| Coordinates | 6°7′55″N1°13′22″N |
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| name | John Tyndall |
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| birth place | Leighlinbridge, County Carlow, Ireland |
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| death date | (aged 73) |
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| death place | Haslemere, Surrey, England |
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| nationality | British |
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| field | Physics, Chemistry |
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| work institution | Royal Institution of Great Britain |
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| alma mater | University of Marburg |
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| known for | Atmosphere, physics education, Tyndall effect, diamagnetism, infrared radiation, Tyndallization |
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| footnotes | }} |
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John Tyndall FRS (2 August 1820 – 4 December 1893) was a prominent 19th century physicist. His initial scientific fame arose in the 1850s from his study of
diamagnetism. Later he studied
thermal radiation, and produced a number of discoveries about processes in the
atmosphere. Tyndall published seventeen books, which brought state-of-the-art 19th century
experimental physics to a wider audience. From 1853 to 1887 he was professor of physics at the
Royal Institution of Great Britain, where he became the successor to positions held by
Michael Faraday.
Early years and education
Tyndall was born in
Leighlinbridge,
County Carlow,
Ireland. His father was a local police constable, descended from
Gloucestershire emigrants who settled in southeast Ireland around 1670. Tyndall attended the local schools in County Carlow until his late teens, and was probably an assistant teacher near the end of his time there. Subjects learned at school notably included
technical drawing and mathematics with some applications of those subjects to
land surveying. He was hired as a
draftsman by the government's land surveying & mapping agency in Ireland in his late teens in 1839, and moved to work for the same agency in England in 1842. In the decade of the 1840s, a railroad-building boom was in progress, and Tyndall's land surveying experience was valuable and in demand by the railway companies. Between 1844 and 1847, he was lucratively employed in railway construction planning.
In 1847 Tyndall opted to become a mathematics and surveying teacher at a boarding school in
Hampshire. Recalling this decision later, he wrote: "the desire to grow intellectually did not forsake me; and, when railway work slackened, I accepted in 1847 a post as master in Queenwood College." Another recently arrived young teacher at Queenwood was
Edward Frankland, who had previously worked as a chemical laboratory assistant for the British Geological Survey. Frankland and Tyndall became good friends. On the strength of Frankland's prior knowledge, they decided to go to Germany to further their education in science. Among other things, Frankland knew that certain German universities were ahead of any in Britain in experimental chemistry and physics. (British universities were still focused on classics and mathematics and not laboratory science.) The pair moved to Germany in summer 1848 and enrolled at the
University of Marburg, where
Robert Bunsen was an influential teacher. Tyndall studied under Bunsen for two years. Perhaps more influential for Tyndall at Marburg was Professor
Hermann Knoblauch, with whom Tyndall maintained communications by letter for many years afterwards. Tyndall's Marburg dissertation was a mathematical analysis of screw surfaces in 1850 (under Friedrich Ludwig Stegmann). He stayed at Marburg for a further year doing research on magnetism with Knoblauch, including some months' visit at the Berlin laboratory of Knoblauch's main teacher,
Heinrich Gustav Magnus. It is clear today that Bunsen and Magnus were among the very best experimental science instructors of the era. Thus, when Tyndall returned to live in England in summer 1851, he probably had as good an education in experimental science as anyone in England.
Early scientific work
Tyndall's early original work in physics was his experiments on
magnetism and
diamagnetic polarity, on which he worked from 1850 to 1856. His two most influential reports were the first two, co-authored with Knoblauch. One of them was entitled "The magneto-optic properties of crystals, and the relation of magnetism and diamagnetism to molecular arrangement", dated May 1850. The two described an inspired experiment, with an inspired interpretation. These and other magnetic investigations very soon made Tyndall known among the leading scientists of the day. He was elected a
Fellow of the Royal Society in 1852. In his search for a suitable research appointment, he was able to ask the longtime editor of the leading German physics journal (
Poggendorff) and other prominent men to write testimonials on his behalf. In 1853, he attained the prestigious appointment of Professor of
Natural Philosophy (Physics) at the Royal Institution in London, due in no small part to the esteem his work had garnered from
Michael Faraday, the leader of magnetic investigations at the Royal Institution.
