventually, Arrhenius' theories became generally accepted and he
turned to other scientific topics. In 1902 he began to investigate
physiological problems in terms of
chemical theory. He determined that reactions in living organisms
and in the test tube followed the same laws. In 1904 he delivered
at the
University of
California a course of lectures, the object of which was to
illustrate the application of the methods of physical chemistry to
the study of the theory of
toxins and
antitoxins, and which were published in
1907 under the title
Immunochemistry.He also turned his
attention to
geology (the origin of
ice ages),
astronomy,
physical cosmology, and
astrophysics, accounting for the birth of the
solar system by interstellar
collision.He considered
radiation
pressure as accounting for
comets, the
solar
corona, the
aurora borealis, and
zodiacal light.
He thought life might have been carried from planet to planet by
the transport of
spores, the theory now known
as
panspermia. He thought of the idea of
a
universal language, proposing a
modification of the
English
language.
In an extension of his
ionic theory Arrhenius
proposed definitions for
acids and
bases, in 1884. He believed that acids were substances
which produce
hydrogen ions in
solution and that bases
were substances which produce hydroxide ions in solution.
In his last years he wrote both textbooks and popular books, trying
to emphasize the need for further work on the topics he
discussed.
In September, 1927, he came down with an attack of acute
intestinal catarrh, died on
2 October, and was buried in Uppsala.
Greenhouse effect
Arrhenius developed a theory to explain the
ice
ages, and first speculated that changes in the levels of carbon
dioxide in the atmosphere could substantially alter the surface
temperature through the
greenhouse
effect. He was influenced by the work of others, including
Joseph Fourier.
Arrhenius used the
infrared observations of the moon by Frank Washington Very and Samuel Pierpont Langley at the
Allegheny
Observatory
in Pittsburgh to calculate the absorption of
CO2 and water vapour. Using 'Stefan's law'
(better known as the
Stefan
Boltzmann law), he formulated his greenhouse law.In its
original form, Arrhenius' greenhouse law reads as follows:
- :if the quantity of carbonic acid increases in geometric
progression, the augmentation of the temperature will increase
nearly in arithmetic progression.
This simplified expression is still used today:
- :ΔF = α ln(C/C_0)
Arrhenius' high absorption values for CO
2, however, met
criticism by
Knut Ångström
in 1900, who published the first modern infrared spectrum of
CO
2 with two absorption bands. Arrhenius replied
strongly in 1901 (
Annalen der Physik), dismissing the
critique altogether. He touched the subject briefly in a technical
book titled
Lehrbuch der kosmischen Physik (1903). He
later wrote
Världarnas utveckling (1906), German
translation:
Das Werden der Welten (1907), English
translation:
Worlds in the Making (1908) directed at a
general audience, where he suggested that the human emission of
CO
2 would be strong enough to prevent the world from
entering a new ice age, and that a warmer earth would be needed to
feed the rapidly increasing population. He was the first person to
predict that emissions of carbon dioxide from the burning of fossil
fuels and other combustion processes would cause global warming.
Arrhenius clearly believed that a warmer world would be a positive
change. From that, the hot-house theory gained more attention.
Nevertheless, until about 1960, most
scientists dismissed the hot-house / greenhouse effect as
implausible for the cause of ice ages as Milutin
Milankovitch
had presented a mechanism using orbital changes of
the earth (Milankovitch
cycles). Nowadays, the accepted explanation is that
orbital forcing sets the timing for
ice ages with CO
2 acting as an essential
amplifying feedback.
Arrhenius estimated that halving of CO
2 would decrease
temperatures by 4 - 5 °C (Celsius) and a doubling of
CO
2 would cause a temperature rise of 5 - 6 °C. In
his 1906 publication, Arrhenius adjusted the value downwards to
1.6 °C (including water vapour feedback: 2.1 °C). Recent
(2007) estimates from
IPCC say this
value (the
Climate sensitivity)
is likely to be between 2 and 4.5 °C. Arrhenius expected
CO
2 levels to rise at a rate given by emissions in his
time. Since then, industrial carbon dioxide levels have risen at a
much faster rate: Arrhenius expected CO
2 doubling to
take about 3000 years; it is now estimated in most scenarios to
take about a century.
Racial biology
Svante
Arrhenius was also actively engaged in the process leading to the
creation in 1922 of The State Institute for
Racial Biology in Uppsala, Sweden, which had originally been
planned as a Nobel
Institute
.
Arrhenius was a member of the institute's board, as he had been in
The Swedish Society for Racial Hygiene (Eugenics), founded in
1909.Swedish racial biology was world-leading at this time, and the
results formed the scientific basis for the
Compulsory sterilization program in
Sweden, as well as inspiring the
Nazi
eugenics in Germany.
See also
Bibliography
- Svante Arrhenius, 1884, Recherches sur la conductivité
galvanique des électrolytes, doctoral dissertation, Stockholm,
Royal publishing house, P.A. Norstedt & söner, 89 pages.
- Svante Arrhenius, 1896a, Ueber den Einfluss des
Atmosphärischen Kohlensäurengehalts auf die Temperatur der
Erdoberfläche, in the Proceedings of the Royal Swedish Academy
of Science, Stockholm 1896, Volume 22, I N. 1, pages 1–101.
- Svante Arrhenius, 1896b, On the Influence of Carbonic Acid in the Air upon the
Temperature of the Ground, London, Edinburgh, and Dublin
Philosophical Magazine and Journal of Science (fifth series), April
1896. vol 41, pages 237–275.
- Svante Arrhenius, 1901a, Ueber die Wärmeabsorption durch
Kohlensäure, Annalen der Physik, Vol 4, 1901, pages
690–705.
- Svante Arrhenius, 1901b, Über Die Wärmeabsorption Durch
Kohlensäure Und Ihren Einfluss Auf Die Temperatur Der
Erdoberfläche. Abstract of the proceedings of the Royal
Academy of Science, 58, 25–58.
- Svante Arrhenius, 1903, Lehrbuch der Kosmischen
Physik, Vol I and II, S. Hirschel publishing house, Leipzig,
1026 pages.
- Svante Arrhenius, 1906, Die vermutliche Ursache der
Klimaschwankungen, Meddelanden från K. Vetenskapsakademiens
Nobelinstitut, Vol 1 No 2, pages 1–10
- Svante Arrhenius, 1908, Das Werden der Welten,
Academic Publishing House, Leipzig, 208 pages.
References
- Patrick Coffey, Cathedrals of Science: The Personalities
and Rivalries That Made Modern Chemistry, Oxford University
Press, 2008,
- Fellow of the month - Arrhenius
- " On the Influence of Carbonic Acid in the Air Upon the
Temperature of the Ground", Philosophical Magazine 1896(41):
237-76
- The Carbon Dioxide Greenhouse Effect at
www.aip.org
Further reading
- Crawford, Elisabeth T. Arrhenius: from ionic theory to the
greenhouse effect Canton, MA: Science History Publications.
ISBN 0881351660
- Patrick Coffey, Cathedrals of Science: The Personalities
and Rivalries That Made Modern Chemistry, Oxford University
Press, 2008. ISBN 978-0-19-532134-0
External links