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VIII.

2. Palacoma Colvini, Salter, op. cit. p. 328 (loc, same as foregoing sp.).
cygnipes, Salter, op. cit. p. 329

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(Bdellacoma) vermiformis, Salter, op. cit. p. 329 (loc. ibid.).
(Rhopalocoma) pyrotechnica, Salter, op. cit.

ditto.

spinosa, Billings, Trenton Limestone. Montmorency Falls, Canada
East.

Palæodiscus feror, Salter, 1857, op. cit. p. 333, pl. ix. fig. 6. Lower Ludlow
Rock, Leintwardine.

IX. Petraster bellulus, Troost, Niagara Group, Grimsby, Canada West.

X. 1. Protaster Miltoni, Salter, 1857. op. cit. pl. ix. fig. 4. Lower Ludlow, Leintwardine, etc.

XI.

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leptosoma, Salter, 1857, op. cit. pl. ix. fig. 5 (locality ibid.).
Sedgwickii, Forbes, 1849, Mem. Geol. Surv. Decade í, pl. iv.
Ludlow Rocks, Underbarrow, Kendal, Westmoreland.

Salteri, Sowerby, 1845, Quart. Journ. Geol. Soc., vol. i. p. 20.
Lower Silurian Cerrig-y-Druidion.

Forbesi, Hall, Upper Silurian, Herkimer Co., New York.
Ptilonaster princeps, Hall, 1866. 20th Report, p. 12, pl. ix. fig 9. Chemung
Group, Cortlandville.

XII. 1. Stenaster Salteri. Billings, Geol. Surv., Canada, Org. Rems. Decade iii. p. 78, pl. x. fig. 1. Trenton Limestone, Belville. Canada West. Huxleyi, Billings, Quebec Group, Lower Silurian, Newfoundland. XIII. 1. Tæniaster spinosus, Billings, Canadian Organic Remains, Decade iii., pl. x., fig. 3, p. 81. Trenton Limestone; Falls of Montmorency. cylindricus, Billings, op. cit. pl. x., fig. 4, p. 81. Trenton Limestone, Ottawa City.

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Urasterella (Stenaster) pulchella, Billings, sp. Geol. Surv. Canada, Report 1856, p. 292. Hall, 20th Report on State Cabinet, 1866, p. 9. Trenton Limestone, Ottawa City, Canada West.

Giving a total of 14 genera and 49 species of Silurian Star-fishes, 18 of which are British and the others (with three exceptions only) are North American.

EXPLANATION OF PLATE VIII.

FIG. 1a. Eucladia Johnsoni, sp. nov. Upper Silurian, Sedgley, near Dudley. Drawn from the original specimen in the Cabinet of Henry Johnson, Esq., Dudley (natural size).

The Madreporiform plate enlarged three times natural size.

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II. ON THE PROBABLE SEAT OF VOLCANIC ACTION.

BY T. STERRY HUNT, LL.D., F.R.S.

HE igneous theory of the earth's crust, which supposes it to have been at one time a fused mass, and to still retain in its interior a great degree of heat, is now generally admitted. In order to explain the origin of eruptive rocks, the phenomena of volcanos, and the movements of the earth's crust, all of which are conceived by geologists to depend upon the internal heat of the earth, three principal hypotheses have been put forward. Of these the first supposes that in the cooling of the globe a solid crust of no great thickness was formed, which rests upon the still uncongealed nucleus. The second hypothesis, maintained by Hopkins and by Poulett Scrope, supposes solidification to have commenced at the centre of the liquid globe, and to have advanced towards the circumference. Before the last portions became solidified, there was produced, it is conceived, a condition of imperfect liquidity, preventing the sinking of the cooled and heavier particles, and giving rise to a superficial crust, from

which solidification would proceed downwards. There would thus be enclosed, between the inner and outer solid parts, a portion of uncongealed matter, which, according to Hopkins, may be supposed still to retain its liquid condition, and to be the seat of volcanic action, whether existing in isolated reservoirs or subterranean lakes; or whether, as suggested by Scrope, forming a continuous sheet surrounding the solid nucleus, whose existence is thus conciliated with the evident facts of a flexible crust, and of liquid ignited matters beneath.

Hopkins, in the discussion of this question, insisted upon the fact, established by his experiments, that pressure favors the solidification of matter, which, like rocks, pass in melting to a less dense condition, and hence concludes that the pressure existing at great depths must have induced solidification of the molten mass, at a temperature at which, under a less pressure, it would have remained liquid. Mr. Scrope has followed this up by the ingenious suggestion that the great pressure upon parts of the solid igneous mass may become relaxed from the effect of local movements of the earth's crust, causing portions of the solidified matter to pass immediately into the liquid state, thus giving rise to eruptive rocks in regions where all before was solid.'