Main scientific work
Beginning in the late 1850s, Tyndall studied the action of
radiant energy on the constituents of
air, and it led him onto several lines of inquiry, and his original research results included the following:
Tyndall explained the heat in the Earth's atmosphere in terms of the capacities of the various gases in the air to
absorb radiant heat, a.k.a. infrared radiation. His measuring device, which used
thermopile technology, is an early landmark in the history of
absorption spectroscopy of gases. He was the first to correctly measure the relative infrared absorptive powers of the gases nitrogen, oxygen, water vapour, carbon dioxide, ozone, methane, etc. He concluded that
water vapour is the strongest absorber of radiant heat in the atmosphere and is the principal gas controlling air temperature. Absorption by the other gases is not negligible but relatively small. Prior to Tyndall it was widely surmised that the Earth's atmosphere has a
Greenhouse Effect, but he was the first to prove it. The proof was that water vapor strongly absorbed infrared radiation.
He devised demonstrations that advanced the question of how radiant heat is absorbed and emitted at the molecular level. He appears to be the first person to have demonstrated experimentally that emission of heat in chemical reactions has its physical origination within the newly created molecules (1864). He produced instructive demonstrations involving what he called calorescence, which is the conversion of infrared into visible light at the molecular level. Among his key laboratory tools were substances that are transparent to infrared and opaque to visible light; or vice versa. He usually referred to infrared as "radiant heat", and sometimes as "ultra-red undulations", as the word "infrared" did not start coming into use until the 1880s. His main published reports of the 1860s were republished as a 450-page collection in 1872 under the title ''Contributions to Molecular Physics in the Domain of Radiant Heat''.
In the investigations on radiant heat in air it had been necessary to use air from which all traces of floating dust and other particulates had been removed. A very sensitive way to detect particulates is to bathe the air with intense light. The scattering of light by particulate impurities in air and other gases, and in liquids, is known today as the Tyndall Effect or Tyndall Scattering. In studying this scattering during the late 1860s Tyndall was a beneficiary of recent improvements in electric-powered lights. He also had the use of good light concentrators. He developed the nephelometer and turbidimeter and similar instruments that show properties of aerosols and colloids through concentrated light beams. Particulates suspended in air are visible to the naked eye in a darkened room with sunlight coming through a crack in the curtains. Mostly visibly that's light reflecting off large particulates which is not the same as light scattering off small particulates. But with dark background illumination and customized light beams, and without microscopes, very low concentrations of particulates very far below the threshold of visibility become visible and quantifiable because of light scattering. When combined with microscopes, the result is the ultramicroscope, which was developed later by others. Tyndall is the founder of this line of instruments, which are based on exploiting the Tyndall effect.
In the lab he came up with a simple way to obtain "optically pure" air. He coated the inside walls of a box with glycerin, which is a sticky syrup. He discovered that after a few days' wait, the air inside the sealed box was entirely particulate-free under examination with light beams (the box had glass windows for the purpose). The various floating-matter particulates had all ended up getting stuck to the walls or settling on the sticky floor. There were no signs of floating micro-organisms ("germs") in the optically pure air. He compared what happened when he let sterilized meat-broths sit in such pure air, and in ordinary air. The broths were sterilized beforehand by boiling. The broths sitting in the optically pure air remained "sweet" (as he said) to smell and taste after many months of sitting, while the ones in ordinary air started to become putrid after a few days. This demonstration extended Louis Pasteur's earlier demonstrations that the presence of micro-organisms is a precondition for biomass decomposition. However, the next year (1876) some repeats of the exercise resulted in a surprising failure to reproduce it. From this he was led to find viable bacterial spores in supposedly heat-sterilized foods. The foods had been contaminated with dry bacterial spores from hay in the lab, he found out. All bacteria are killed by boiling but they have a spore form that can survive boiling, he correctly contended, citing research by Ferdinand Cohn. Tyndall found a way to eradicate the bacterial spores that came to be known as "Tyndallization". At the time, it affirmed the "germ theory" against a number of critics whose experimental results had been defective from the same cause. During the mid-1870s Pasteur and Tyndall were in frequent communication.
