The Chautauquan, Vol. 03, February 1883: A Monthly Magazine Devoted to the Promotion of True Culture.; Organ of the Chautauqua Literary and Scientific Circle.Chautauqua Literary and Scientific Circle
History
The Chautauquan, Vol. 03, February 1883: A Monthly Magazine Devoted to the Promotion of True Culture.; Organ of the Chautauqua Literary and Scientific Circle.
Chautauqua Literary and Scientific Circle
Chautauqua Institution -- Periodicals; Chautauqua Literary and Scientific Circle -- Periodicals
60. Q. What is all that we ordinarily see with the eye or telescope of
the sun? A. The shining surface called the photosphere on which the
cromosphere rests.
61. Q. What is the diameter of the photosphere, or the visible and
measurable part of the sun? A. Eight hundred and sixty thousand miles.
62. Q. How many globes like the earth would it require to measure the
sun’s diameter? A. One hundred and eight.
63. Q. What is the volume of the sun as compared with that of the
earth? A. It is 1,245,000 times greater.
64. Q. What is the density of the sun as compared with that of the
earth? A. It is only one-fourth as great.
65. Q. What is the mass of the sun as compared with that of all the
planets, asteroids, and satellites of the solar system put together?
A. It is seven hundred times as great.
66. Q. What are some of the opinions as to the surface of the sun? A.
That it is hot beyond all estimate is indubitable. Whether it is solid
or gaseous we are not sure.
67. Q. What on the surface of the sun have been objects of earnest and
almost hourly study on the part of eminent astronomers for years? A.
The spots.
68. Q. To what must the speed of the orbital revolution of the planets
be proportioned? A. To the distance from the sun.
69. Q. What is the orbital speed of Mercury, and what that of Neptune?
A. That of Mercury is about twenty-nine and a half miles in a second,
and that of Neptune about three and one-third miles a second, or nearly
nine times as slow.
70. Q. How do the periods of the axial revolution, which determine the
length of the day, vary with the four planets nearest the sun? A. They
vary only half an hour from that of the earth.
71. Q. In what time do Jupiter and Saturn revolve? A. In ten and ten
and a quarter hours respectively.
72. Q. What is the density of Jupiter and Saturn as compared with the
earth? A. That of Jupiter is about one-fourth and that of Saturn is
about one-eighth that of the earth.
73. Q. How much less is the polar diameter of Jupiter than the
equatorial? A. Five thousand miles.
74. Q. If we represent the sun by a globe two feet in diameter, how
could we represent the comparative size of the five planets nearest the
sun? A. Vulcan and Mercury by mustard seeds, Venus and Earth by peas,
and Mars by one half the size.
75. Q. How could the comparative size of the other planets be
represented? A. Asteroids, by the motes in a sunbeam; Jupiter, by a
small-sized orange; Saturn, by a smaller one; Uranus, by a cherry; and
Neptune, by one a little larger.
76. Q. Applying the principle that attraction is in proportion to the
mass, what would a man weighing one hundred and fifty pounds on the
earth weigh on Jupiter, and what on Mars? A. On Jupiter he would weigh
three hundred and ninety-six pounds, and on Mars only fifty-eight
pounds.
77. Q. How are the seasons of the planets caused? A. By the inclination
of its axis to the plane of its orbit.
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