Similar views have been put forward in a note by Rev. O. Fisher, and in an essay on the formation of mountain chains, by Mr. N. S. Shaler, in the proceedings of the Boston Society of Natural History, both of which appear in the GEOLOGICAL MAGAZINE for November last. As summed up by Mr. Shaler, the second hypothesis supposes that the earth "consists of an immense solid nucleus, a hardened outer crust, and an intermediate region of comparatively slight depth, in an imperfect state of igneous fusion." In this connection it is curious to remark that, as pointed out by Mr. J. Clifton Ward, in the same Magazine for December (page 581), Halley was led, from the study of terrestrial magnetism, to a similar hypothesis. He supposed the existence of two magnetic poles situated in the earth's outer crust, and two others in an interior mass, separated from the solid envelope by a fluid medium, and revolving, by a very small degree, slower than the outer crust. The same conclusion was subsequently adopted by Hanstein.

The formation of a solid layer at the surface of the viscid and nearly congealed mass of the cooling globe, as supposed by the advocates of the second hypothesis, is readily admissible. That this process should commence when the remaining envelope of liquid was yet so deep that the refrigeration from that time to the present

1 See Scrope on Volcanos, and also his communication to the GEOLOGICAL MAGAZINE for Dec., 1868.

2 The elevated temperature of the 'interior of the globe would probably offer no obstacle to the development of magnetism. In a recent experiment of M. Trève, communicated by M. Faye, to the French Academy of Sciences, it was found that molten cast iron when poured into a mould, surrounded by a helix which was traversed by an electric current, became a strong magnet when liquid at a temperature of 1300° C., and retained its magnetism while cooling (Comptes Rendus de l'Acad. des Sciences, Feb. 1869),

has not been sufficient for its entire solidification, is, however, not so probable. Such a crust on the cooling superficial layer would, from the contraction consequent on the further refrigeration of the liquid stratum beneath, become more or less depressed and corrugated, so that there would probably result, as I have elsewhere said, "an irregular diversified surface from the contraction of the congealing mass which at last formed a liquid bath of no great depth, surrounding the solid nucleus." Geological phenomena do not, however, in my opinion afford any evidence of the existence of yet unsolidified portions of the originally liquid material, but are more simply explained by the third hypothesis. This, like the last, supposes the existence of a solid nucleus, and of an outer crust, with an interposed layer of partially fluid matter, which is not, however, a still unsolidified portion of the once liquid globe, but consists of the outer part of the congealed primitive mass, disintegrated and modified by chemical and mechanical agencies, impregnated with water, and in a state of igneo-aqueous fusion.

The history of this view forms an interesting chapter in geology. As remarked by Humboldt, a notion that volcanic phenomena have their seat in the sedimentary formations, and are dependent on the combustion of organic substances, belongs to the infancy of geology. To this period belong the notions of Lémary and Breislak (Cosmos, v. 443; Otte's translation). Keferstein in his Naturgeschichte des Erdkörpers, published in 1834, maintained that all crystalline nonstratified rocks from granite to lava, are products of the transformation of sedimentary strata, in part very recent, and that there is no well-defined line to be drawn between Neptunian and volcanic rocks, since they pass into each other. Volcanic phenomena, according to him, have their origin not in an igneous fluid centre, nor in an oxydizing metallic nucleus (Davy, Daubeny), but in known sedimentary formations, where they are the result of a peculiar kind of fermentation, which crystallizes and arranges in new forms the elements of the sedimentary strata, with an evolution of heat as a result of the chemical process (Naturgeschichte, vol. i. p. 109; also Bull. Soc. Geol. de France [1], vol. vii. p. 197). In commenting upon these views (Am. Jour. Science, July, 1860), I have remarked that, by ignoring the incandescent nucleus as a source of heat, Keferstein has excluded the true exciting cause of the chemical changes which take place in the buried sediments. The notion of a subterranean combustion or fermentation as a source of heat is to be rejected as irrational.

A view identical with that of Keferstein, as to the seat of volcanic phenomena, was soon after put forth by Sir John Herschel in a letter to Sir Charles Lyell in 1836 (Proc. Geol. Soc. London, ii. 548). Starting from the suggestion of Scrope and Babbage, that the isothermal horizons in the earth's crust must rise as a consequence of the accumulation of sediments, he insisted that deeply buried strata will thus become crystallized by heat, and may eventually, with their included water, be raised to the melting point, by which process gases would be generated, and earthquakes and volcanic eruptions follow. At the same time the mechanical disturbance of

