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HORROCKS, JEREMIAH (1619-1641)

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Originally appearing in Volume V13, Page 712 of the 1911 Encyclopedia Britannica.
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HORROCKS, See also:JEREMIAH (1619-1641) , See also:English astronomer, was See also:born in 1619 at Toxteth See also:Park, near See also:Liverpool His See also:family was poor, and the See also:register of See also:Emmanuel See also:College, See also:Cambridge, testifies to his entry as See also:sizar on the 18th of May 1632. Isolated in his scientific tastes, and painfully straitened in means, he those which have a schistose See also:character. The See also:andalusite may be See also:pink and is then often pleochroic in thin sections, or it may be See also:white with the See also:cross-shaped dark enclosures of the See also:matrix which are characteristic of chiastolite. See also:Sillimanite usually forms exceedingly See also:minute needles embedded in See also:quartz. In the rocks of this See also:group cordierite also occurs, not rarely, and may have the outlines of imperfect hexagonal prisms which are divided up into six sectors when seen in polarized See also:light. In See also:biotite hornfelses a faint striping may indicate the See also:original bedding of the unaltered See also:rock and corresponds to small changes in the nature of the sediment deposited. More commonly there is a distinct spotting, visible on the surfaces of the See also:hand specimens.. The spots are See also:round or elliptical, and may be paler or darker t han the See also:rest of the rock. In some cases they are See also:rich in See also:graphite or carbonaceous matters; in others they are full of See also:brown See also:mica; some spots consist of rather coarser grains of quartz than occur in the matrix. The frequency with which this feature reappears in the less altered slates and hornfelses is rather remarkable, especially as it seems certain that the spots are not always of the same nature or origin. " See also:Tourmaline hornfelses " are found sometimes near the margins of tourmaline granites; they are See also:black with small needles of See also:schorl which under the See also:microscope are dark brown and richly pleochroic. As the tourmaline contains See also:boron there must have been some permeation of vapours from the See also:granite into the''sediments.

Rocks of this group are often seen in the Cornish See also:

tin-See also:mining districts, especially near the lodes. A second See also:great group of hornfelses are the See also:talc-silicate-hornirises which arise from the thermal alteration of impure See also:lime-stones. The purer beds recrystallize as See also:marbles, but where there has been originally an admixture of See also:sand or See also:clay lime-bearing silicates are formed, such as See also:diopside, See also:epidote, See also:garnet, See also:sphene, See also:vesuvianite, See also:scapolite; with these See also:phlogopite, various felspars, See also:pyrites, quartz and actinolite often occur. These rocks are See also:fine-grained, and though often banded are tough and much harder than the original limestones. They are excessively variable in their mineralogical See also:composition, and very often alternate in thin seams with biotite See also:hornfels and indurated quartzites. When perfused with boric and fluoric vapours from the granite they may contain much See also:axinite, fluorite and See also:datolite, but the aluminous silicates (andalusite, &c.) are absent from these rocks. From diabases, basalts, andesites and other igneous rocks a third type of hornfels is produced. They consist essentially of See also:felspar with See also:hornblende (generally of brown See also:colour) and See also:pale See also:pyroxene. Sphene, biotite and See also:iron oxides are the other See also:common constituents, but these rocks show much variety of composition and structure. Where the original See also:mass was decomposed and contained See also:calcite, See also:zeolites, See also:chlorite and other secondary minerals either in See also:veins or in cavities, there are usually rounded a reas or irregular streaks containing a See also:suite of new minerals, which may resemble those of the talc silicate hornfelses above described. The original porphyritic, fluidal, vesicular or fragmental structures of the igneous rock are clearly visible in the less advanced stages of hornfelsing, but become less, evident as the alteration progresses. In some districts hornfelsed rocks occur which have acquired a schistose structure through shearing, and these See also:form transitions to See also:schists and gneisses which contain the same minerals as the hornfelses, but have a schistose instead of a hornfels structure.

Among these may be mentioned cordierite and sillimanite gneisses, andalusite and kyanite mica schists, and those schistose talc silicate rocks which are known as cipolins. That these are sediments which have undergone thermal alteration is generally admitted, but the exact conditions under which they were formed is not always clear. The essential features of hornfelsing are ascribed to the See also:

