Recreations in Astronomy: With Directions for Practical Experiments and Telescopic WorkWarren, Henry White
Religion
Recreations in Astronomy: With Directions for Practical Experiments and Telescopic Work
Warren, Henry White
Astronomy
Apply the principle that attraction is in proportion to the mass,
and a man who weighs one hundred and fifty pounds on the earth
weighs three hundred and ninety-six on Jupiter, and only fifty-eight
on Mars; while on the Asteroids he could play with bowlders for
marbles, hurl hills like Milton's angels, leap into the fifth-story
windows with ease, tumble over precipices without harm, and go
around the little worlds in seven jumps.
[Illustration: Fig. 39.--Orbit of Earth, showing Parallelism of
Axis and Seasons.]
The seasons of a planet are caused by the inclination of its axis
to the plane of its orbit. In Fig. 39 the rotating earth is seen
at A, with its northern pole turning in constant sunlight, and
its southern pole in constant darkness; everywhere south of the
equator is more darkness than day, and hence winter. Passing on
to B, the world is seen illuminated equally on each side of the
equator. Every place has its twelve hours' darkness and light at
each revolution. But at C--the axis of the earth always preserving
the same direction--the northern pole is shrouded in continual
gloom. Every place [Page 105] north of the equator gets more
darkness than light, and hence winter.
The varying inclination of the axes of the different planets gives
a wonderful variety to their seasons. The sun is always nearly
over the equator of Jupiter, and every place has nearly its five
hours day and five hours night. The seasons of Earth, Mars, and
Saturn are so much alike, except in length, that no comment is
necessary. The ice-fields at either pole of Mars are observed to
enlarge and contract, according as it is winter or summer there.
Saturn's seasons are each seven and a half years long. The alternate
darkness and light at the poles is fifteen years long.
But the seasons of Venus present the greatest anomaly, if its assigned
inclination of axis (75°) can be relied on as correct, which is
doubtful. Its tropic zone extends nearly to the pole, and at the
same time the winter at the other pole reaches the equator. The
short period of this planet causes it to present the south pole to
the sun only one hundred and twelve days after it has been scorching
the one at the north. This gives two winters, springs, summers, and
autumns to the equator in two hundred and twenty-five days.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account