Distance Quotes (6)
Any opinion as to the form in which the energy of gravitation exists in space is of great importance, and whoever can make his opinion probable will have, made an enormous stride in physical speculation. The apparent universality of gravitation, and the equality of its effects on matter of all kinds are most remarkable facts, hitherto without exception; but they are purely experimental facts, liable to be corrected by a single observed exception. We cannot conceive of matter with negative inertia or mass; but we see no way of accounting for the proportionality of gravitation to mass by any legitimate method of demonstration. If we can see the tails of comets fly off in the direction opposed to the sun with an accelerated velocity, and if we believe these tails to be matter and not optical illusions or mere tracks of vibrating disturbance, then we must admit a force in that direction, and we may establish that it is caused by the sun if it always depends upon his position and distance.
Letter to William Huggins (13 Oct 1868). In P. M. Hannan (ed.), The Scientific Letters and Papers of James Clerk Maxwell (1995), Vol. 2, 1862-1873, 451-2.
See also: | Comet (14) | Energy (42) | Exception (4) | Gravity (41) | Illusion (7) | Importance (18) | Inertia (4) | Mass (8) | Matter (64) | Observation (147) | Opinion (40) | Opinion (40) | Position (3) | Space (25) | Speculation (21) | Sun (43) | Sun (43) | Vibration (5)
But in the heavens we discover by their light, and by their light alone, stars so distant from each other that no material thing can ever have passed from one to another; and yet this light, which is to us the sole evidence of the existence of these distant worlds, tells us also that each of them is built up of molecules of the same kinds as those which we find on earth. A molecule of hydrogen, for example, whether in Sirius or in Arcturus, executes its vibrations in precisely the same time. Each molecule, therefore, throughout the universe, bears impressed on it the stamp of a metric system as distinctly as does the metre of the Archives at Paris, or the double royal cubit of the Temple of Karnac ... the exact quantity of each molecule to all others of same kind gives it, as Sir John Herschel has well said, the essential character of a manufactured article and precludes the idea of its being external and self-existent.
'Molecules', 1873. In W. D. Niven (ed.), The Scientific Papers of James Clerk Maxwell (1890), Vol. 2, 375-6.
See also: | Character (11) | Earth (98) | Evidence (37) | Existence (54) | Sir John Herschel (13) | Hydrogen (14) | Kind (2) | Light (52) | Metric System (4) | Molecule (42) | Star (60) | Vibration (5)
In 1684 Dr Halley came to visit him at Cambridge, after they had been some time together, the Dr asked him what he thought the Curve would be that would be described by the Planets supposing the force of attraction towards the Sun to be reciprocal to the square of their distance from it. Sr Isaac replied immediately that it would be an Ellipsis, the Doctor struck with joy & amazement asked him how he knew it, why saith he I have calculated it, whereupon Dr Halley asked him for his calculation without any farther delay. Sr Isaac looked among his papers but could not find it, but he promised him to renew it, & then to send it him.
[Recollecting Newton's account of the meeting after which Halley prompted Newton to write The Principia. When asking Newton this question, Halley was aware, without revealing it to Newton that Robert Hooke had made this hypothesis of plantary motion a decade earlier.]
[Recollecting Newton's account of the meeting after which Halley prompted Newton to write The Principia. When asking Newton this question, Halley was aware, without revealing it to Newton that Robert Hooke had made this hypothesis of plantary motion a decade earlier.]
Quoted in Richard Westfall, Never at Rest: A Biography of Isaac Newton (1980), 403.
See also: | Amazement (2) | Attraction (7) | Calculation (13) | Curve (2) | Ellipse (2) | Force (26) | Gravity (41) | Edmond Halley (5) | Robert Hooke (15) | Joy (9) | Sir Isaac Newton (131) | Orbit (21) | Paper (10) | Planet (40) | Promise (3) | Search (12) | Square (3) | Sun (43)
The mountains too, at a distance, appear airy masses and smooth, but seen near at hand they are rough.
Diogenes Laertius, trans. Charles Duke Yonge, The Lives and Opinions of Eminent Philosophers (1901), 411.
The present state of the system of nature is evidently a consequence of what it was in the preceding moment, and if we conceive of an intelligence that at a given instant comprehends all the relations of the entities of this universe, it could state the respective position, motions, and general affects of all these entities at any time in the past or future. Physical astronomy, the branch of knowledge that does the greatest honor to the human mind, gives us an idea, albeit imperfect, of what such an intelligence would be. The simplicity of the law by which the celestial bodies move, and the relations of their masses and distances, permit analysis to follow their motions up to a certain point; and in order to determine the state of the system of these great bodies in past or future centuries, it suffices for the mathematician that their position and their velocity be given by observation for any moment in time. Man owes that advantage to the power of the instrument he employs, and to the small number of relations that it embraces in its calculations. But ignorance of the different causes involved in the production of events, as well as their complexity, taken together with the imperfection of analysis, prevents our reaching the same certainty about the vast majority of phenomena. Thus there are things that are uncertain for us, things more or less probable, and we seek to compensate for the impossibility of knowing them by determining their different degrees of likelihood. So it was that we owe to the weakness of the human mind one of the most delicate and ingenious of mathematical theories, the science of chance or probability.
'Recherches, 1º, sur l'Intégration des Équations Différentielles aux Différences Finies, et sur leur Usage dans la Théorie des Hasards' (1773, published 1776). In Oeuvres complètes de Laplace, 14 Vols. (1843-1912), Vol. 8, 144-5, trans. Charles Coulston Gillispie, Pierre-Simon Laplace 1749-1827: A Life in Exact Science (1997), 26.
See also: | Analysis (39) | Astronomy (68) | Calculation (13) | Celestial (3) | Certainty (25) | Chance (40) | Complexity (22) | Difference (30) | Event (20) | Honour (9) | Human Mind (4) | Ignorance (63) | Impossibility (3) | Instrument (9) | Intelligence (34) | Knowledge (341) | Law (145) | Mass (8) | Mathematician (69) | Motion (31) | Nature (255) | Observation (147) | Phenomenon (35) | Position (3) | Prediction (11) | Probability (34) | Relation (9) | Simplicity (33) | Theory (192) | Time (57) | Uncertainty (11) | Universe (143) | Weakness (3)
Thus far I have explained the phenomena of the heavens and of our sea by the force of gravity, but I have not yet assigned a cause to gravity. Indeed, this force arises from some cause that penetrates as far as the centers of the sun and planets without any diminution of its power to act, and that acts not in proportion to the quantity of the surfaces of the particles on which it acts (as mechanical causes are wont to do) but in proportion to the quantity of solid matter, and whose action is extended everywhere to immense distances, always decreasing as the squares of the distances.
The Principia: Mathematical Principles of Natural Philosophy (1687), 3rd edition (1726), trans. I. B. Cohen and Anne Whitman (1999), General Scholium, 943.
See also: | Cause (54) | Centre (3) | Explanation (26) | Force (26) | Gravity (41) | Heaven (21) | Inverse Square Law (3) | Law Of Gravity (2) | Matter (64) | Mechanics (18) | Phenomenon (35) | Planet (40) | Proportion (10) | Sea (15) | Sun (43) | Surface (8)