He was the first to observe and report the phenomenon of thermophoresis in aerosols. He spotted it surrounding hot objects while investigating the Tyndall Effect with focused lightbeams in a dark room. He devised a better way to demonstrate it, and then simply reported it (1870), without investigating the physics of it in depth.
In radiant-heat experiments that called for much laboratory expertise in the early 1860s, he showed for a variety of readily vaporizable liquids that, molecule for molecule, the vapor form and the liquid form have essentially the same power to absorb radiant heat. (In modern experiments using narrow-band spectra, some relatively small differences are found that Tyndall's equipment was unable to get at; see e.g. absorption spectrum of H2O).
He consolidated and enhanced the work of Desains, Forbes, Knoblauch and others demonstrating that the principal properties of visible light can be reproduced for radiant heat, namely reflection, refraction, diffraction, polarization, depolarization, double refraction, and rotation in a magnetic field (Faraday effect).
When studying the absorption of radiant heat by ozone, he came up with a demonstration that helped confirm that ozone is an oxygen cluster.
Using his expertise about radiant heat absorption by gases, he invented a system for measuring the amount of carbon dioxide in a sample of exhaled human breath (1862, 1864). The basics of Tyndall's system is in daily use in hospitals today for monitoring patients under anesthesia. (See capnometry.)
Invented a better fireman's respirator, a hood that filtered smoke and noxious gas from air (1871, 1874).
In the late 1860s and early 1870s he wrote an introductory book and several research reports about sound propagation in air, and was one of the chief participants in a large-scale British project that developed a better foghorn. In laboratory demonstrations motivated by foghorn issues, he established that sound is partially ''reflected'' (i.e. partially bounced back like an echo) at the location where an air mass of one temperature meets another air mass of a different temperature; and more generally when a body of air contains two or more separate air masses of different densities or temperatures, the sound travels poorly because of reflections occurring at the interfaces between the air masses, and very poorly when many such interfaces are present. (He then argued, though inconclusively, that this is the usual main reason why the same distant sound, e.g. foghorn, can be heard stronger or fainter on different days or at different times of day.)
An index of 19th century scientific research journals has John Tyndall as the author of more than 147 papers, with practically all of them dated between 1850 and 1884, which is an average of more than four papers a year over that 35-year period.
Tyndall was an experimenter and laboratory apparatus builder, not an abstract model builder. He did attempt to extend his studies on the heat-absorptive power of gases and vapors into a research program about molecules. That is one of the underlying agendas of his 1872 book ''Contributions to Molecular Physics in the Domain of Radiant Heat''. It is also evident in the spirit of his widely read 1863 book ''Heat Considered as a Mode of Motion''. Besides heat, he also saw phenomena of magnetism and sound propagation as reducible to molecular behaviors. Invisible molecular behaviors were the ultimate substrate of all physical activity. With this mindset, and his experiments, he outlined an account whereby differing types of molecules have differing absorptions of infrared radiation because their molecular structures give them differing oscillating resonances. He'd gotten into the oscillating resonances idea because he'd seen that any one type of molecule has differing absorptions at differing radiant frequencies and he was entirely persuaded that the only difference between one frequency and another is the frequency. He'd also seen that the absorption behavior of molecules is quite different from that of the atoms composing the molecules — for example the gas nitric oxide (NO) absorbed more than a thousand times more infrared radiation than either nitrogen (N2) or oxygen (O2). He'd also seen in several kinds of experiments that no matter whether a gas is a weak absorber of broad-spectrum radiant heat, it will strongly absorb the radiant heat coming from a separate body of the same type of gas. That demonstrated a kinship between the molecular mechanisms of absorption and emission. Such a kinship was also in evidence in experiments by Balfour Stewart and others, cited and extended by Tyndall, that showed with respect to broad-spectrum radiant heat that molecules that are weak absorbers are weak emitters and strong absorbers are strong emitters. (For example rock-salt is an exceptionally poor absorber of heat via radiation, and a good absorber of heat via conduction. When a plate of rock-salt is heated via conduction and let stand on an insulator, it takes an exceptionally long time to cool down; i.e., it's a poor emitter of infrared.) The kinship between absorption and emission was also consistent with some generic or abstract features of resonators. The photochemical effect convinced Tyndall that the resonator could not be the molecule as a whole unit; it had to be some substructure, because otherwise the photochemical effect would be impossible. But he was without testable ideas as to the form of this substructure, and did not partake in speculation in print. His promotion of the molecular mindset, and his efforts to experimentally expose what molecules are, has been discussed by one historian under the title ''"John Tyndall, The Rhetorician Of Molecularity"''.
