Mass 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 (12)  |  Distance (4)  |  Energy (38)  |  Exception (2)  |  Gravity (34)  |  Illusion (6)  |  Importance (14)  |  Inertia (4)  |  Matter (61)  |  Observation (142)  |  Opinion (36)  |  Opinion (36)  |  Position (3)  |  Space (23)  |  Speculation (18)  |  Sun (37)  |  Sun (37)  |  Vibration (3)

But when we face the great questions about gravitation Does it require time? Is it polar to the 'outside of the universe' or to anything? Has it any reference to electricity? or does it stand on the very foundation of matter–mass or inertia? then we feel the need of tests, whether they be comets or nebulae or laboratory experiments or bold questions as to the truth of received opinions.
Letter to Michael Faraday, 9 Nov 1857. In P. M. Harman (ed.), The Scientific Letters and Papers of James Clerk Maxwell (1990), Vol. 1, 1846-1862, 551-2.
See also:  |  Comet (12)  |  Electricity (30)  |  Experiment (199)  |  Gravity (34)  |  Inertia (4)  |  Matter (61)  |  Nebula (3)  |  Question (45)  |  Test (12)  |  Time (55)  |  Universe (138)

The mass starts into a million suns;
Earths round each sun with quick explosions burst,
And second planets issue from the first.
[The first concept of a 'big bang' theory of the universe.]
The Botanic Garden (1789-1791, 1805), 12.
See also:  |  Big Bang (15)  |  Earth (93)  |  Explosion (4)  |  Planet (34)  |  Sun (37)

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 (37)  |  Astronomy (65)  |  Calculation (8)  |  Celestial (3)  |  Certainty (24)  |  Chance (33)  |  Complexity (18)  |  Difference (25)  |  Distance (4)  |  Event (15)  |  Honour (5)  |  Human Mind (4)  |  Ignorance (62)  |  Impossibility (3)  |  Instrument (8)  |  Intelligence (31)  |  Knowledge (330)  |  Law (134)  |  Mathematician (66)  |  Motion (24)  |  Nature (243)  |  Observation (142)  |  Phenomenon (25)  |  Position (3)  |  Prediction (10)  |  Probability (33)  |  Relation (5)  |  Simplicity (30)  |  Theory (179)  |  Time (55)  |  Uncertainty (10)  |  Universe (138)  |  Weakness (2)

The radius of space began at zero; the first stages of the expansion consisted of a rapid expansion determined by the mass of the initial atom, almost equal to the present mass of the universe. If this mass is sufficient, and the estimates which we can make indicate that this is indeed so, the initial expansion was able to permit the radius to exceed the value of the equilibrium radius. The expansion thus took place in three phases: a first period of rapid expansion in which the atom-universe was broken into atomic stars, a period of slowing-down, followed by a third period of accelerated expansion. It is doubtless in this third period that we find ourselves today, and the acceleration of space which followed the period of slow expansion could well be responsible for the separation of stars into extra-galactic nebulae.
'La formation des nebuleuses dans l'univers en expansion', Comptes Rendus (1933), 196, 903-4. Trans. Helge Kragh, Cosmology and Controversy: The Historical Development of Two Theories of the Universe (1996), 52.
See also:  |  Big Bang (15)  |  Expansion (3)  |  Origin Of The Universe (4)  |  Space (23)

[In the beginning, before creation] There was neither Aught nor Naught, no air nor sky beyond. ...
[There was only]
A self-supporting mass beneath, and energy above.
Who knows, who ever told, from whence this vast creation rose?
No gods had yet been born—who then can e'er the truth disclose?
Rigveda
In Rigveda. In John Robson, Hinduism and Its Relations to Christianity (1893), 17.
See also:  |  Air (25)  |  Big Bang (15)  |  Creation (46)  |  Energy (38)  |  Myth (14)  |  Sky (7)  |  Truth (241)  |  Universe (138)

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