|
|
|
|
John Michell
|
| |
|
| |
John Michell (December 25, 1724 – April 29, 1793) was an English natural philosopher and geologist whose work spanned a wide range of subjects from astronomy to geology, optics, and gravitation. He was both a theorist and an experimenter.
Michell was educated at Queens' College, Cambridge and later became a Fellow of Queens'. He obtained his M.A. in 1752 and B.D. in 1761. In 1760 he was elected a Fellow of the Royal Society, in the same year as Henry Cavendish. In 1762 he was appointed Woodwardian Professor of Geology, and in 1767 he became rector of Thornhill, West Yorkshire, near Dewsbury, where he died.
He was thus described by a contemporary commentator:
John Michell, BD is a little short Man, of a black Complexion, and fat; but having no Acquaintance with him, can say little of him.
Discussion
Ask a question about 'John Michell' Start a new discussion about 'John Michell' Answer questions from other users |
Encyclopedia
John Michell (December 25, 1724 – April 29, 1793) was an English natural philosopher and geologist whose work spanned a wide range of subjects from astronomy to geology, optics, and gravitation. He was both a theorist and an experimenter.
Michell was educated at Queens' College, Cambridge and later became a Fellow of Queens'. He obtained his M.A. in 1752 and B.D. in 1761. In 1760 he was elected a Fellow of the Royal Society, in the same year as Henry Cavendish. In 1762 he was appointed Woodwardian Professor of Geology, and in 1767 he became rector of Thornhill, West Yorkshire, near Dewsbury, where he died.
He was thus described by a contemporary commentator:
John Michell, BD is a little short Man, of a black Complexion, and fat; but having no Acquaintance with him, can say little of him. I think he had the care of St. Botolph’s Church Cambridge, while he continued Fellow of Queen's College, where he was esteemed a very ingenious Man, and an excellent Philosopher. He has published some things in that way, on the Magnet and Electricity.’
.
Work
Gravity, magnetism & light
Michell conceived, sometime before 1783, the experiment now known as the Cavendish experiment. It was the first to measure the force of gravity between masses in the laboratory and produced the first accurate values for the mass of the Earth and the gravitational constant. He invented and built, independently of co-inventor Charles Augustin de Coulomb, a torsion balance for the experiment but didn’t live to put it to use. His apparatus passed to Henry Cavendish, who performed the experiment in 1798. In 1987, gravity researcher A.H. Cook wrote:
- The most important advance in experiments on gravitation and other delicate measurements was the introduction of the torsion balance by Michell and its use by Cavendish. It has been the basis of all the most significant experiments on gravitation ever since.
In 1750 he published at Cambridge a work of some eighty pages entitled A Treatise of Artificial Magnets, in which is shown an easy and expeditious method of making them superior to the best natural ones. Besides the description of the method of magnetization which still bears his name, this work contains a variety of accurate magnetic observations, and is distinguished by a lucid exposition of the nature of magnetic induction.
At one point, Michell attempted to measure the radiation pressure of light by focusing sunlight onto one side of a compass needle. The experiment was not a success: the needle melted.
Geology
In scientific biographies written during the early 20th century, Michell's historical importance is ascribed to his work on geology. His most important geological essay was entitled "Conjectures concerning the Cause and Observations upon the Phaenomena of Earthquakes" (Philosophical Transactions, li. 1760), which showed a remarkable knowledge of the strata in various parts of England and abroad.
Effect of gravity on light
More recently, Michell's main "claim to fame" is considered to be his letter to Cavendish, published in 1784, on the effect of gravity on light. This paper was only generally "rediscovered" in the 1970s and is now recognised as anticipating several astronomical ideas that had been considered to be 20th century innovations. Michell is now credited with being the first to study the case of a heavenly object massive enough to prevent light from escaping (the concept of escape velocity was well known at the time). Such an object would not be directly visible, but could be identified by the motions of a companion star if it was part of a binary system. Michell also suggested using a prism to measure the gravitational weakening of starlight due to the surface gravity of the source ("gravitational shift"). Michell acknowledged that some of these ideas were not technically practical at the time, but wrote that he hoped they would be useful to future generations. By the time that Michell's paper was "resurrected" nearly two centuries later, these ideas had been reinvented by others.
The mathematician Pierre-Simon Laplace suggested the same idea of high-gravity objects trapping light in his book Exposition du Systeme du Monde in 1796. This sort of high-gravity object under Newtonian theory is commonly referred to as a dark star, and can be thought of as being the predecessor of the modern idea of a black hole under general relativity.
Some of Michell's contributions
- Observations On the Comet of January 1760 at Cambridge, Philosophical Transactions (1760)
- Conjectures Concerning the Cause and Observations upon the Phaenomena of Earthquakes, ibid. (1760)
- A Recommendation of Hadley's Quadrant for Surveying, ibid. (1765)
- Proposal of a Method for measuring Degrees of Longitude upon Parallels of the Equator, ibid. (1766)
- An Inquiry into the Probable Parallax and Magnitude of the Fixed Stars, ibid. (1767)
- On the Twinkling of the Fixed Stars, ibid. (1767)
- On the Means of Discovering the Distance, Magnitude, &c., of the Fixed Stars, ibid. (1784).
External links
- . Description of Michell's theory of black holes
-
-
|
| |
|
|
