Page images
PDF
EPUB
[ocr errors]

one-celled. There is only one species, viz. S. canadensis, Canadian sanguinaria, bloodwort, or puccoon: a native of the northern parts of America, where it grows plentifully in the woods; and in the spring, before the leaves of the trees come out, the surface of the ground is in many places covered with the flowers, which have some resemblance to our wood anemone; but they have short naked pedicels, each supporting one flower at top. Some of these flowers will have ten or twelve petals, so that they appear to have a double range of leaves, which has occasioned their being termed double flowers; but this is only accidental, the same roots in different years producing different flowers.

SANGUISORBA, in botany, a genus of the Tetrandria Monogynia class and order. Natural order of Miscellaneæ, Linnæus. Rosaceæ, Jussieu. Essential character: calyx two-leaved, inferior; corolla superior; germ between the calyx and corolla. There are three species with several varieties.

SANICULA, in botany, sanicle, a genus of the Pentandria Digynia class and order. Natural order of Umbellatæ, or Umbelli feræ. Essential character: umbels clus. tered, subcapitate; fruit rugged; flowers of the disk abortive. There are three species.

remains in India. The red sanders, though in less estimation, and less generally used, is sent by preference into Europe. This is the produce of a different tree, which is common on the coast of Coromandel. Some travellers confound it with the wood of Caliatour, which is used in dyeing.

The S. album, or white sanders, is brought from the East Indies, in billets about the thickness of a man's leg, of a pale-whitish colour. It is that part of the yellow sanders wood' which lies next the bark., Great part of it, as met with in the shops, has no smell or taste, nor any sensible quality that can recommend it to the notice of the physician.

The S. flavum, or yellow sanders, is the interior part of the wood of the same tree which furnishes the former, is of a pale yellowish colour, of a pleasant smell, and a bitterish aromatic taste, accompanied with an agreeable kind of pungency. This elegant wood might undoubtedly be applied to valuable medical purposes, though at present very rarely used. Distilled with water, it yields a fragrant essential oil, which thickens in the cold into the consistence of a balsam. Digested in pure spirit, it imparts a rich yellow tincture; which being committed to distillation, the spirit arises without bringing over any thing considerable of the flavour of the sanders. The residuum contains the virtues of six times its weight of the wood.

SANTOLINA, in botany, lavender-cotton, a genus of the Syngenesia Polygamia Equalis class and order. Natural order of Compositæ Discoideæ. Corymbiferæ, Jussieu. Essential character: calyx imbricate, hemispherical; down none; receptacle chaffy. There are six species, S. chamocyparisus, common lavender-cotton; grows and is much cultivated in English gardens. naturally in the southern parts of Europe, All the species are ornamental plants, and may be propagated by planting slips and cuttings in the spring.

SANTALUM, in botany, a genus of the Tetrandria Monogynia class and order. Natural order of Onagræ, Jussieu. Essen. tial character: calyx four-toothed; corolla four-petalled, with the petals growing on the calyx, besides four glands; berry inferior, one-seeded. There is only one species, riz. S. album, white and yellow sandal wood. This tree has the appearance of a myrtle, with stiff branchiate branches, jointed; in habit, leaves and inflorescence resembling the privet. It is a native of many parts of India. In the Circar mountains, where it is wild, it is of little value, as it is generally of a small stature. On the Malabar coast it is very large, and the wood of the best kind. The difference of colour constitutes two kinds of sanders, both employed for the same purposes, and having equally a bitter taste, and an aromatic smell. With the powder of this wood a paste is prepared, with which the Chinese, Indians, Persians, Arabians, and Turks, anoint their SAP, or SAPP, in the art of war, is the bodies. It is likewise burnt in their houses, digging deep under the earth of the glacis, and yields a fragrant and wholesome smell. in order to open a covered passage into the The greatest quantity of this wood, to which moat. It is only a deep trench, covered at a sharp and attenuating virtue is ascribed, top with boards, hurdles, earth, sand-bags,

SAP. See PLANT.

The sap of trees, chemically considered, is a watery mucilaginous liquid,often strongly saccharine, so as to yield a large quantity of sugar, and to furnish a very strong fermented liquor.

