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Reference : SLIVCN-9783836588348
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9783836588348
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(Paris, Bachelier, 1851-52). 4to. Later blank wrapper. Extracted from ""Comptes rendus hebdomadaires des séances de l’Académie des sciences"", Vol. 32 and vol. 35. Foucault's papers: pp. 135-138 (1851, vol. 32), pp. 421-424 (1852, vol. 35), pp. 424-427 (1852, vol. 35), pp. 469-470 (1852, vol. 35) and p. 602 (1852, vol. 35).
First appearance of the papers in which Foucault presented his discovery of the proof of the rotation of the earth by the large pendulum, called FOUCAULT'S PENDULUM. It was presented by Arago at the meeting of the Acadey of Scieces on February 3, 1851 (the first paper offered). In the third paper offered, ""Sur les phénoménes d'orientation des corps tournant entraînés par un axe fixe..."", Foucault presents his invention of the GYROSCOPE, a freely spinning flywheel, which constitutes a different method of demonstrating the rotation of the Earth"" he furthermore correctly predicts the use of the gyroscope as a compass. The word ""gyroscope"" was coined by Foucault (on p. 427 of the third paper), taken from the Greek, meaning ""to look at the rotation"".Since Léon Foucault's public demonstration of his pendulum experiment, it has played a prominent role in physics, physics education, and the history of science. The Foucault pendulum is a long pendulum suspended high above the ground and carefully set into planar motion. The phenomenon described by Foucault1 concerns the orientation of the plane of oscillation of the pendulum. ""The experiment (with the pendulum) caused great excitement at the time. Heracleides had first suggested twenty-two centuries before that the earth was rotating and Copernicus had renewed the suggestion three centuries before. Since the time of Galileo two and a half centuries before, the world of scholarship had not doubted the matter. Nevertheless, all evidence as to that rotation had been indirect, and not until Foucault's experiment could the earth's rotation actually be said to have been demonstrated rather that deduced."" ""Continuing to experiment on the mechanics of the earth's rotation, Foucault in 1852 invented the gyroscope, which, he showed, gave a clearer demonstration than the pendulum of the earth's rotation and had the property, similar to that of the magnetic needle, of maintaining a fixed direction. Foucault's pendulum and gyroscope had more than a popular significance (which continues to this day). First, they stimulated the development of theoretical mechanics, making relative motion and the theories of the pendulum and the gyroscope standard topics for study and investigation. Second, prior to Foucault's demonstrations the study of those motions on the earth's surface in which the deflecting force of rotation plays a prominent part (especially winds and ocean currents) was dominated by unphysical notions of how this force acted. Foucault's demonstrations and the theoretical treatments they inspired showed conclusively that this deflecting force acts in all horizontal directions, thus providing the sound physical insight on which Buys Ballot, Ferrel, Ulrich Vettin, and others could build. (DSB).PMM: 330 lists the offprint with the title ""Sur Divers Signes Sensibles du Mouvement Diurne de la Terre"" - Barchas Collection, 738 (the periodical version, but only the first paper) - Dibner, No. 17 (offprint version).
Paris, Bachelier, 1851-52. 4to. 2 uniform full cloth bindings. Gilt spines, gilt lettering. Gil lettering on spines: ""The Chemist's Club"". Faint marks of earlier paper labels to spine. In ""Comptes rendus hebdomadaires des séances de l’Académie des sciences"", Vol. 32 and vol. 35. Entire volumes offered. (4),1026 pp. + (4),1010 pp. A stamp on top and verso of title-pages. Foucault's papers: pp. 135-138 (1851, vol. 32), pp. 421-424 (1852, vol. 35), pp. 424-427 (1852, vol. 35), pp. 469-470 (1852, vol. 35) and p. 602 (1852, vol. 35).
First appearance of the seminal papers, in which Foucault presented his discovery of the proof of the rotation of the earth by the large pendulum, known as Foucault's Pendulum. The first papr offered here was presented by Arago at the meeting of the Acadey of Scieces on February 3, 1851. In the third paper, ""Sur les phénoménes d'orientation des corps tournant entraînés par un axe fixe..."", Foucault presents his invention of the gyroscope, a freely spinning flywheel, which constitutes a different method of demonstrating the rotation of the Earth"" he furthermore correctly predicts the use of the gyroscope as a compass and coins the word ""gyroscope"" (on p. 427), taken from the Greek, meaning ""to look at the rotation"".Ever since Léon Foucault's public demonstration of his pendulum experiment, it has played a prominent role in physics, physics education, and the history of science. The Foucault pendulum is a long pendulum suspended high above the ground and carefully set into planar motion. The phenomenon described by Foucault concerns the orientation of the plane of oscillation of the pendulum. ""The experiment (with the pendulum) caused great excitement at the time. Heracleides had first suggested twenty-two centuries before that the earth was rotating and Copernicus had renewed the suggestion three centuries before. Since the time of Galileo two and a half centuries before, the world of scholarship had not doubted the matter. Nevertheless, all evidence as to that rotation had been indirect, and not until Foucault's experiment could the earth's rotation actually be said to have been demonstrated rather that deduced."" ""Continuing to experiment on the mechanics of the earth's rotation, Foucault in 1852 invented the gyroscope, which, he showed, gave a clearer demonstration than the pendulum of the earth's rotation and had the property, similar to that of the magnetic needle, of maintaining a fixed direction. Foucault's pendulum and gyroscope had more than a popular significance (which continues to this day). First, they stimulated the development of theoretical mechanics, making relative motion and the theories of the pendulum and the gyroscope standard topics for study and investigation. Second, prior to Foucault's demonstrations the study of those motions on the earth's surface in which the deflecting force of rotation plays a prominent part (especially winds and ocean currents) was dominated by unphysical notions of how this force acted. Foucault's demonstrations and the theoretical treatments they inspired showed conclusively that this deflecting force acts in all horizontal directions, thus providing the sound physical insight on which Buys Ballot, Ferrel, Ulrich Vettin, and others could build. (DSB).PMM: 330 lists the offprint with the title ""Sur Divers Signes Sensibles du Mouvement Diurne de la Terre"" - Barchas Collection, 738 (the periodical version, but only the first paper) - Dibner, No. 17 (offprint version).
