Mechanism of the HeavensJ. Murray, 1831 - 621 pages |
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Page xx
... parallax . For it seems incredible that the species or rays of the celestial bodies can pass through the immense interval between them and us in an instant ; or that they do not even require some considerable portion of time . ' 6 6 As ...
... parallax . For it seems incredible that the species or rays of the celestial bodies can pass through the immense interval between them and us in an instant ; or that they do not even require some considerable portion of time . ' 6 6 As ...
Page xxv
... parallax of that object ; it evidently increases and decreases with the distance ; therefore the base must be very great indeed , to be visible at all from the celestial bodies . But the globe itself whose dimensions are ascertained by ...
... parallax of that object ; it evidently increases and decreases with the distance ; therefore the base must be very great indeed , to be visible at all from the celestial bodies . But the globe itself whose dimensions are ascertained by ...
Page xxviii
... parallax or angle at the moon can be measured , all the angles and one side are given ; whence the distance of the moon from the centre of the earth may be computed . The parallax of an object may be found , if two observers under the ...
... parallax or angle at the moon can be measured , all the angles and one side are given ; whence the distance of the moon from the centre of the earth may be computed . The parallax of an object may be found , if two observers under the ...
Page xxix
... parallax , the line described by the planet on his disc , and the duration of the transit , would be the same to all the inhabitants of the earth ; but as the sun is not so remote but that the semidiameter of the earth has a sensible ...
... parallax , the line described by the planet on his disc , and the duration of the transit , would be the same to all the inhabitants of the earth ; but as the sun is not so remote but that the semidiameter of the earth has a sensible ...
Page xxx
... parallax has been detected , even in the nearest of these remote suns . If a fixed star had the parallax of one second , its distance from the sun would be 20500000 millions of miles . At such a distance not only the terrestrial orbit ...
... parallax has been detected , even in the nearest of these remote suns . If a fixed star had the parallax of one second , its distance from the sun would be 20500000 millions of miles . At such a distance not only the terrestrial orbit ...
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Common terms and phrases
action angle appears arising assumed attraction axes axis becomes bodies cause centre of gravity changes co-ordinates coefficients computed consequently constant contain curve depending described determined differential direction distance disturbing earth eccentricity ecliptic effect elements epoch equal equation expression fixed fluid force functions give given greater hence inclination increase inequalities integral Jupiter Jupiter's known latitude longitude mass mean motion moon move nearly nodes observation obtained omitted orbit parallax particle periodic planets position preceding principal produce quantities radius ratio regard represented result revolve rotation satellites Saturn secular sine space square substituted supposed surface theory third tion true values variation varies vector velocity whence whole zero
Popular passages
Page xviii - ... that the mean longitude of the first satellite, minus three times that of the second, plus twice that of the third, is always equal to two right angles.
Page vii - His works, but trace, with precision, the operation of His laws, use the globe he inhabits as a base wherewith to measure the magnitude and distance of the sun and planets, and make the diameter of the earth's orbit the first step of a scale by which he may ascend to the starry firmament. Such pursuits, while they ennoble the mind, at the same time inculcate humility, by showing that there is a barrier which no energy, mental or physical, can ever enable us to pass: that, however profoundly we may...
Page xv - That day, as other solemn days, they spent In song and dance about the sacred hill ; Mystical dance, which yonder starry sphere Of planets, and of fix'd, in all her wheels Resembles nearest, mazes intricate, Eccentric, intervolved, yet regular Then most, when most irregular they seem ; And in their motions harmony divine So smooths her charming tones, that God's own ear Listens delighted.
Page xlix - An account of experiments for determining the length of the pendulum vibrating seconds in the latitude of London.
Page lxiv - Jupiter ; it then gradually diminished in splendor, and having exhibited all the variety of tints that indicate the changes of combustion, vanished sixteen months after its discovery, without altering its position. It is impossible to imagine anything more tremendous than a conflagration that could be visible at such a distance.
Page xiv - But, in the midst of all these vicissitudes, the length of the major axes and the mean motions of the planets remain permanently independent of secular changes. They are so connected by Kepler's law, of the squares of the periodic times being proportional to the cubes of the mean distances of the planets from the sun, that one cannot vary without affecting the other.
Page lxix - If the attraction of the sun for the огпtre of the earth, and of the hemisphere diametrically opposite to him, were diminished by a difficulty in penetrating the interposed matter, the tides would be more obviously affected. Its attraction is the same also, whatever the substances of the celestial bodies may be; for if the action of...
Page vi - is to inspire the love of truth, of wisdom, of beauty — especially of goodness, the highest beauty — and of that supreme and eternal Mind, which contains all truth and wisdom, all beauty and goodness. By the love or delightful contemplation and pursuit of these transcendent aims, for their own sake only, the mind of man is raised from low and perishable objects, and prepared for those high destinies which are appointed for all those who are capable of them.
Page xii - ... depends upon the velocity with which they were first propelled in space. Had that velocity been such as to make the planets move in orbits of unstable equilibrium, their mutual attractions might have changed them into parabolas, or even hyperbolas, so that the earth and planets might, ages ago, have been sweeping far from our sun through the abyss of space.
Page xxxvi - ... the waters back to their sources ; and thus again by removing matter to a greater distance from the centre, destroy the velocity generated by its previous approach ; so that the descent of the rivers does not affect the earth's rotation.
Bibliographic information
| Title | Mechanism of the Heavens |
| Author | Mary Somerville |
| Publisher | J. Murray, 1831 |
| Original from | Harvard University |
| Digitized | 17 Nov 2007 |
| Length | 621 pages |
| Export Citation | BiBTeX EndNote RefMan |