J

[blocks in formation]

SAPINDUS, in botany, soap-berry-tree, a genus of the Octandria Trigynia class and order. Natural order of Tribilatæ. Sapindi, Jussieu. Essential character: calyx four-leaved; petals four; capsule fleshy, connate, ventricose. There are thirteen species; ; of which we shall notice the S. saponaria, with winged leaves, which grows naturally in the islands of the West Indies, where it rises with a woody stalk from 20 to 30 feet high, sending out many branches with winged leaves, composed of several pair of spearshaped lobes. The flowers are produced in loose spikes at the end of the branches; they are small and white, so make no great appearance. These are succeeded by oval berries as large as middling cherries, sometimes single, at others, two, three, or four are joined together; these have a saponaceous skin or cover, which incloses a very smooth roundish nut of the same form, of a shining black when ripe. The skin, or pulp, which surrounds the nuts, is used in America to wash linen; but it is very apt to burn and destroy it if often used, being of a very acrid nature.

SAPONARIA, in botany, soup-wort, a genus of the Decandria Digynia class and order. Natural order of Caryophyllei. Caryophylleæ, Jussieu. Essential character calyx one-leafed, naked; petals five, clawed; capsule oblong, one-celled. There are nine species. S. officinalis, a British plant, has a creeping root, so that in a short time it would fill a large space of ground. The stalks are above two feet high, and of a purplish colour. The foot-stalks of the flowers arise from the wings of the leaves opposite; they sustain four, five, or more purple flowers each, which have generally two small leaves placed under them. The

stalk is also terminated by a loose bunch of flowers growing in form of an umbel; they have each a large swelling cylindrical em. palement, and five broad obtuse petals, which spread open, of a purple colour. These are succeeded by oval capsules, with one cell filled with small seeds. The decoction of this plant is used to cleanse and scour woollen cloths: the poor people in some countries use it instead of soap for washing; from which use it had its name.

SAPPHIRE. See CORUNDUM, where we have given the analysis of the blue corundum, or sapphire. It is infusible without addition before the blow-pipe, but with borax it melts with effervescence. Sapphire, and oriental ruby, of which an analysis is also given in the article CORUNDUM, are next to the diamond, the most valuable of precious stones, and are used in the finest kind of jewelry. The oriental ruby differs from the sapphire in its colour: it is also softer and of less specific gravity. In its geognostic character, it differs also from the ruby, as it occurs sometimes imbedded in corundum, which is an inmate of primitive mountains, while sapphire appears to be a production of a later period. The violet coloured sapphire is the oriental amethyst: the yellow, the oriental chrysolite and topaz; and the green, the oriental emerald.

SARACA, in botany, a genus of the Diadelphia Hexandria class and order. Natural order of Lomentaceæ. Essential character: calyx none; corolla funnelform, four-cleft; filaments three on each side the throat; legume pedicelled. There is but one species, viz. S. indica, a native of the East Indies.

SARCOCOL, in chemistry, a gum resin, supposed to be the product of the penæa sarcocolla. It is brought from Persia and Arabia, in the form of small grains; they have sweet and bitterish taste, and are very soluble in water.

SARMENTACACEAE, in botany, the name of the eleventh class in Linnæus's Fragments of a Natural Method, consisting of plants that have climbing stems and branches, which like the vine attach them. selves to the bodies in their neighbourhood for the purpose of support.

SAROTHRA, in botany, a genus of the Pentandria Trigynia class and order. Natural order of Rotaceæ. Caryophylleæ, Jussieu. Essential character: calyx, five parted; corolla five petalled; capsule onecelled, three-valved, coloured. There is but one species, viz. S. gentianoides an an

ported in large straight blocks: it is said to be warm, aperient, and corroborant; and frequently employed, with good suc

nual plant, and a native of Virginia and Pennsylvania, growing abundantly in the fields, and under the bushes, in a dry sandy ground, near the capital of the latter process, for purifying the blood, for which purvince.

SARRACENIA in botany, side-saddle flower, so named in honour of Dr. Sarrazin, professor of botany, a genus of the Polyandria Monogynia class and order. Natural order of Succulenta. Essential character: calyx double, three-leaved, and five-leaved; corolla, five-petalled; capsule, five-celled, with the style having a clypeate stigma. There are four species, all natives of North America.

SARSAPARILLA, in pharmacy, the root of the rough smilax of Peru, consisting of a great number of long strings hanging from one head: these long roots, the only parts made use of, are about the thickness of a goose-quill, or thicker, flexible, and composed of fibres running their whole length: they have a bitterish but not ungrateful taste and no smell: and as to their medicinal virtues, they are sudorific and attenuant, and should be given in decoc. tion, or by way of diet-drink.

