Lord Kelvin and the age of the earth

1977 ◽  
Vol 303 (2) ◽  
pp. 223-224
Author(s):  
Alan J. Rocke
Keyword(s):  
1926 ◽  
Vol 45 (1) ◽  
pp. 1-2
Author(s):  
J. Alfred Ewing

In this the centenary year of Lord Kelvin's birth it is fitting that the Society should call to remembrance one who was for long its most distinguished Fellow, who first became its President at the age of thirty-nine, and was repeatedly re-elected to the office, which he held for twenty-one years in all, and who used the Society as a medium for the publication of many of his most brilliant discoveries. In the long list of his published papers there are at least one hundred and twenty items communicated to the Royal Society of Edinburgh. No other contributor has done so much to give to our Proceedings and Transactions a world-wide and lasting fame. It was to this Society that he brought, in 1849, his account of Carnot's Theory, which marks the beginning of his study of Thermodynamics, and it was in our Transactions that he published his epochmaking series of papers on the “Dynamical Theory of Heat” from 1851 to 1854. It was here in 1852 that he propounded the doctrine of the Dissipation of Energy. It was here that his investigations of underground temperature and the secular cooling of the Earth appeared in 1860 and 1862. It was here in 1865 that he “briefly refuted” the doctrine of Uniformity in Geology. Here, too, were published his long series of papers on Vortex Motion and Vortex Atoms, from 1867 to 1881, and much of his work on the molecular constitution of matter. Here he first showed, in germ, his mariner's compass, in 1874.


Philosophy ◽  
1930 ◽  
Vol 5 (19) ◽  
pp. 364-378 ◽  
Author(s):  
Leonard Hill

With the progress of science we become more and more aware of the undiscovered, and of our feebleness to visualize or express what is dimly known to us. Geologists estimate that man evolved some 1,000,000 years ago on an earth which astronomers say is some 2,000,000,000 years old. Caution is required in accepting such figures, for we must remember how far out Lord Kelvin was in estimating the age of the earth—before the discovery of radium. Man has been civilized for some 5,000 years, and Galileo, with his telescope and revolutionary ideas, lived some 300 years ago. There may be, we are told, a million million years before the sun grows weak and the earth becomes farther from the sun so that all life freezes. Long before this man may use up the metals available for his machines, and those ready sources of energy now so wastefully used, by which he at present multiplies and swarms in cities. In such case he will return through birth control or famine, or both, to a simple, uncrowded, pastoral existence. There is little likelihood of his being able to use atomic energy, other than that which reaches the earth as sun radiation and is available directly or as energy stored in water-power, wood, coal, and oil.


Isis ◽  
1976 ◽  
Vol 67 (3) ◽  
pp. 492-494
Author(s):  
Jed Z. Buchwald
Keyword(s):  

Author(s):  
A. Cook

Fellows of The Royal Society have been concerned with the definition and measurement of time from the first days of the Society. John Flamsteed, F.R.S., ‘Royal Astronomer’, showed that the rotation of the Earth was isochronous and that the length of the solar day varied with the season because the path of the Earth about the Sun was an ellipse inclined to the Equator of the Earth. In the 20th century, D.W. Dye, F.R.S., made quartz oscillators that replaced mechanical clocks, and L. Essen, F.R.S., brought into use at the National Physical Laboratory the first caesium beam frequency standard and advocated that atomic time should replace astronomical time as the standard. The Society supported the development of chronometers for use at sea to determine longitude, and Fellows used the electric telegraph to find longitude in India. Edmond Halley, F.R.S., estimated the age of the Earth from the saltiness of lakes and seas; Lord Kelvin, F.R.S., estimated the rate at which energy was being radiated from the Sun; and Lord Rutherford, F.R.S., showed how the ages of rocks and of the Earth could be found from decay of radioactive minerals in them.


1982 ◽  
Vol 15 (2) ◽  
pp. 155-181 ◽  
Author(s):  
Frank A. J. L. James

In 1859 Charles Darwin in chapter nine of the Origin of Species showed how he had calculated that the age of the Weald was three hundred million years and that consequently the age of the earth was considerably greater than that. Darwin of course needed such a long period of time for the process of evolution by natural selection to occur. Arguments which showed that the earth could not be that old would therefore cast serious doubt on his theory. Such views were advanced in 1862 by William Thomson, later Lord Kelvin, professor of Natural Philosophy at Glasgow. He specifically challenged the result of Darwin's calculation of the age of the Weald by arguing that the sun could not have emitted its heat and light for that length of time. The consequences of this assertion for the biological and geological sciences for the remainder of the nineteenth century have already been delineated by Burchfield. What I wish to do in this paper is to show that the theoretical basis of Thomson's 1862 assertion had not been specifically developed as a response to Darwin, but that it was a consequence of the formulation of the first two laws of thermodynamics. I shall also show that Thomson's work was not done in isolation but that the question of the maintenance of solar energy was a serious concern of a number of physicists who had formulated the laws of thermodynamics.


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