THREE VIEWS OF AN ERUPTIVE PROMINENCE OF THE SUN.

From photographs taken at Kenwood Observatory, Chicago, March 25,

1895, and kindly loaned by Professor George E. Hale, of the Chicago

University.]

In the ordinary incandescent electric lamp, the brilliant light is

produced by a glowing filament of carbon. The powerful current of

electricity experiences so much resistance as it flows through this

badly conducting substance, that it raises the temperature of the

carbon wire so as to make it dazzlingly white-hot. Indeed the carbon

is thus elevated to a temperature far in excess of that which could

be obtained in any other way. The reason why carbon is employed in

the electric lamp, in preference to any other substance, may be easily

understood. Suppose we tried to employ an iron wire as the glowing

filament within the well-known glass globe. Then when the current was

turned on that iron would of course become red-hot and white-hot;

but ere a sufficient temperature had been attained to produce the

requisite illumination, the iron wire would have been fused into drops

of liquid, the current would have been broken, and the lamp would have

been destroyed. Nor would the attempt to make an incandescent lamp

have proved much more successful had the filament been made of

any other metal. The least fusible of metals is the costly element

platinum, but even a wire of platinum, though it would stand much

more heat than a wire of iron or of steel, would not have retained the

solid form by the time it had been raised to the temperature necessary

for an incandescent lamp.

There is no known metal, and perhaps no substance whatever, which

demands so high a temperature to fuse it as does the element carbon.

A filament of carbon, and a filament of carbon alone, will remain

unfused and unbroken when heated by the electric current to the

dazzling brilliance necessary for effective illumination. This is

the reason why this particular element is so indispensable for our

incandescent electric lamps. Modern research has now taught us that,

just as the electrician has to employ carbon as the immediate agent in

producing the brightest of artificial lights down here, so the sun in

heaven uses precisely the same element as the immediate agent in

the production of its transcendent light and heat. Owing to the

extraordinary fervor which prevails in the interior parts of the sun,

all substances there present, no matter how difficult we may find

their fusion, would have to submit to be melted, nay, even to be

driven off into vapor. If submitted to the heat of this appalling

solar furnace, an iron poker, for instance, would vanish into

invisible vapor. In the presence of the intense heat of the inner

parts of the sun, even carbon itself is unable to remain solid.

It would seem that it must assume a gaseous form under such

circumstances, just as the copper and the iron and all the other

substances do which yield more readily than it to the fierce heat of

their surroundings.

The buoyancy of carbon vapor is one of its most remarkable

characteristics. Accordingly immense volumes of the carbon steam

in the sun soar at a higher level than do the vapors of the other

elements. Thus carbon becomes a very large and important constituent

of the more elevated regions of the solar atmosphere. We can

understand what happens to these carbon vapors by the analogous case

of the familiar clouds in our own skies. It is true, no doubt, that

our terrestrial clouds are composed of a material totally different

from that which constitutes the solar clouds. The sun evaporates the

water from the great oceans which cover so large a proportion of our

earth. The vapor thus produced ascends in the form of invisible gas

through our atmosphere, until it reaches an altitude thousands of

feet above the surface of the earth. The chill that the watery vapor

experiences up there is so great that the vapor collects into little

liquid beads, and it is, of course, these liquid beads, associated in

countless myriads, which form the clouds we know so well.

We can now understand what happens as the buoyant carbon vapors

soar upwards through the sun's atmosphere. They attain at last to an

elevation where the fearful intensity of the solar heat has so

far abated that, though nearly all other elements may still remain

entirely gaseous, yet the exceptionally refractory carbon begins to

return to the liquid state. At the first stage in this return, the

carbon vapor conducts itself just as does the ascending watery vapor

from the earth when about to be transformed into a visible cloud.

Under the influence of a chill the carbon vapor collects into a myriad

host of little beads of liquid. Each of these drops of liquid carbon

in the glorious solar clouds has a temperature and a corresponding

radiance vastly exceeding that with which the filament glows in the

incandescent electric lamp. When we remember further that the entire

surface of our luminary is coated with these clouds, every particle

of which is thus intensely luminous, we need no longer wonder at that

dazzling brilliance which, even across the awful gulf of ninety-three

millions of miles, produces for us the indescribable glory of

daylight.

_Sir Robert Ball will contribute a series of articles on "The Marvels

of the Universe." Six or eight of these articles may be expected

during the coming year_.

[Illustration: THEOLOGICAL SEMINARY BUILDINGS, ANDOVER,

MASSACHUSETTS.]

McClure's Magazine, Vol. 6, No. 2, January, 1896 · 第 71 / 89 题