SASH, a mark of distinction, which in the British service is generally made of crimson silk for the officers, and of crimson mixed with white cotton for the serjeants. It is worn round the waist in inost regiments; in some few, particularly in the Highland corps, it is thrown across the shoulder. Sashes were originally invented for the convenience and ease of wounded officers, &c. by means of which, in case any of them were so badly wounded as to render them incapable of remaining at their posts, they might be carried off with the assistance of two men. They are now reduced to a very small size, and of course unfit for the original purpose. Both the sash and gorget, indeed, must be considered as mere marks of distinction, to point out officers on duty. In some instances they are worn together; in others, the gorget is laid aside, and the sash only worn. The British cavalry tie the sash on the right, the infantry on the left side. The sashes for the imperial army are made of crimson and gold, for the Prussian army black silk and silver, the Hanoverians yellow silk, the Portuguese crimson silk with blue tassels. The French have their sashes made of three colours, viz. white, pink, and light-blue, to correspond with the national flag.

SASSAFRAS, in pharmacy, the wood of an American tree, of the laurel-kind, imVOL. VI.

pose an infusion, in the way of tea, is a very pleasant drink: its oil is very fragrant, and possesses most of the virtues of the wood.

SATELLITES, in astronomy, are certain secondary planets, moving round the other planets, as the Moon does round the Earth. They are so called because they always attend them, and make the tour about the Sun together with them. The words moon and satellite are sometimes used indifferent ly: thus we say, either Jupiter's moons, or Jupiter's satellites; but usually we distinguish, restraining the term moon to the Earth's attendant, and applying the term satellite to the little moons more recently discovered about Jupiter, Saturn, and the Herschel planet, by the assistance of the telescope, which is necessary to render them visible.

The satellites move round their primary planets, as their centres, by the same laws as those primary ones do round their centre the Sun; viz. in such manner that, in the satellites of the same planet, the squares of the periodic times are proportional to the cubes of their distances from the primary planet.

SATELLITES of Jupiter, are four little moons, or secondary planets performing their revolutions about Jupiter, as that planet does about the Sun.

Simon Marius, mathematician of the Elector of Brandenburg, about the end of November 1609, observed three little stars moving round Jupiter's body, and proceeding along with him; and in January 1610, he found a fourth. In January 1610, Galileo also observed the same in Italy, and in the 1 same year published his observations. These satellites were also observed in the same month of January 1610, by Thomas Harriot, the author of a work upon algebra, and who made constant observations on these satellites, from that time till the 26th of February 1612.

When Jupiter comes into a line between any of his satellites and the Sun, the satellite disappears, being then eclipsed, or involved in his shadow. When the satellite goes behind the body of Jupiter, with respect to an observer on the Earth, it is then said to be occulted, being hidden from our sight by his body, whether in his shadow or not. And when the satellite comes into a posi tion between Jupiter and the Sun, it casts

с

a shadow upon the face of that planet, which we see as an obscure round spot. And lastly, when the satellite comes into a line between Jupiter and us, it is said to transit the disc of the planet, upon which it appears as a round black spot. The periods or revolutions of Jupiter's satellites, are found out from their conjunctions with that planet, after the same manner as those of the primary planets are discovered from their opposition to the Sun. And their distances from the body of Jupiter, are measured by a micrometer, and estimated in semi-diameters of that planet, and thence in miles. The periodical times and distances of these satellites, and the angles under which their orbits are seen from the Earth, at its mean distance from Jupiter, are as below.

[merged small][merged small][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][merged small]

Orbit.

and when the Sun is directly between Jupiter and the Earth, they are at their greatest distance asunder, the distance being more than before by the whole diameter of the Earth's annual orbit, or by double the Earth's distance from the Sun, then the eclipses are seen to happen the latest of any, and later than before by about a quarter of an hour. Hence therefore it follows, that light takes up a quarter of an hour in travelling across the orbit of the Earth, or nearly eight minutes in passing from the Sun to the Earth; which gives us about 12 millions of miles per minute, or 200,000 miles per second, for the velocity of light. A discovery that was first made by M. Roemer.

The third and greatest advantage derived from the eclipses of the satellites, is the knowledge of the longitudes of places on the Earth. Suppose two observers of an Angles of eclipse, the one, for example, at London, the other at the Canaries; it is certain that the eclipse will appear at the same moment to both observers; but as they are situated under different meridians, they count different hours, being perhaps 9 o'clock to the one, when it is only 8 to the other; by which observations of the true time of the eclipse, on communication, they find the difference of their longitudes to be one hour in time, which answers to 15 degrees of longitude.