In his lectures at the Royal Institution Tyndall put a great value on — and was talented at producing — lively, visible demonstrations of physics concepts. In one lecture, published later in one of his books, Tyndall demonstrated the propagation of light down through a stream of falling water via total internal reflection of the light. It was referred to as the "light fountain". It is historically significant today because it demonstrates the scientific foundation for modern fiber optic technology. During second half of the 20th century Tyndall was usually credited with being the first to make this demonstration. However, Jean-Daniel Colladon published a report of it in Comptes Rendus in 1842, and there's some suggestive evidence that Tyndall's knowledge of it came ultimately from Colladon and no evidence that Tyndall claimed to have originated it himself.
Alpine mountaineering and glaciology
Tyndall visited the Alps mountains in 1856 for scientific reasons and ended up becoming a pioneering mountain climber. He visited the Alps almost every summer from 1856 onward, was a member of the very first mountain-climbing team to reach the top of the Weisshorn (1861), and lead of one of the early teams to reach the top of the Matterhorn (1868). He is one the names associated with the "golden age of Alpinism", i.e. the mid-Victorian years when the more difficult of the Alpine peaks were summited for the first time.
In the Alps, Tyndall studied glaciers, and especially glacier motion. His explanation of glacial flow brought him into dispute with others, particularly James David Forbes. Much of the early scientific work had been done by Forbes, but Forbes at that time didn't know of the phenomenon of Regelation which was discovered a little later by Michael Faraday. Regelation played a key role in Tyndall's explanation. Forbes didn't see regelation in the same way at all. Complicating their debate, a disagreement arose publicly over who deserved to get investigator credit for what. Articulate friends of Forbes, as well as Forbes himself, thought that Forbes should get the credit for most of the good science, whereas Tyndall thought the credit should be distributed more widely. Tyndall commented: "The idea of semi-fluid motion belongs entirely to Louis Rendu; the proof of the quicker central flow belongs in part to Rendu, but almost wholly to Louis Agassiz and Forbes; the proof of the retardation of the bed belongs to Forbes alone; while the discovery of the locus of the point of maximum motion belongs, I suppose, to me." When Forbes and Tyndall were in the grave, their disagreement was continued by their respective official biographers. Everyone tried to be reasonable, but agreement wasn't attained. More disappointingly, aspects of glacier motion remained not understood or not proved.
Tyndall Glacier in Chile is named after John Tyndall, as is Mount Tyndall in California and Mount Tyndall in Tasmania.
Educator
Besides being a scientist, John Tyndall was a science teacher and evangelist for the cause of science. He spent a significant amount of his time disseminating science to the general public — contributing over the years to science columns in popular middle class periodicals such as the ''
Athenaeum'' and the ''
Saturday Review'' in the UK, and ''
Popular Science Monthly'' in the USA; and giving hundreds of public lectures to non-specialist audiences at the Royal Institution. When he went on a public lecture tour in the USA in 1872, large crowds paid fees to hear him lecture about the nature of
light. A typical statement of Tyndall's reputation at the time is this from a London publication in 1878: "Following the precedent set by Faraday, Professor Tyndall has succeeded not only in original investigation and in teaching science soundly and accurately, but in making it attractive.... When he lectures at the Royal Institution the theatre is crowded." Tyndall said of the occupation of teacher "I do not know a higher, nobler, and more blessed calling." His greatest audience was gained ultimately through his books, most of which were not written for experts or specialists. He published 17 science books. From the mid-1860s on, he was one of the world's most famous living physicists, due firstly to his skill and industry as a tutorialist. Most of his books were translated into German and French with his main tutorials staying in print in those languages for decades.
