School educationMason, Charlotte M. (Charlotte Maria)
Philosophy
School education
Mason, Charlotte M. (Charlotte Maria)
Education -- Curricula; Education -- Philosophy
There is no continuous range in the Scandinavian mountains; the
whole is a high table-land, which increases in height as we go
south, with here and there groups of peaks which appear like
huge rocks dotted over the surface. These plateaux are topped
with moors or snowfields from which glaciers descend right down
into the sea.
7. How does the position of the mountains affect the rivers? Compare the
rivers of Norway with those of Sweden.
NOTE.
Describe how, in Norway, the rivers rush in torrents over
their rocky beds, while those in Sweden flow more gently
down the gradual slope of the land. Give the threefold
reason—great rainfall, small evaporation owing to the coldness
of the climate, and small waste owing to the hardness of
the rocks—for the great volume of water in the short, quick,
Norwegian rivers.
8. Recapitulate with blank map, the girls adding descriptive notes as
they answer the map questions.
_Subject: Astronomy._
Group: Science. Class IV. Age: 16.
Time: 30 minutes.
OBJECTS.
1. To interest the pupils in studying the heavens for themselves.
2. To show where the planets may be looked for and how they may be
recognised.
3. To help the pupils to apply their theoretical knowledge of the planets
to explain the movements they can observe with the naked eye.
4. To exercise the reasoning powers.
LESSON.
_Step 1._—Get the pupils to describe the changes to be seen in the sky at
night, and, excluding the apparent motion caused by the earth’s rotation,
find out whether they have noticed and contrasted the constellations of
fixed stars and the planets (wanderers).
Let the pupils tell which of the planets are visible to the naked eye,
and ask whether they have noticed when and where are to be seen, at
the present date, Jupiter, Saturn, and Mars, which are in Capricornus,
Sagittarius, and Leo, respectively.
_Step 2._—Draw from the pupils, if possible, the marks by which planets
can be distinguished from stars.—
(_a_) Their steady light.
(_b_) Size (in the case of Venus and Jupiter).
(_c_) Colour (in the case of Mars).
(_d_) Position (relatively to known constellations).
(_e_) Motion (noticeable after successive observations).
_Step 3._—To enlarge on Point (_d_), let the pupils name the planets
whose orbits are within that of the earth and those whose orbits are
outside ours. By the help of a diagram (blackboard) of the solar system,
get them to infer, from the nearness to the sun of Venus and Mercury,
that these planets are never visible at midnight, but only just before
sunrise and after sunset.
_Step 4._—To appreciate Points (_d_) and (_e_), get the pupils to
recognise the advantage of knowing the constellations by sight. Show
Philip’s Planisphere, and refer to the Zodiac, showing that, besides
being the sun’s apparent path, this is the region in which to seek the
planets.
Public-domain text, read in full here on John Shaqi.
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