266,000 3′ 55′′ 423,000 6 14 676,000 9 58 1,189,000 17 30

The eclipses of the satellites, especially of those of Jupiter, are of very great use in astronomy. First, iu determining pretty exactly the distance of Jupiter from the Earth. A second advantage still more considerable, which is drawn from these eclipses, is the proof which they give of the progressive motion of light. It is demonstrated by these eclipses, that light does not come to us in an instant, although its motion is extremely rapid. For if the motion of light were infinite, or came to us in an instant, it is evident that we should see the commencement of an eclipse of a satellite at the same moment, at whatever distance we might be from it; but, on the contrary, if light move progressively, then it is as evi dent, that the further we are from a planet, the later we shall be in seeing the moment of its eclipse, because the light will take up a longer time in arriving at us; and so it is found in fact to happen, the eclipses of these satellites appearing always later and later than the true computed times, as the Earth removes further and further from the planet. When Jupiter and the Earth are at their nearest distance, being in conjunction both on the same side of the Sun, then the eclipses are seen to happen the soonest ;

Saturn has seven secondary planets revolving about him. One of them, which till lately was reckoned the fourth in order from Saturn, was discovered by Huygens, the 25th of March, 1655, by means of a telescope 12 feet long; and the first, second, third, and fifth, at different times, by Cassini, viz. the fifth in October, 1671, by a telescope of 17 feet; the third in December, 1672, by a telescope of Campani's, 35 feet long; and the first and second in March, 1684, by help of Campani's glasses, of 100 and 136 feet. Finally, the sixth and seventh satellites were discovered by Dr. Herschel, with his 40 feet reflecting telescope, viz. the sixth on the 19th of August, 1787, and the seventh on the 17th of September, 1788. These two he has called the sixth and seventh satellites, though they are nearer to the planet Saturn than any of the former five, that the names or numbers of these might not be mistaken or confounded, with regard to former observations of them.

Moreover, the great distance between the fourth and fifth satellite, gave occasion

[blocks in formation]

The four first describe ellipses like to those of the ring, and are in the same plane. Their inclination to the ecliptic is from 30 to 31 degrees. The fifth describes an orbit inclined from 17 to 18 degrees with the orbit of Saturn; his plane lying between the ecliptic and those of the other satellites, &c. Dr. Herschel observes that the fifth satellite turns once round its axis exactly in the time in which it revolves about the planet Saturn; in which respect it resembles our Moon, which does the same thing. And he makes the angle of its distance from Saturn, at his mean distance, 17' 2". Philosophical Transactions, 1792, p. 22. a long account of observations of these satellites, with tables of their mean motions, by Dr. Herschel. Philosophical Transac tion, 1790.

See

The Herschel has six satellites, or moons, that revolve about him, like those of Jupiter and Saturn. These satellites were discovered by Dr. Herschel, who gave an ac count of them in the Philosophical Transactions.

SATIN, a glossy kind of silk stuff, the warp of which is very fine, and stands out so as to cover the coarser woof. Some satins are quite plain, others wrought; some flowered with gold or silver, and others striped, &c. The Chinese satins are most valued, because of their cleaning and bleaching easily, without losing any thing of

their lustre ; in other respects they are inferior to those of Europe.

SATINET, a slight thin kind of satin, commonly striped, and chiefly used by the ladies for summer night gowns.

SATURATION, in chemistry. As there are certain limits to the proportions in which bodies combine together, beyond which they cannot pass, these are called the points of saturation; and when two bodies, in uniting together, have reached this point, they are said to be saturated, or the one body is said to be saturated with the other; in other words, the change has taken place, and a new compound is formed. When, for instance, a salt is dissolved in water, as common salt, the water combines only with a certain proportion; and whatever quantity of salt is added beyond this proportion, it falls to the bottom undissolved. The reason of this is, that the particles of the salt are held together by their affinity for each other; that is, by the force of cohesion. Now, before any combination can be ef fected between the particles of the salt and the water, this force must be overcome. The force of affinity, therefore, between the water and the particles of salt, is greater than that between the particles of salt themselves, and thus they are separated and dissolve in the water; but this force of affinity between the water and the salt is li mited; and when it has arrived at its ut. most limit, the action between the two bodies ceases. The two forces which were opposed to each other; that is, the force of affinity between the water and the salt on the one hand, and the force of cohesion between the particles of the salt on the other, are balanced. The water in this case is said to be saturated with salt.

SATUREIA, in botany, savory, a genus of the Didynamia Gymnospermia class and order. Natural order of Verticillatæ. Labiatæ, Jussieu. Essential character: corolla with segments nearly equal; stamina distant. There are eight species, S. hortensis, or summer savory, is an annual plant, which grows naturally in the south of France and Italy, but is cultivated in this country both for the kitchen and medicinal The S. montana, or winter savory, a perennial plant, growing naturally in the south of France and Italy, but is cultivated in gardens both for culinary and medicinal purposes. Both kinds are propagated by seeds. Summer savory is a very warm pungent aromatie, and affords in distillation with water a subtile essential oil, of a

use.

« PreviousContinue »