On the Connexion of the Physical Sciences |
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Page 8
The gravitation of matter , directed to a centre , and attracting directly as the mass and inversely · as the square of the distance , does not belong to it when considered in mass only ; particle acts on particle according to the same ...
The gravitation of matter , directed to a centre , and attracting directly as the mass and inversely · as the square of the distance , does not belong to it when considered in mass only ; particle acts on particle according to the same ...
Page 16
In consequence of these , the disturbed planet is sometimes drawn away from the sun , sometimes brought nearer to him ; at one time it is drawn above the plane of its orbit , at another time below it , according to the position of the ...
In consequence of these , the disturbed planet is sometimes drawn away from the sun , sometimes brought nearer to him ; at one time it is drawn above the plane of its orbit , at another time below it , according to the position of the ...
Page 40
... whence the three motions of the moon , with regard to the sun , to her perigee , and to her nodes , are continually accelerated , and their secular equations are as the numbers 1 , 4 , and 0.265 , or , according to the most recent ...
... whence the three motions of the moon , with regard to the sun , to her perigee , and to her nodes , are continually accelerated , and their secular equations are as the numbers 1 , 4 , and 0.265 , or , according to the most recent ...
Page 57
... fraction is called the compression of the earth , because , according as it is greater or less , the terrestrial ellipsoid is more or less flattened at the poles ; it does not differ much from that given by the lunar inequalities .
... fraction is called the compression of the earth , because , according as it is greater or less , the terrestrial ellipsoid is more or less flattened at the poles ; it does not differ much from that given by the lunar inequalities .
Page 63
... the line described by the planet in its passage over his disc appears to be nearer to his centre , or farther from it , according to the position of the observer ; so that the duration of the transit varies with the different points ...
... the line described by the planet in its passage over his disc appears to be nearer to his centre , or farther from it , according to the position of the observer ; so that the duration of the transit varies with the different points ...
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according action angle appears arising atmosphere attraction axis becomes bodies cause centre changes colours comet consequently continued currents density depends determined diameter diminishes direction distance disturbing earth ecliptic effect electricity equal equator existence experiments extent extremely fluid force give given glass gravitation greater heat height increase influence intensity kind known latitude length less light liquid magnetic mass matter mean measured meridian miles moon motion move nature nearly needle object observed occasions ocean opposite orbit particles passing period phenomena plane plate polarized poles position probably produce proved quantity rays reflected refraction remain rest result revolve rings rotation round satellites seen separated side similar solar solid sound space square stars substances surface temperature terrestrial theory tides tion transmitted undulations variation varies vibrations waves whole wire
Popular passages
Page 29 - ... 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 20 - In song and dance about the sacred Hill — Mystical dance, which yonder starry sphere Of planets and of fixed 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 21 - that must render the name for ever memorable in science, and revered by those who delight in the contemplation of whatever is excellent and sublime." After Newton's discovery of the mechanical laws of the elliptical orbits of the planets, La Grange's discovery of their periodical inequalities is, without doubt, the noblest truth in physical astronomy ; and, in respect of the doctrine of final causes, it may be regarded as the greatest of all.
Page 386 - 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 110 - D'Alembert, was the Precession of the equinoxes and the Nutation of the earth's axis, according to the theory of gravitation.
Page 310 - ... that is, in the plane which passes through the north and south magnetic poles. There are places where the magnetic meridian coincides with the terrestrial meridian ; in these a magnetic needle freely suspended, points to the true north, but if it be carried successively to different places on the earth's surface, its direction will deviate sometimes to the east and sometimes to the west of north. Lines drawn on the globe through all the places where the needle points due north and south, are...
Page 357 - Hence arises still further confirmation, if any were required, of the identity of common and voltaic electricity, and that the differences of intensity and quantity are quite sufficient to account for what were supposed to be their distinctive qualities.
Page 175 - ... follows, that the orange and green rays of the spectrum, though they cannot be decomposed by prismatic refraction, can be decomposed by absorption, and actually consist of two different colours possessing the same degree of refrangibility.
Page 51 - ... solid parts, by their cohesion, nearly destroy that part of the centrifugal force which gives the particles a tendency to accumulate at the equator, though not altogether ; otherwise the sea, by the superior mobility of its particles, would flow towards the equator and leave the poles dry. Besides, it is well known, that the continents at the equator are more elevated than they are in higher latitudes. It is also necessary for the equilibrium of the ocean, that its density should be less than...
Bibliographic information
| Title | On the Connexion of the Physical Sciences |
| Author | Mary Somerville |
| Publisher | J. Murray, 1834 |
| Original from | the New York Public Library |
| Digitized | 26 Jun 2006 |
| Length | 458 pages |
| Export Citation | BiBTeX EndNote RefMan |