Arthur Eddington
Arthur Eddington
Sir Arthur Stanley Eddington OM FRSwas an English astronomer, physicist, and mathematician of the early 20th century who did his greatest work in astrophysics. He was also a philosopher of science and a popularizer of science. The Eddington limit, the natural limit to the luminosity of stars, or the radiation generated by accretion onto a compact object, is named in his honor...
NationalityBritish
ProfessionScientist
Date of Birth28 December 1882
facts accepting theory
Never accept a fact until it has been verified by theory.
statistics theory results
It is also a good rule not to put overmuch confidence in the observational results that are put forward until they are confirmed by theory.
knowledge theory amount
Something unknown is doing we don't know what-that is what our theory amounts to.
too-much theory results
Do not put too much confidence in experimental results until they have been confirmed by theory.
believe results theory
Don't believe the results of experiments until they're confirmed by theory.
against british-scientist collapse found second theory
If your theory is found to be against the second law of theromodynamics, I give you no hope; there is nothing for it but to collapse in deepest humiliation.
science thinking path
[When thinking about the new relativity and quantum theories] I have felt a homesickness for the paths of physical science where there are ore or less discernible handrails to keep us from the worst morasses of foolishness.
science bottles atoms
The electron, as it leaves the atom, crystallises out of Schrödinger's mist like a genie emerging from his bottle.
men quests physics
In Einstein's theory of relativity the observer is a man who sets out in quest of truth armed with a measuring-rod. In quantum theory he sets out with a sieve.
falling-in-love love-is men
Falling in love is one of the activities forbidden that tiresome person, the consistently reasonable man.
reality
The word reality frightens me.
stars hot enough
I am aware that many critics consider the conditions in the stars not sufficiently extreme . . . the stars are not hot enough. The critics lay themselves open to an obvious retort: we tell them to go and find a hotter place.
future years radio-waves
The universe will finally become a ball of radiation, becoming more and more rarified and passing into longer and longer wave-lengths. The longest waves of radiation are Hertzian waves of the kind used in broadcasting. About every 1500 million years this ball of radio waves will double in diameter; and it will go on expanding in geometrical progression for ever. Perhaps then I may describe the end of the physical world as-one stupendous broadcast.
science atoms levels
But it is necessary to insist more strongly than usual that what I am putting before you is a model-the Bohr model atom-because later I shall take you to a profounder level of representation in which the electron instead of being confined to a particular locality is distributed in a sort of probability haze all over the atom.