SURFACE FEATURES

Seen through a telescope, Jupiter shows the loveliest variety of

colors, with the reddish ones always most conspicuous. The slightly

pink-tinted steady light that we get from the planet with the naked eye

in no way suggests the turbulent, flame-like aspect that a telescopic

view opens to us. The telescope also reveals very clearly that

flattening at the poles which has already been spoken of.

With so dense an atmosphere as Jupiter most likely has, it is sometimes

doubtful whether his surface can be seen by us at all. But it is

certain that we see something apparently much more dense and stable

than an atmosphere is supposed to be; and hence it is thought that, in

spite of its thickness, the atmosphere may be only partially opaque,

and that it may be in some places even more or less transparent.

It does not seem probable that the markings on Jupiter are wholly

atmospheric. Some of them indicate that the substance we see has

considerably more consistency than a mere gas. The whole surface of

the planet is covered with belts and spots of various colors and

varying shapes. The belted appearance is particularly marked. It has

been noticed for more than two hundred years, and can be seen with a

comparatively small telescope. Sometimes as many as twenty or thirty

belts have been seen at one time. All of them are parallel with the

equator.

Two broad red belts on each side of the equator, called the tropical

belts, are very distinct, and sometimes retain the same shape and

color for months at a time, though sometimes they change rapidly in

both color and outline. Between them is the equatorial belt, which

is also a semi-permanent feature, remaining often for a considerable

period unchanged. These belts, and the spots that sometimes appear on

and near them, have been closely watched, because about the equator,

and especially just south of it, is the region of greatest activity on

Jupiter’s surface.

One feature that more nearly suggests solidity and permanency than

anything else on Jupiter is the famous great red spot which lies in the

southern hemisphere just below the southern tropical belt. It appeared

about thirty-five years ago, in July, 1878, as a pale pink spot, grew

brighter for two or three years, and then faded, until, at the end of

two or three more years, it was almost invisible. In another year it

came again, and increased in brightness for five or six years. Then it

grew a little fainter, and has since remained a rather faint red spot,

but plainly visible.

In shape the great red spot is an immense oval as much as thirty

thousand miles from east to west and seven thousand miles from north

to south, which gives it a surface four or five times as large as the

land area on the entire earth, and larger even than the whole surface

of the earth including the oceans. Although retaining its own shape,

it seems to drift about among its surroundings, showing that it is not

attached to any solid surface; and yet it has a suggestion of solidity

in itself, which was shown when it and another smaller spot were seen

to be drifting toward each other, and then finally to meet. Instead of

colliding or going over or under, they calmly drifted to one side and

went around each other.

Appearances such as this have suggested the idea that the great spot

might be a continent in process of formation. Such an idea is at best a

speculation; but it would be interesting if it should prove that we are

witnessing on Jupiter the process through which our own earth must at

one time have passed when its crust began to solidify in patches, as

one of the steps in the long period of evolution which has prepared it

for our uses. It is not at all certain that Jupiter will ever be just

like the earth. The differences between its atmosphere and ours may

have some influence in its development that we have little knowledge

of at present, and there are some other fundamental differences

between the two planets which may in some way effect a difference in

development. But in a general way we know that the planet will in time

become more condensed than it now is and will finally solidify. Whether

the processes will be carried on in just the same way in which they

have been here on the earth is not so certain.

The Ways of the Planets · 第 80 / 101 题