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1,080 words, including any schedule, &c. 168 Containing more than 1,080 words, 17. 108 And further, for every 1,080 words beyond the first 1,080, 1.

Almanack or Calendar for the year, or less, 18. If for more years, then for each year for which it will serve, 1s. Perpetual Almanack, 10s.

Calendars or perpetual almanacks, in bibles or prayer books, excepted.

Appraisement of estate, real or personal, in any case whatsoever, except appraisement by order of an admiralty court, amount not exceeding 501, 2s. 6d-Exceeding 50 to 1002, 5s.-Exceeding 1007. to 2007, 10s.-Exceeding 2001. to 500%, 15s- Exceeding 5007., 17.

Articles of Apprenticeship and Clerkship. Any profession or trade, &c. except attorneys and others specifically charged, where the premium does not amount to

1. s. d.

other officer, who shall act in any of the above capacities for any other emolument than the regular emolument of the office; when residing within the limits of the two-penny post in England, or within the have been admitted 3 years or upwards, city or shire of Edinburgh, and if he shall residing elsewhere, and admitted for 101. Or if not so long admitted, 51. When long admitted, 31. three years, or upwards, 67. Or if not so

Conveyance (whether grant, assignment, scription whatever) on the sale of any transfer, renunciation, or of any other delands, rents, or other property, real or personal, heritable or moveable, or of any the principal or only deed whereby such right, title, interest, &c. in the same; for property shall be granted or conveyed to or vested in the purchaser, &c.

Where the purchase-money (which shall be truly expressed therein) shall not amount to 50, 158.

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Where the total amount of the money secured, or to be ultimately recoverable, shall be uncertain, being for money to be hereafter advanced, or to become due on account current, 50%

Certificate to be taken out yearly by attornies, solicitors, or proctors, in England; and by writers to the signet, solicitors, agents, attornies, or procurators, in any of the courts in Scotland; notaries public in England and Scotland; and also by every sworn clerk, clerk in court, and

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Of East India stock, 1l. 10s.

Of stock of any other corporation, not otherwise charged under the head of mortgage or conveyance, 17. 108.

STRAW hat manufacture, is of very modern invention: it has, however, of late years afforded the means of support to a large class of our industrious poor, and of not a few in the middle ranks of life The manufacture requires but little capital, and the art is quickly required. Thirty or forty shillings are said to be sufficient for the purchase of the machines and materials for employing one hundred persons some length of time. The straw used is readily obtained, and, when properly sorted, it is cut at the joints, and the outer covering being removed, it is then ranged according to the different sizes, and made up into bundles of eight or ten inches in length, and about a foot in circumference. The bundles are then dipped in water, and shaken a little, so as not to retain much moisture; and then they are to be placed on their edges

in a box, which is sufficiently close to prevent the evaporation of the smoke. In the middle of the box is an earthen vessel, containing sulphur, which is set on fire, and the box covered over for several hours. The straws are next to be split, which operation is performed by a small machine, made chiefly of wood. When split, the straws are denominated splints, and of these each braider has a certain quantity, which they hold under the arm, and draw them out as wanted. The rules laid down are these: platters should be taught to use their second fingers and thumbs instead of the fore fingers, which are often required to assist in turning the splints, and very much facilitate the platting; and they should take care not to wet the splints too much. Each platter should have a small linen bag, and a piece of pasteboard to roll the plat round. When five yards are worked up, it is wound about a piece of board, fastened at the top with yarn, and kept there several days, to form it in a proper shape. Four of these parcels, or a score, is the measurement by which the plat is sold. When the straw it platted, it comes into the hand of the person who sews it together into the form of hats, bonnets, &c. of various shapes and sizes. These are then put on wooden blocks, for the purpose of hot pressing; and, to render them of a more delicate white, they are again exposed to the fumes of sulphur.

STURGEON, a species of the Acipenser genus is referred to, and being omitted in its place, we may briefly observe, that it is a very large fish, of eighteen or twenty feet long, an inhabitant of the northern seas, migrating during the early summer months into the larger rivers and Jakes, and returning to the sea again in autumn after having deposited its spawn. It is a fish of slow motion, and is easily ta ken: it is admired for the delicacy and firmness of the flesh From the roe is prepared the substance cailed caviar. In this country the sturgeon annually ascends rivers, but in no great quantities, and is occasionally taken in salmon nets. In its manner of breeding the sturgeon forms an exception among cartilaginous fishes, it being oviparous The sturgeon was a fish in high repute among the ancients, and was brought to table with much pomp, and ornamented with flowers, the slaves who carried it being likewise adorned with garlands, and accompanied with music. The flavour of the sturgeon is said to vary with the food on which it is chiefly fed; hence it is distinguished in

the North of Europe, into mackerel-sturgeon, herring-sturgeon, &c. See Shaw's "Zoology"

SUBSTANCES, simple. To this article references have been made, and it having been omitted in the alphabetical order, we must not pass it by here. In other cases we are grieved that haste or negligence should have required these additions and corrections; in this we have reason for different emotions, having, by the omission, an opportunity of stating some facts, and some results, which have not been made public more than two or three days.