(London, Taylor and Francis, 1856). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1856 - Vol. 146 - Part I. Pp. 297-342 a. pp. 343-355. Clean and fine.
First printing of the paper in which Airy describes his remarkable experiments aiming at finding the density of the earth. His approach to the problem was to determine the differences of gravity at the top as well at the bottom of a suitable deep mine.""One of the most remarkable of Airy's researches was his determination of the mean density of the Earth. In 1826, the idea occurred to him of attacking this problem by means of pendulum experiments at the top and bottom of a deep mine. His first attempt, made in the same year, at the Dolcoath mine in Cornwall, failed in consequence of an accident to one of the pendulums. A second attempt in 1828 was defeated by a flooding of the mine, and many years elapsed before another opportunity presented itself. The experiments eventually took place at the Harton pit near South Shields in 1854. Their immediate result was to show that gravity at the bottom of the mine exceeded that at the top by 1/19286 of its amount, the depth being 383 m (1,256 ft) From this he was led to the final value of Earth's specific density of 6.566.[This value, although considerably in excess of that previously found by different methods, was held by Airy, from the care and completeness with which the observations were carried out and discussed, to be ""entitled to compete with the others on, at least, equal terms."" (The currently accepted value for Earth's density is 5.5153 g/cm.). (Wikipedia).
"CAVENDISH, HENRY. - WEIGHING THE WORLD - THE MOST IMPORTENT ADDITION TO GRAVITATION THEORY SINCE NEWTON.
Reference : 43865
(1799)
Halle, Rengerschen Buchhandlung, 1799. Without wrappers. In ""Annalen der Physik. Herausgegeben von Ludwig Wilhelm Gilbert"", Bd. 2, Erstes Stück. (The entire issue offered). Titlepage to vol. 2. Pp. 1-118 a. 2 folded engraved plates. Cavendish's paper: pp. 1-62. (the torsion balance of Michell shown on the plates).
First German edition of Cavendish's famous paper in which he calculated the weight of the earth and determined its mass. He also, as the first, observed gravitational motion of minute portions of matter. He estimates the earth's mass to 6,6 x 10 to the potential of 24 kg. The original paper ""Experiments to determine the Density of the Earth"" appeared in Philosophical Transaction, 1798.""Cavendish published five papers between 1784 and 1809...With one exception they were comparatively minor productions....The exception was his determination of the density of the earth or weighing of the world in 1798, by means of John Michell's torsion balance. The apparatus consisted of two lead balls on either end of a suspended beam" these movable balls were attracted by a pair of stationary lead balls. Cavendish calculated the the force of attraction between the balls fro the observed period of oscillation of the balance and deduced the density of the earth from the force. He found it to be 5.48 times that of water. Cavendish was the first to observe gravitational motions induced by comparatively minute portions of ordinary matter...By weighing the world he rendered the law of gravitation complete. The law was no longer a proportionally statement but a quantitatively exact one" this was the most importent addition to the science of gravitation since Newton.""(DSB III, p. 158.).
"CAVENDISH, HENRY. - WEIGHING THE WORLD - THE MOST IMPORTENT ADDITION TO GRAVITATION THEORY SINCE NEWTON.
Reference : 48206
(1799)
(Halle, Rengerschen Buchhandlung, 1799). Without wrappers. In ""Annalen der Physik. Herausgegeben von Ludwig Wilhelm Gilbert"", Bd. 2, Erstes Stück. (The entire issue offered). 1-118 a. 2 folded engraved plates. Cavendish's paper: pp. 1-62. (the torsion balance of Michell shown on the plates).
First German edition of Cavendish's famous paper in which he calculated the weight of the earth and determined its mass. He also, as the first, observed gravitational motion of minute portions of matter. He estimates the earth's mass to 6,6 x 10 to the potential of 24 kg. The original paper ""Experiments to determine the Density of the Earth"" appeared in Philosophical Transaction, 1798.""Cavendish published five papers between 1784 and 1809...With one exception they were comparatively minor productions....The exception was his determination of the density of the earth or weighing of the world in 1798, by means of John Michell's torsion balance. The apparatus consisted of two lead balls on either end of a suspended beam" these movable balls were attracted by a pair of stationary lead balls. Cavendish calculated the the force of attraction between the balls fro the observed period of oscillation of the balance and deduced the density of the earth from the force. He found it to be 5.48 times that of water. Cavendish was the first to observe gravitational motions induced by comparatively minute portions of ordinary matter...By weighing the world he rendered the law of gravitation complete. The law was no longer a proportionally statement but a quantitatively exact one" this was the most importent addition to the science of gravitation since Newton.""(DSB III, p. 158.).The issue contains further papers by Ritter, Chladni et al.