# Perturbations Sentence Examples

- It has not indeed proved practically available; but his system of calculating cometary
**perturbations**by means of "mechanical quadratures" has formed the startingpoint of all subsequent researches on the subject. - The discordance of their results incited Laplace to a searching examination of the whole subject of planetary
**perturbations**, and his maiden effort was rewarded with a discovery which constituted, when developed and completely demonstrated by his own further labours and those of his illustrious rival Lagrange, the most important advance made in physical astronomy since the time of Newton. - Many of the symptoms of diseases were caused by the passions and
**perturbations**of the archeus, and medicines acted by modifying the ideas of the same archeus. - Thus it came about not only that classifications of disease based on superficial likeness - such as jaundice, dropsy, inflammation - were broken up, and their parts redistributed, but also that even more set diseases began to lose their settlements, and were recognized as terms of series, as transitory or culminating phases of
**perturbations**which might be traced to their origins, and in their earlier stages perhaps withstood. - This law has important ethical and political bearings; but in the province of disease this advance of what may be compared to the interlocking of points and signals has had wide influence not only in altering our conceptions of disease, but also in enlarging our views of all
**perturbations**of function. - Many other diseases formerly regarded as primarily diseases of the nervous system are not such; but, by means of agents either introduced into the body or modified there, establish themselves after the affinities of these in contiguous associated parts of the structure, as in vascular, membranous or connective elements, or again in distant and peripheral parts; the
**perturbations**of nervous function being secondary and consequential. - His researches into the
**perturbations**of Uranus and Neptune (Proc. Amer. - After a rough estimate of the
**perturbations**it must sustain from the attraction of the planets, he predicted its return for 1757,-a bold prediction at that time, but justified by the event, for the comet again made its appearance as was expected, though it did not pass through its perihelion till the month of March 1759, the attraction of Jupiter and Saturn having caused, as was computed by Clairault previously to its return, a retardation of 618 days. - The manuscript residue includes papers on atmospheric refraction (dated 1755), on the motion of Mars as affected by the
**perturbations**of Jupiter and the Earth (1756), and on terrestrial magnetism (1760 and 1762). - - When a simple periodic force acts on a system capable of oscillatory motion the ultimate forced vibration has a period equal to that of the impressed force, but the ultimate state is only reached theoretically after an infinite time, and if meanwhile the vibrating system suffers any
**perturbations**its free periods will at once assert themselves. - This is not inconsistent with the law of gravitation, for such estimates as have been made of planetary
**perturbations**due to stars give results which are insignificant in comparison with quantities at present measurable. - The
**perturbations**of the comets discovered, the one by H. - That entitled Developpemens sur diferents points de la theorie des
**perturbations**(1841), was translated in part xviii. - His first work on this abstruse subject, entitled T heorie des
**perturbations**de la lune, qui sont dues a faction des planetes,1 is remarkable for the boldness of its conception, and constitutes an important addition to celestial dynamics. - From the motion of the satellites he finds that the mass of Uranus is - T - A o o th of that of the sun, while for the planet Neptune he finds a mass equal to 19 Toth of the sun, agreeing with the value previously found by him from the
**perturbations**of Uranus within o th of its amount. - We have memoirs relating to the proof of the theorem that every numerical equation has a real or imaginary root, the memoir on the Hypergeometric Series, that on Interpolation, and the memoir Determinatio attractionis - in which a planetary mass is considered as distributed over its orbit according to the time in which each portion of the orbit is described, and the question (having an implied reference to the theory of secular
**perturbations**) is to find the attraction of such a ring. - He made some preliminary use of these expressions in 1817, in a paper on Kepler's Problem (Transactions Berlin Academy, 1816-1817, p. 49), and fully developed them seven years later, for the purposes of a research into planetary
**perturbations**(Ibid. - As practically attacked it consists in the problem of determining the
**perturbations**or disturbances in the motion of one of the bodies around the principal or central body, produced by the attraction of the third. - The sun is a small target for a meteorite coming from infinity to hit, and if this considerable quantity reaches its mark, a much greater amount will circulate round the sun in parabolas, and there is no evidence of it where it would certainly make itself felt, in
**perturbations**of the planets. - It was this: from the observed
**perturbations**of a known planet to deduce by calculation, assuming only Newton's law of gravitation, the mass and orbit of an unknown disturbing body. - Using a powerful and elaborate analysis, Adams ascertained that this cluster of meteors, which belongs to the solar system, traverses an elongated ellipse in 334 years, and is subject to definite
**perturbations**from the larger planets, Jupiter, Saturn and Uranus. - But when definitive results as to the orbits are required, it is necessary to compute the
**perturbations**produced by such of the major planets as have affected the motions of the body. - The principal modification is that,up to the present time, stellar astronomy has not advanced so far that a computation of the
**perturbations**in each case of a system of stars is either necessary or possible, except in exceptional cases. **Perturbations**of the Planets.- The problem of determining the
**perturbations**of the (2) Q heavenly bodies is perhaps the most complicated with which the mathematical astronomer has to grapple; and the forms under which it has to be studied are so numerous that they cannot be easily arranged under any one head. - The practical methods of computing
**perturbations**of the planets and satellites were first exhaustively developed by Pierre Simon Laplace in his Mecanique celeste. - The subject of planetary
**perturbations**was next attacked. - The prize of the Berlin Academy was, in 1780, adjudged to Lagrange for a treatise on the
**perturbations**of comets; and he contributed to the Berlin Memoirs, 1781-1784, a set of five elaborate papers, embodying and unifying his perfected methods and their results. - Among the fruits of the strenuous career of Nicolas Louis de Lacaille were tables of the sun, in which terms depending upon planetary
**perturbations**were, for the first time, introduced (1758); an extended acquaintance with the southern heavens; and a determination of the moon's parallax from observations made at opposite extremities of an arc of the meridian 85' in length. - The oscillation of the centre of power between Meath and Tir Eogain, according as the ardri belonged to the southern or northern Hy Neill, produced corresponding
**perturbations**in the balance of parties among the minor kings. - A research into the mutual
**perturbations**of Jupiter and Saturn secured for him the prize of the Berlin Academy in 1830, and a memoir on cometary disturbances was crowned by the Paris Academy in 1850. - An example of this process is that of the discovery of the planet Neptune: certain
**perturbations**of the orbit of Uranus had been observed, and it was seen that these could be explained on the hypothesis of the existence of a then unknown planet, and this hypothesis was verified by actual observation. - He shows that, supposing the cloud of particles to move around the sun in nearly circular orbits immediately outside the earth, the
**perturbations**by the earth in the motion of the particles will result in their retardation in that part of the orbit nearest the earth, and therefore in their always being more numerous in a given space in this part of the orbit Ethan in any other.