In the language of modern chemistry, the term simple substances has a different signification from that attached to it in ancient philosophy. By elements, or simple substances, was formerly understood primary principles, which were essentially simple and indistructible, which, by modification of form, or by mutual combination, formed the different substances which compose the material world. Modern philosophy pursues a different mode of investigation: it analyses substances, and endeavours to decompose them, or separate them into their constituent parts, and when it arrives at any which it cannot decompose, and beyond which analysis cannot be carried, and whose properties can only be changed by causing them to combine with others, then such substances are denominated simple. This term does not imply their absolute simplicity, because new experiments, or new agents, may be able to reduce certain bodies that at present have not been decomposed into others that are more simple. Till very lately the fixed alkalies, the boracic, Auoric, and muriatic acids were reckoned among the simple substances: to these may be added the metals, the several earths, sulphur, phosphorus, and the diamond.

By the Voltaic battery, in the hands of Mr. Davy, Professor of Chemistry at the Royal Institution, many of these substances, which were deemed simple a few months since, have been decomposed. For his experiments on the alkalies, we refer to the articles ALKALI and POTASSIUM: and on Saturday last, Dec. 17th, he announced in his public lecture, that he had decomposed sulphur and phosphorus, the component parts of which are oxygen and hydrogen, and a metallic base; that charcoal he had found to consist of hydrogen and the carbonaceous principle, and that diamond was a compound of the carbonaceous principle and

1

oxygen; that he had succeeded in obtaining the metallic base of ammonia, which, when combined with mercury, in the proportion of only 6th part, rendered the mercury solid, and reduced the specific gravity from 13 to 3. The professor likewise informed his audience that he had decomposed the boracic and fluoric acids, and had enjoyed a glimpse of their metallic bases; and that he had fully ascertained, that lime, magnesia, strontites, and barytes, are compound bodies, each having a metallic substance as a base. Hence the number of simple substances, which, but a year ago, was estimated by Dr. Thomson at 38, is in a very short space of time considerably reduced. Chemistry, indeed, as a science, will probably undergo a complete renovation: the discoveries of Mr. Davy promise a total overthrow to the beautiful, and, as it was formerly deemed, simple, and almost perfect system of Lavoisier. The English professor assumes electricity as a general agent of decomposition; that different bodies are naturally in different electrical states; that by altering these states their affinities are altered. In justification of this theory, he has ascertained that oxygen, and all bodies containing an excess of oxygen, are naturally negative, and that all bodies containing an excess of inflammable principle are naturally positive. Should subsequent facts confirm this theory, it is highly probable that many other of the bodies, hitherto regarded as simple, will yield to the powers of his apparatus.

SUBSTANCES, imponderable, in chemistry, are, caloric, light, electricity, and galvanism; perhaps the identity of the two former may hereafter be discovered: and likewise that of the two latter more completely demonstrated. The common character that they all possess is, that of not being subject to the attraction of gravitation; at least their gravity has hitherto been incapable of appreciation, hence the term "imponderable." They possess the greatest subtility, or tenuity; they cannot easily be obtained in a sepa rate state of existence; they are observed only in states of combination, or in their rapid transition from one body to another. We can scarcely discover their specific affinities, or measure their force, and we are unable to trace their particular combinations, or consider them as essential constituent principles of any compound. They are moreover diffused over every kind of matter; at least caloric exists in all bodies, and probably also the electric

and galvanic agents. See Murray's Chemistry.

TELESIE, in mineralogy, a gem so named by Hauy, which answers to the perfect CORUNDUM and the SAPPHIRE : to these articles the reader might be referred without further addition, but hav ing directed him already to TELESIE from the article GEM, we shall, in this place, give Mr. Murray's description. It occurs in fragments, and is crystallized, the form of its crystals being the double threesided pyramid, the single six-sided pyramid, and the six-sided prism, variously modified by truncations and acuminations.. Its colours are numerous, blue, green, red, of numerous shades, and yellow or yellowish white, and sometimes more than one colour is present even in the same crystal. It is more or less transparent; its lustre is resplendent and vitreous; and it often presents a beautiful reflection of light, in the form of a star: the fracture is conchoidal, or imperfectly foliated: the hardness is inferior to that of the diamond, but superior to that of every other fossil, and not yielding to the file: the specific gravity is from 3.9 to 4.1.