the equilibrium of pressure, consequent upon a transfer of sediments, while the yielding surface reposes on matters partly liquefied, will explain the movements of elevation and subsidence of the earth's crust. Herschel was probably ignorant of the extent to which his views had been anticipated by Keferstein; and the suggestions of the one and the other seemed to have passed unnoticed by geologists until, in March, 1858, I reproduced them in a paper read before the Canadian Institute (Toronto), being at that time acquainted with Herschel's letter, but not having met with the writings of Keferstein. I there considered the reaction which would take place under the influence of a high temperature in sediments permeated with water, and containing, besides silicious and aluminous matter, carbonates, sulphates, chloride, and carbonaceous substances. From these, it was shown, might be produced all the gaseous emanations of volcanic districts, while from aqueo-igneous fusion of the various admixtures might result the great variety of eruptive rocks. To quote the words of my paper just referred to: "We conceive that the earth's solid crust of anhydrous and primitive igneous rock is everywhere deeply concealed beneath its own ruins, which form a great mass of sedimentary strata, permeated by water. As heat from beneath invades these sediments, it produces in them that change which constitutes normal metamorphism. These rocks, at a sufficient depth, are necessarily in a state of igneo-aqueous fusion; and in the event of fracture in the overlying strata, may rise among them, taking the form of eruptive rocks. When the nature of the sediments is such as to generate great amounts of elastic fluids by their fusion, earthquakes and volcanic eruptions may result, and these other things being equal-will be most likely to occur under the more recent formation." (Canadian Journal, May 1858, vol. iii. p. 207.)

The same views are insisted upon in a paper "On Some Points in Chemical Geology" (Quart. Jour. Geol. Soc., London, Nov. 1859, vol. xv. page 594), and have since been repeatedly put forward by me with farther explanations as to what I have designated above the ruins of the crust of anhydrous and primitive igneous rock. This, it is conceived, must, by contraction in cooling, have become porous and permeable, for a considerable depth, to the waters afterwards precipitated upon its surface. In this way it was prepared alike for mechanical disintegration, and for the chemical action of the acids, which, as shown in the two papers just referred to, must have been present in the air and the waters of the time. It is, moreover, not improbable that a yet unsolidified sheet of molten matter may then have existed beneath the earth's crust, and may have intervened in the volcanic phenomena of that early period, contributing by its extravasation to swell the vast amount of mineral matter then brought within aqueous and atmospheric influences. The earth, air, and water thus made to react upon each other, constitute the first matter from which by mechanical and chemical transformations the whole mineral world known to us has been produced.

It is the lower portions of this great disintegrated and waterimpregnated mass which form, according to the present hypothesis,

the semi-liquid layer supposed to intervene between the outer solid crust and the inner solid and anhydrous nucleus. In order to obtain a correct notion of the condition of this mass, both in earlier and later times, two points must be especially considered, the relation of temperature to depth, and that of solubility to pressure. It being conceded that the increase of temperature in descending in the earth's crust is due to the transmission and escape of heat from the interior, Mr. Hopkins showed mathematically that there exists a constant proportion between the effect of internal heat at the surface and the rate at which the temperature increases in descending. Thus, at the present time, while the mean temperature at the earth's surface is augmented only about one-twentieth of a degree Fahrenheit, by the escape of heat from below, the increase is to be found to be equal to about one degree for each sixty feet in depth. If, however, we go back to a period in the history of our globe when the heat passing upwards through its crust was sufficient to raise the superficial temperature twenty times as much as at present, that is to say, one degree of Fahrenheit, the augmentation of heat in descending would be twenty times as great as now, or one degree for each three feet in depth (Geol. Journal, viii. 59). The conclusion is inevitable that a condition of things must have existed during long periods in the history of the cooling globe when the accumulation of comparatively thin layers of sediment would have been sufficient to give rise to all the phenomena of metamorphism, vulcanicity, and movements of the crust, whose origin Herschel has so well explained.

Coming, in the next place, to consider the influence of pressure upon the buried materials derived from the mechanical and chemical disintegration of the primitive crust, we find that by the pressure of heated water throughout them, they are placed under conditions very unlike those of the original cooling mass. While pressure raises the fusing point of such bodies as expand in passing into the liquid state, it depresses that point for those which like ice contract in becoming liquid. The same principle extends to that liquefaction which constitutes solution; where, as is with few exceptions the case, the process is attended with condensation or diminution of volume, pressure will, as shown by the experiments of Sorby, augment the solvent power of the liquid,' under the influence of the elevated temperature, and the great pressure which prevail at considerable depths. Sediments should, therefore, by the effect of the water which they contain, acquire a certain degree of liquidity, rendering not improbable the suggestion of Scheerer, that the presence of five or ten per cent. of water may suffice, at temperatures approaching redness, to give to a granitic mass a liquidity partaking at once of the character of an igneous and an aqueous fusion. The studies by Mr. Sorby of the cavities in crystals have led him to conclude that the constituents of granitic and trachytic rocks have crystallized in the presence of liquid water, under great pressure, at temperatures not above redness, and consequently very far below 1 Sorby, Bakerian Lecture, Royal Society, 1863.

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