SUN                                                           I848                                    SUNDAY-SCHOOLS

command of the South Carolina troops, he had gained the rank of brigadier-general. At the close of the Revolutionary War he acted as a member of the South Carolina convention which ratified the Federal constitution, and for two periods (1789-93 and 1797-1801) was a member of the Federal house of representatives. During 1801-09 he served in the national senate, and during 1809-11 he was minister to Brazil. When he died, he was the last general officer of the Revolutionary era.

Sun, The, our nearest star and the central body of the solar system. For the inhabitants of the earth no other body in the heavens compares for an instant with the sun in interest and vital importance. For not only are the orbits of the earth and the other planets determined by the sun, but all forms of life on the earth immediately depend upon heat and light from the sun.

The distance of the sun from the earth is 92,897,000 miles, a stretch which baffles the imagination. Professor Young illustrates this quantity by saying that if a child were provided with an arm long enough to reach the sun and thus burn his hand, he would die of old age before he learned that he was burnt, assuming, as Helmholtz found, that sensations travel along the nerves at the rate of about 40 feet per second. Even light itself, traveling with the stupendous speed of 186,000 miles per second, requires 499 seconds for the trip from the sun to the earth.

The diameter of the sun is approximately 866,500 miles, a distance nearly twice as great as the diameter of the moon's orbit, while the mass is 1,332,000 times that of the earth, making its density about ij times that of water and the attraction of gravitation at the surface of the sun 27 times as great as at the surface of the earth. The weight of an ordinary man at the solar surface would, therefore, be such that he could not stand erect with his present strength of muscles.

The period of rotation of the sun was first determined after Galileo had discovered spots on the solar surface; and this rotation takes place in a very remarkable manner, for Carrington found that at the sun's equator spots travel once around the sun in 25 days, while at latitude 300 the period is 26Ì, days, and at latitude 400 is no less than 27 days. Hence the sun rotates most rapidly near the equator and diminishes constantly in angular speed as one approaches the poles. This fact has never been satisfactorily explained.

As to the constitution of the sun and as to the nature of sun-spots there are almost as many "theories" as there are men. What is reasonably certain, however, is that practically all of the elements which have been found in the eprth's crust are

to be found in the sun, making it highly probable that at some time the earth split off from the sun in the manner suggested by the nebular hypothesis. Concerning the interior of the sun practically nothing is known; for its temperature is outside the range of our experiments.

The white surface of the central body of the sun is called the photosphere. The spectroscope shows that this photosphere is surrounded by a layer of incandescent gases which we call the chromosphere. Certain parts of this chromosphere appear at times to be heaped up into brilliant clouds thousands and even hundreds of thousands of miles high; these are called prominences. Beyond the prominences and the chromosphere is a halo of light seen only at times of eclipse. It is called the corona, but beyond the mere fact that it is an appendage of the sun little is known about it. The fact, however, that its spectrum contains bright lines would seem to indicate that it consists partly, at least, of a self-luminous gas.

The best account of solar phenomena is to be found in Professor Young's delightful volume, The Sun, published in the International Scientific Series. See Astronomy and Planets.

Sun'bury, Perm., a borough, county-seat of Northumberland County, on Susquehanna River about 55 miles from Harrisburg. It is in a coal and lumbering region, and makes extensive coal-shipments. Its important manufacturing establishments are sash, door and nail factories, coffin and casket works, a rolling and a planing mill, silk-mills, dye-works and railroad-shops. Among its noteworthy buildings are Mary M. Packer Hospital, the county courthouse and municipal, buildings. East Sun-bury is just across a small stream. Though the towns have separate municipal governments, they are united in their industrial interests. Sunbury was settled in 1772 and incorporated in 1797. It has the service of the Pennsylvania and Reading railways. Population 13,770.

Sun'day=SchooIs are schools for religious instruction, meeting on Sunday. There were schools for religious instruction in connection with the Jewish synagogues and also among the early Christians. Luther established such schools in Germany, and Knox in Scotland. But the credit of founding the modern system of Sunday-schools belongs to Robert Raikes, who in 1780, when living in Gloucester, England, gathered the children from the streets on Sunday and hired teachers for them at 25 cents a day. These schools opened at 8 A. M., lasted until the children went to church, and after the second service began again, holding until 5 30 P. M. The children were taught their letters, reading and the church-catechism. The first Sunday-school in