St. Nicholas Magazine for Boys and Girls, Vol. 5, Nov 1877-Nov 1878 - No 1, Nov 1877 by Various
page 78 of 206 (37%)
page 78 of 206 (37%)
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On September 5 the earth and Mars came to the position shown at E and
M. You observe that they could not be much nearer. It is indeed very seldom that Mars is so well placed for observation. His illuminated face was turned toward the dark or night half of the earth, so that he shone brightly in the sky at midnight, and can be well studied with the telescope. When Galileo turned toward Mars the telescope with which he had discovered the moons of Jupiter, the crescent form of Venus, and many other wonders in the heavens, he was altogether disappointed. His telescope was indeed too small to show any features of interest in Mars, though the planet of war is much nearer to us than Jupiter. Mars is but a small world. The diameter of the planet is about 4,400 miles, that of our earth being nearly 8,000. Jupiter, though much farther away, has an immense diameter of more than 80,000 miles to make up, and much more than make up, for the effect of distance. With his noble system of moons he appears a remarkable object even with a small telescope, while Mars shows no feature of interest even with telescopes of considerable size. It was not, then, till very powerful telescopes had been constructed that astronomers learned what we now know about Mars.[4] [Footnote 4: See the "Moons of Mars" in "Letter Box" Department] It is found that his surface is divided into land and water, like the surface of our own earth. But his seas and oceans are not nearly so large compared with his continents and lands. You know that on our own earth the water covers so much larger a surface than the land that the great continents are in reality islands. Europe, Asia and Africa |
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