A treatise on infinitesimal calculus, Volume 3The University Press, 1856 |
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Autres éditions - Tout afficher
A Treatise on Infinitesimal Calculus: Containing Differential and Integral ... Bartholomew Price Affichage du livre entier - 1856 |
A Treatise on Infinitesimal Calculus: Containing Differential and ..., Volume 3 Bartholomew Price Affichage du livre entier - 1856 |
A Treatise on Infinitesimal Calculus: Containing Differential and Integral ... Bartholomew Price Affichage du livre entier - 1856 |
Expressions et termes fréquents
accelerating force angle attracted particle axis balls body bounding surface catenary centre of gravity centrifugal force components confocal constant coordinate axes curve d2x dt2 determine direction displacement distance dt2 dt2 dx dy dz dy dx earth elastic force element ellipsoid equal equilibrium expressed velocity external particle finite forces acting given point Hence homogeneous horizontal impact impressed infinitesimal integrating investigate law of attraction length let us suppose line of action m₁ mass material particle matter molecules moment-centre momentum momentum-increment normal origin parallel perpendicular phænomena plane plate position pressures quantity r₁ radius resolved rest resultant shell space described sphere square straight line string theorem thickness and density tion unit varies directly varies inversely velo velocity vertical vertical strength vis viva weight αξ
Fréquemment cités
Page 5 - Admission to its sanctuary, and to the privileges and feelings of a- votary, is only to be gained by one means — sound and sufficient knowledge of mathematics, the great instrument of all exact inquiry, without which no man can ever make such advances in this or any other of the higher departments of science as can entitle him to form an independent opinion on any subject of discussion within their range.
Page 497 - When we contemplate the constituents of the planetary system from the point of view which this relation affords us, it is no longer mere analogy which strikes us — no longer a general resemblance among them, as individuals independent of each other, and circulating about the sun, each according to its own peculiar nature, and connected with it by its own peculiar tie. The resemblance is now perceived to be a true family likeness ; they are bound up in one chain — interwoven in one web of mutual...
Page 61 - ... 7, 6, and 9 pounds respectively at the points A, B, D, E, F; AB = 3 feet, BD = 6 feet, DE = 5 feet, EF = 4 feet. Find the magnitude of the resultant, and the distance of its point of application, G, from A. Ans. R — 42 pounds. AG = 8| feet.
Page 518 - ... the squares of the periodic times are as the cubes of the distances from the common centre, the centripetal forces will be inversely as the squares of the distances.
Page 415 - V (5) <7 which is the equation of a parabola with its axis vertical and the vertex the highest point of the curve. The distance, OB, between the point of projection and the point where the projectile strikes the horizontal plane is called the Range on the horizontal plane, and is the value of x when y = 0. Putting y = 0 in (3) of Art.
Page 497 - Of all the laws to which induction from pure observation has ever conducted man, this third law (as it is called) of Kepler may justly be regarded as the most remarkable, and the most pregnant with important consequences.
Page 243 - Every particle of matter in the universe attracts every other particle with a force that varies directly as the product of the masses of the particles and inversely as the square of the distance between them.
Page 499 - In this case, it is obvious that the plane of the circle of illumination would be perpendicular to a line drawn from the centre of the sun to the centre of the earth...
Page 429 - ... force between bodies as varying directly as their masses and inversely as the square of the distance between them; and would predict the elliptical planetary orbits that are in fact found in the solar system.
Page 254 - ... bodies is proportional to the product of their masses divided by the square of the distance between them.