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    Chapter 22 - Page 2

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    the sun, once in twenty-four hours; the last to the
    oblique manner in which its rays struck this orb, in all places but near
    its centre.

    But the globe ought not to be made to move around the table with its axis
    perpendicular to its surface, or to the "plane of the earth's orbit." In
    point of fact, the earth is inclined to this plane, and the globe should
    be placed at a corresponding inclination. Let the globe be brought to the
    edge of the table, at its south side, and with its upper or north pole
    inclining to the sun, and then commence the circuit, taking care always to
    keep this north pole of the globe pointing in the same direction, or to
    keep the globe itself in what we have termed a fixed attitude. As one half
    of the globe must always be in light, and the other half in darkness, this
    inclination from the perpendicular will bring the circle of light some
    distance beyond the north pole, when the globe is due-south from the
    light, and will leave an equal space around the opposite pole without any
    light at all, or any light directly received. Now it is that what we have
    termed the _fixed attitude_ of the globe begins to tell. If the north pole
    inclined towards the orbit facing the rim of the table, the light would
    still cut the poles, the days and nights would still be equal, and there
    would be no changes in the seasons, though there would be a rival
    revolution of the globe, by causing it to turn once a year, shifting the
    poles end for end. The inclination being to the surface of the table, or
    to _the plane_ of the orbit, the phenomena that are known to exist are a
    consequence. Thus it is, that the change in the seasons is as much owing
    to the fixed attitude of the earth in space, as we have chosen to term its
    polar directions, as to the inclination of its axis. Neither would produce
    the phenomena without the assistance of the other, as our experiment with
    the table will show.

    Place, then, the globe at the south side of the rim of the table, with its
    axis inclining towards its surface, and its poles always pointing in the
    same general direction, not following the circuit of the orbit, and set it
    in motion towards the east, revolving rapidly on its axis as it moves.

    While directly south of the light, it would be found that the north pole
    would be illuminated, while no revolution on the axis would bring the
    south pole within the circle of the light. This is when a line drawn from
    the axis of the globe would cut the lamp, were the inclination brought as
    low as the surface of the table. Next set the globe in motion, following
    the rim of the table, and proceeding to the east or right hand, keeping
    its axis always looking in the same general direction, or in an attitude
    that would be parallel to a north
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