As an indicator of his teaching attitude, here are his concluding remarks to the reader at the end of a 200-page tutorial book (1872): "Here, my friend, our labours close. It has been a true pleasure to me to have you at my side so long. In the sweat of our brows we have often reached the heights where our work lay, but you have been steadfast and industrious throughout, using in all possible cases your own muscles instead of relying upon mine. Here and there I have stretched an arm and helped you to a ledge, but the work of climbing has been almost exclusively your own. It is thus that I should like to teach you all things; showing you the way to profitable exertion, but leaving the exertion to you.... Our task seems plain enough, but you and I know how often we have had to wrangle resolutely with the facts to bring out their meaning. The work, however, is now done, and you are master of a fragment of that sure and certain knowledge which is founded on the faithful study of nature.... Here then we part. And should we not meet again, the memory of these days will still unite us. Give me your hand. Good bye."
As another indicator, here is the opening paragraph of his 350-page tutorial entitled ''Sound'' (1867): "In the following pages I have tried to render the science of acoustics interesting to all intelligent persons, including those who do not possess any special scientific culture. The subject is treated experimentally throughout, and I have endeavoured so to place each experiment before the reader that he should realise it as an actual operation." In the preface to the 3rd edition of this book he reports that earlier editions were translated into Chinese at the expense of the Chinese government; and translated into German under the supervision of Hermann von Helmholtz (a big name in the science of acoustics). His first published tutorial, which was about glaciers (1860), similarly states: "The work is written with a desire to interest intelligent persons who may not possess any special scientific culture."
His most widely praised tutorial, and perhaps also his biggest seller, was the 550-page ''"Heat: a Mode of Motion"'' (1863; updated editions until 1880). It was in print for at least 50 years, and is in print today. Its primary feature is as James Clerk Maxwell said, "the doctrines of the science [of heat] are forcibly impressed on the mind by well-chosen illustrative experiments."
His three longest tutorials, namely ''Heat'' (1863), ''Sound'' (1867), and ''Light'' (1873), represented state-of-the-art experimental physics at the time they were written. Much of their contents were recent major innovations in the understanding of their respective subjects, which Tyndall was the first writer to present to a wider audience. One caveat is called for about the meaning of "state of the art". The books were devoted to laboratory science and they avoided mathematics. In particular, they contain absolutely no infinitesimal calculus. Mathematical modeling using infinitesimal calculus, especially differential equations, was a component of the state-of-the-art understanding of heat, light and sound at the time.
Demarcation of science from religion
The majority of the progressive and innovative British physicists of Tyndall's generation were conservative and orthodox on matters of religion. That includes for example James Joule, Balfour Stewart, James Clerk Maxwell, George Gabriel Stokes and William Thomson — all names investigating heat or light contemporaneously with Tyndall. These conservatives believed, and sought to strengthen the basis for believing, that religion and science were consistent and harmonious with each other. Tyndall, however, was a member of the X Club that vocally supported Darwin's theory of evolution and sought to strengthen the barrier, or separation, between religion and science. The most prominent member of this club was the anatomist Thomas Henry Huxley. Tyndall first met Huxley in 1851 and the two had a lifelong friendship. Chemist Edward Frankland and mathematician Thomas Archer Hirst, both of whom Tyndall had known since before going to university in Germany, were members too. Others included the social philosopher Herbert Spencer. See X-Club.