action of See also:heat, pressure and permeating vapours, regenerating a rock mass without the See also:production of See also:fusion (at least on a large See also:scale). It has been argued, however, that often there is extensive chemical See also:change owing to the introduction of See also:matter from the granite into the rocks surrounding it. The formation of new felspar in the hornfelses is pointed out as pursued amid innumerable difficulties his purpose of self-See also:education. His university career lasted three years, and on its termination he became a See also:tutor at Toxteth, devoting to astronomical observations his brief intervals of leisure. In 1636 he met with a congenial spirit in See also:William Crabtree, a See also:draper of See also:Broughton, near See also:Manchester; and encouraged by his See also:advice he exchanged the guidance of Philipp von Lansberg, a pretentious but in-accurate Belgian astronomer, for that of See also:Kepler. He now set himself to the revision of the Rudolphine Tables (published by Kepler in 1627), and in the progress of his task became convinced that a transit of See also:Venus overlooked by Kepler would nevertheless occur on the 24th of See also:November (O.S.) 1639. He was at this See also:time See also:curate of See also:Hoole, near See also:Preston, having recently taken orders in the See also:Church of See also:England, although, according to the received accounts, he had not attained the canonical See also:age. The 24th of November falling on a See also:Sunday, his clerical duties threatened fatally to clash with his astronomical observations; he was, however, released just in time to See also:witness the punctual verification of his forecast, and carefully noted the progress of the phenomenon during See also:half an See also:hour before sunset (3.15 to 3'45). This transit of Venus is remarkable as the first ever observed, that of 1631 predicted by Kepler having been invisible in western See also:Europe. Notwithstanding the See also:rude character of the apparatus at his disposal, Horrocks was enabled by his observation of it to introduce some important corrections into the elements of the See also:planet's See also:orbit, and to reduce to its exact value the received estimate of its apparent See also:diameter.

After a See also:

year spent at Hoole, he returned to Toxteth, and there, on the See also:eve of a See also:long-promised visit to his friend Crabtree, he died, on the 3rd of See also:January 1641, when only in his twenty-second year. To the inventive activity of the discoverer he had already See also:united the patient skill of the observer and the See also:practical sagacity of the experimentalist. Before he was twenty he had afforded a specimen of his See also:powers by an important contribution to the lunar theory. He first brought the revolutions of our See also:satellite within the domain of Kepler's See also:laws, pointing out that her apparent irregularities could be completely accounted for by supposing her to move in an See also:ellipse with a variable eccentricity and directly rotatory See also:major See also:axis, of which the See also:earth occupied one See also:focus. These precise conditions were afterwards demonstrated by See also:Newton to follow necessarily from the See also:law of See also:gravitation. In his speculations as to the See also:physical cause of the See also:celestial motions, his mind, though not wholly emancipated from the tyranny of gratuitous assumptions, was working steadily towards the light. He clearly perceived the significant See also:analogy between terrestrial gravity and the force exerted in the See also:solar See also:system, and by the ingenious See also:device of a circular pendulum illustrated the composite character of the planetary movements. He also reduced the solar See also:parallax to 14" (less than a See also:quarter of Kepler's estimate), corrected the See also:sun's semi-diameter to 15' 45", recommended decimal notation, and was the first to make tidal observations. Only a remnant of the papers See also:left by Horrocks was preserved by the care of William Crabtree. After his See also:death (which occurred soon after that of his friend) these were See also:purchased by Dr Worthington, of Cambridge; and from his hands the See also:treatise Venus in See also:sole visa passed into those of See also:Hevelius, and was published by him in 1662 with his own observations on a transit of See also:Mercury. The remaining fragments were, under the directions of the Royal Society, reduced by Dr See also:Wallis to a compact form, with the heading Astronomia Kepleriana defensa et promota, and published with numerous extracts from the letters of Horrocks to Crabtree, and a See also:sketch of the author's See also:life, in a See also:volume entitled Jeremiae Horroccii See also:opera posthuma (See also:London, 1672). A memoir of his life by the Rev.

See also:

Arundel] See also:Blount Whatton, prefixed to a See also:translation of the Venus in sole visa, appeared at London in 1859. For additional particulars, see J. E. See also:Bailey's See also:Palatine See also:Note-See also:Book, ii. 253. iii. 17; Bailey's " Writings of Horrocks and Crabtree " (from Notes and Queries, Dec. 2, 1882); Notes and Queries, 3rd See also:series, vol. v., 5th series, vols. ii., iv.; See also:Martin's Biographia philosophica, p. 271 (1764) ; R. Brickel, Transits of Venus, 1639–1874 (Preston, 1874); Astronomical Register, xii. 293; Hevelii, Mercurius in sole visus, pp. 116-140; S. See also:Rigaud's See also:Correspondence of Scientific Men; Th.

See also:

Birch, See also:History of the Royal Society, i. 386, 395, 470; See also:Sir E. Sherburne's See also:Sphere of M. See also:Manilius, p. 92 (1675); Sir J. A. See also:Picton's Memorials of Liverpool, ii. 561; M. Gregson's Fragments relative to the Duchy of See also:Lancaster, p. 166 (1817); Liverpool Repository, i. 570 (1826); Phil. Trans.

Abridged, ii. 12 (1809); C. See also:

Hutton's Phil. and Math. See also:Dictionary (1815); See also:Penny Cyclopaedia (De See also:Morgan); Nature, viii. 117, 137; J. B. J. See also:Delambre, Hist. de l'astronomie moderne, ii. 495; Hist. de l'astronomie au X VIII siecle, pp. 28, 61, 74; W. See also:Whewell, Hist. of the Inductive Sciences, i. 331; R.

See also:

Grant, Hist. of Physical See also:Astronomy, pp. 420, 545; J. Madler, Geschichte der Himmelskunde, i. 275; M. See also:Marie, Hist. See also:des Sciences, iv. 168, vi. 9o; J. C. Houzeau, Bibl. Astr. ii. 167. (A.

M.

End of Article: HORROCKS, JEREMIAH (1619-1641)

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