TIME, equation of. The most usual and best measure of time that we have is a clock, regulated by the vibration of a pendulum. But with whatever accuracy a clock may be made, it must be subject to irregularities, as well from the imperfection of the workmanship, as from the expansion and contraction of the materi als by heat and cold, by which the length of the pendulum, and consequently the time of vibration, will vary. As no clock, therefore, can be depended upon for keeping time accurately, it is necessary that we should be able at any time to ascertain how much it is too fast or too slow, and at what rate it gains or loses. For this purpose it must be compared with some motion which is uniform, or of which, if it be not uniform, one can find the variation. The motions of the heavenly bodies have therefore been considered as most proper for the purpose. Now as the earth revolves uniformly about its axis, the apparent diurnal motion of the heavenly bodies about the axis must be uniform. If a clock, therefore, be adjusted to go 24 hours from the pas. sage of any fixed star over the meridian till it returns to it again, its rate of going may be determined by comparing it with the transit of any fixed star, and observing whether the interval continues to be 24 hours: if not, the difference shows how much it gains or loses in that time. A

clock thus adjusted is said to be adjusted time from the passage of a fixed star over to sidereal time, and all the sidereal days the meridian till it returns to it again. are equal. But all the solar days are not From these considerations it will be eviequal, that is, the intervals from the sun's dent, that if a clock be adjusted to go 24 leaving the meridian till it returns to it hours in a mean solar day, it will not conagain are not all equal; so that if a clock tinue to coincide with the sun, that is, to be adjusted to go 24 hours in one interval, show 12 when the sun comes to the merianother interval will be performed in dian, because the true solar days differ in more or less than 24 hours, and thus the length from a mean solar day; but the sun and the clock will not agree; that is, sun will pass the meridian, sometimes bethe clock will not continue to show 12 fore 12, and sometimes after 12, and this when the sun comes to the meridian. It difference is called the equation. A clock is found that the length of the solar day thus adjusted, is said to be adjusted to is equal to the time of the earth's rotation mean solar time. The time shown by the about its axis, together with the time of clock is called true or mean time; and describing an angle equal to the increase that shown by the sun is called apparent of the sun's right ascension in a true solar time: thus, when the sun comes to the day. Now if the sun moved, or appeared meridian, it is said to be 12 o'clock appato move, uniformly, and in the equator, rent time. Hence the time shown by the this increase would be always the same in sun-dial is apparent time; and therefore a the same time, and therefore the solar days dial will differ from a clock by how much would be all equal; but the sun moves, or the equation of time is on that day. appears to move, in the ecliptic; and, When, therefore, we set a clock or watch therefore, if its motions were uniform, by the dial, we must attend to what the equal arcs upon the ecliptic would not equation of time is upon that day by a tagive equal arcs upon the equator. But ble, such as that given below, and allow the apparent motion of the sun in the for it: thus, if the equation be 4 minutes, ecliptic is not uniform, and hence also as it is on new year's day, and the watch any arc upon the ecliptic, described in a or clock be faster than the sun; then the given time, is subject to a variation, and watch or clock must be made to show 4 consequently that on the equator is sub- minutes past 12 when the dial shows 12 ject to a variation. The increase then of precisely. On the 30th of April, when the the sun's right ascension in a true solar dial shows 12, the clock or watch, to be day varies, from two causes: first, because accurate, must want 3 mintes of that the ecliptic, in which the sun appears to hour, and so of the rest. In calculating move, is inclined to the equator; secondly, tables of the equation of time, for every because his motion in the ecliptic is not day in the year, the sun and clock are set uniform, therefore the length of a true together, when the sun is in his apogee, solar day is subject to a continual variation; and then they investigate the difference consequently, a clock which is adjusted to between the sun and the clock, for every go 24 hours for any one true solar day, day at noon, and insert them in a table, will not continue to show 12 when the stating, by means of the signs + and —, sun comes to the meridian, because the how much the clock is before or after the intervals by the clock will continue equal, if the clock be supposed accurate; but the intervals of the sun's apparent passage over the meridian are not equal.

:

As the sun appears to move through 360° of right ascension in about 365 days, therefore 365.25 : 1 day :: 360° 59′ 8′′ 2", the increase of right ascension in one day, if the increase were uniform; or it would be the increase in a mean solar day, that is, if the solar days were all equal; for they would be all equal, if the sun's right ascension increased uniformly. As the earth describes an angle of 360° 59′, about its axis in a mean solar day of 24 hours, and an angle of 360° in a sidereal day, we say, as 360° 59′ 8′ 2′′" : 360°:: 24h: 23h 56′ 4′′, the length of a sidereal day in mean solar time; or the VOL. XII.

sun.

The inclination of the equator to the ecliptic, upon which the equation of time partly depends, and the place of the sun's apogee, when the clock and sun set off together, being both subject to vary, the equation of time for the same days of the year will every year vary, and therefore it must, where great accuracy is required, be calculated for every year. Besides the time when the sun is in his apogee, there are three other times of the year when the clock and sun agree, or when mean and apparent time is the same, as will be seen in the following table, which is adapted to the second year after Bissextile, and will always be found within a few seconds of the truth, and, therefore, sufficiently accurate for all common purposes.

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