DIVERSITIES OF THE PLANETS.

In illustration of the great diversity of the physical peculiarities

and probable condition of the planets, Sir John Herschel describes

the intensity of solar radiation as nearly seven times greater on

Mercury than on the earth, and on Uranus 330 times less; the proportion

between the two extremes being that of upwards of 2000 to 1. Let any

one figure to himself, (adds Sir John,) the condition of our globe

were the sun to be septupled, to say nothing of the greater ratio; or

were it diminished to a seventh, or to a 300th of its actual power!

Again, the intensity of gravity, or its efficacy in counteracting

muscular power and repressing animal activity, on Jupiter is nearly

two-and-a-half times that on the earth; on Mars not more than one-half;

on the moon one-sixth; and on the smaller planets probably not more

than one-twentieth; giving a scale of which the extremes are in the

proportion of sixty to one. Lastly, the density of Saturn hardly

exceeds one-eighth of the mean density of the earth, so that it must

consist of materials not much heavier than cork.

Jupiter is eleven times, Saturn ten times, Uranus five times, and

Neptune nearly six times, the diameter of our earth.

These four bodies revolve in space at such distances from the sun,

that if it were possible to start thence for each in succession,

and to travel at the railway speed of 33 miles per hour, the

traveller would reach

Jupiter in 1712 years

Saturn 3113 ”

Uranus 6226 ”

Neptune 9685 ”

If, therefore, a person had commenced his journey at the period of

the Christian era, he would now have to travel nearly 1300 years

before he would arrive at the planet Saturn; more than 4300 years

before he would reach Uranus; and no less than 7800 years before he

could reach the orbit of Neptune.

Yet the light which comes to us from these remote confines of the

solar system first issued from the sun, and is then reflected

from the surface of the planet. When the telescope is turned

towards Neptune, the observer’s eye sees the object by means of

light that issued from the sun eight hours before, and which

since then has passed nearly twice through that vast space which

railway speed would require almost a century of centuries to

accomplish.--_Bouvier’s Familiar Astronomy._

Curiosities of Science, Past and Present A Book for Old and Young · 第 172 / 469 题