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gs together appropriately; the situation, motion, and expression of the figures; their shapes, and lights, and shadows, according. A perfect outline is of most consequence, and can only be acquired by study. Next to this, the situation, colour, and quantity of shadows; these being infinite, may be variously managed. At the same time, it requires much more observation and study to _shade_ a picture, than to merely draw the lines of it. No fixed rule can be given for this; but, after having got the outline free and flowing, endeavour, by various trials, on other bits of paper, to leave the _masses_ of shadow and light _broad_, so as to convey an appearance of _space_ and extent. In the infinite gradations of shade, and the blending of them, nature has no determined law. Objects out of doors, which receive the general light of the sky, and where the surrounding air gives light on _all_ sides, will look altogether different from the same objects drawn and shaded in a room, which would give dark shadows where in nature there are none. (_Plate 3, fig. 2._) Without shadows, the forms of things would be unrevealed. At different times of the day, objects will give shadows quite different in size and form, corresponding with the course of the sun. The difference of your own shadow exemplifies this, as well as the variation of the shadows in your room. Direct your attention to the difference of the shadows thrown by candle-light; this luminary being _smaller_ than the object placed against it, would make a figure, cut from a card, two or three inches high, give a shadow on the wall the size of life. Place any object in the sun, and turn it round to the north, south, east, and west, at different periods; and, observing the difference of shapes in the shadows, will be found excellent practice. Placed in certain directions, the form of every thing may be inferred from its shadow. The shadow of a person arriving, on an open door, will, if the sun is behind him, distinguish to the inmate the comer's identity. Shadow is most articulate and defined when the light is brightest, by reason of the _contrast_ formed by the light; and will always, under these circumstances, appear much stronger than it is; though it is not so strong, in reality, as shadow in cloudy weather, from its being more equalized with the light. Shadow is only, more or less, by _comparison_ with the brightness of the light. This is best explained by mak
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