Though not nearly so prominent as Huxley in controversy over philosophical problems, Tyndall played his part in communicating to the educated public what he thought were the virtues of having a clear separation between science (knowledge & rationality) and religion (faith & spirituality). As the elected president of the British Association for the Advancement of Science in 1874, he gave a long keynote speech at the Association's annual meeting held that year in Belfast. The speech gave a favorable account of the history of evolutionary theories, mentioning Darwin's name favorably more than 20 times, and concluded by asserting that religious sentiment should not be permitted to "intrude on the region of ''knowledge'', over which it holds no command". This was a hot topic. The newspapers carried the report of it on their front pages — in the British Isles, North America, even the European Continent — and many critiques of it appeared soon after. The attention and scrutiny increased the friends of the evolutionists' philosophical position, and brought it closer to mainstream ascendancy.
In Rome the Pope in 1864 decreed that it was an ''error'' that "reason is the ultimate standard by which man can and ought to arrive at knowledge" and an ''error'' that "divine revelation is imperfect" in the Bible — and anyone maintaining those errors was to be "anathematized" — and in 1888 decreed as follows: "The fundamental doctrine of rationalism is the supremacy of the human reason, which, refusing due submission to the divine and eternal reason, proclaims its own independence.... A doctrine of such character is most hurtful both to individuals and to the State.... It follows that it is quite unlawful to demand, to defend, or to grant, unconditional [or promiscuous] freedom of thought, speech, writing, or religion." Those principles and Tyndall's principles were profound enemies. Luckily for Tyndall he didn't need to get into a contest with them, in Britain, nor in most other parts of the world. Even in Italy, Huxley and Darwin were awarded honorary medals and most of the Italian governing class was hostile to the papacy. But in Ireland during Tyndall's lifetime the majority of the population grew increasingly doctrinaire and vigorous in its Roman Catholicism and also grew stronger politically. It would've been a waste of everybody's time for Tyndall to debate the Irish Catholics, but he was active in the debate in England about whether to give the Catholics of Ireland more freedom to go their own way. Like the great majority of Irish-born scientists of the 19th century he opposed the Irish Home Rule Movement. He had ardent views about it, which were published in newspapers and pamphlets. For example in an opinion piece in ''The Times'' on 27 Dec 1890 he saw priests and Catholicism as "the heart and soul of this movement" and wrote that placing the non-Catholic minority under the dominion of "the priestly horde" would be "an unspeakable crime". He tried unsuccessfully to get the UK's premier scientific society to denounce the Irish Home Rule proposal as contrary to the interests of science.
In several essays included in his book ''Fragments of Science for Unscientific People'', Tyndall attempted to dissuade people from believing in the potential effectiveness of prayers. At the same time, though, he was not broadly anti-religious, and his writings leave no straightforward evidence that he was not a Christian or at least a Deist.
Private life
Tyndall did not marry until age 55. His bride, Louisa Hamilton, who he had first met in the Alps, was the 30-year-old daughter of a member of parliament (
Lord Claud Hamilton, M.P.). The following year, 1877, they built a summer
chalet at
Belalp, in the Swiss Alps, where, after his death, his wife had the "Tyndall-Denkmal" monument erected 20 minutes above the Tyndall chalet, on the Triembiel. Before getting married Tyndall had been living for many years in an upstairs apartment at the Royal Institution and continued living there after marriage until 1885 when a move was made to a house near
Haslemere 45 miles southwest of London. The marriage was a happy one and without children. He retired from the Royal Institution at age 66 having complaints of ill health.
Tyndall became financially well-off from sales of his popular books and fees from his lectures (but there is no evidence that he owned commercial patents). For many years he got non-trivial payments for being a part-time scientific advisor to a couple of quasi-governmental agencies and partly donated the payments to charity. His successful lecture tour of the United States in 1872 netted him a substantial amount of dollars, all of which he promptly donated to a trustee for fostering science in America. Late in life his money donations went most visibly to the Irish Unionist political cause. When he died, his wealth was £22122. For comparison's sake, the income of a police constable in London was about £80 per year at the time.
In his last years Tyndall often took chloral hydrate to treat his insomnia. When bedridden and ailing, he died from an accidental overdose of this drug at age 73, and was buried at Haslemere. Afterwards, Tyndall's wife took possession of his papers and assigned herself as supervisor of an official biography of him. She dragged her feet on the project, however, and it was still unfinished when she died in 1940 aged 95. The book eventually appeared in 1945, written by A. S. Eve and C. H. Creasey, whom Louisa Tyndall had authorized shortly before her death.
John Tyndall's books
The Glaciers of the Alps (470 pages) (1860)
Heat as a Mode of Motion (550 pages) (1863; revised later editions)
On Radiation: One Lecture (40 pages) (1865)
Sound: A Course of Eight Lectures (350 pages) (1867; revised later editions)
Faraday as a Discoverer (180 pages) (1868)
Natural Philosophy in Easy Lessons (180 pages) (1869) (a book intended for use in secondary schools)
Three Scientific Addresses by Prof. John Tyndall (75 pages) (1870)
Notes of a Course of Nine Lectures on Light (80 pages) (1870)
Notes of a Course of Seven Lectures on Electrical Phenomena and Theories (50 pages) (1870)
Researches on Diamagnetism and Magne-crystallic Action (380 pages) (1870) (a compilation of 1850s research reports)
Hours of Exercise in the Alps (450 pages) (1871)
Fragments of Science: A Series of Detached Essays, Lectures, and Reviews (over 500 pages) (1871; expanded later editions)
The Forms of Water in Clouds and Rivers, Ice and Glaciers (200 pages) (1872)
Contributions to Molecular Physics in the Domain of Radiant Heat (450 pages) (1872) (a compilation of 1860s research reports)
Six Lectures on Light (290 pages) (1873)
Lessons in Electricity at the Royal Institution (100 pages) (1876)
Essays on the Floating-matter of the Air in relation to Putrefaction and Infection (360 pages) (1881)
New Fragments (500 pages) (1892)
''All of the above books can be freely downloaded at
Archive.org.''
''Nearly all of them are in print and can be
bought new.''
Biographies of John Tyndall
430 pages. This is the "official" biography.
William T. Jeans wrote a 100-page biography of Professor Tyndall in 1887 (the year Tyndall retired from the Royal Institution). It is available
here
Louisa Charlotte Tyndall, his wife, wrote an 8-page biography of John Tyndall that appeared in 1903 as the preface to one of his books. Available
here
Edward Frankland wrote a 16-page biography of John Tyndall as an obituary in 1894 in a British scientific journal. The journal volume is available
here
D. Thompson in ''Journal of Vocational Education & Training'', volume 9:18, pages 38–48, year 1957, has an article entitled "John Tyndall (1820–1893): A study in vocational enterprise" which gives an account of Tyndall's vocational development prior to 1853. Available here.
220 pages.
Arthur Whitmore Smith, a professor of physics, wrote a 10-page biography of John Tyndall in 1920 in an American scientific monthly. Available
here (page 91)
John Walter Gregory, a naturalist, wrote a nine-page obituary of John Tyndall in 1894 in the monthly journal "''Natural Science''". The journal volume is here.
An early, seven-page profile of John Tyndall appeared in 1864 in ''Portraits of Men of Eminence in Literature, Science and Art'' (volume II). Available
here
A one-page profile of Tyndall, based on information supplied by Tyndall himself, appeared in 1874 in the weekly magazine ''Nature''. Available here.
''John Tyndall as a Mountaineer'', 56-page essay by Claud Schuster. Included in Schuster's book ''Postscript to Adventure'' New Alpine Library Eyre & Spottiswoode London 1950.
See also
Ice sheet dynamics
Spontaneous generation
John Tyndall's system for measuring radiant heat absorption in gases
Greenhouse gas
Footnotes
External links
Works by John Tyndall at Internet Archive
A blog maintained by a historian who is involved in transcribing Tyndall's letters.
Category:1820 births
Category:1893 deaths
Category:Experimental physicists
Category:University of Marburg alumni
Category:Scientific instrument makers
Category:British physicists
Category:Optical physicists
Category:Glaciologists
Category:British mountain climbers
Category:People from County Carlow
Category:Royal Medal winners
Category:Fellows of the Royal Society
Category:Drug-related deaths in England
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