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Here we meet with Wouverman (1619-1668), a painter of horses, cavalry, battles, and riding parties placed in landscape. His landscape is bright and his horses are spirited in action. There is some mannerism apparent in his reiterated concentration of light on a white horse, and some repetition in his canvases, of which there are many; but on the whole he was an interesting, if smooth and neat painter. Paul Potter (1625-1654) hardly merited his great repute. He was a harsh, exact recorder of facts, often tin-like or woodeny in his cattle, and not in any way remarkable in his landscapes, least of all in their composition. The Young Bull at the Hague is an ambitious piece of drawing, but is not successful in color, light, or _ensemble_. It is a brittle work all through, and not nearly so good as some smaller things in the National Gallery London, and in the Louvre. Adrien van de Velde (1635?-1672) was short-lived, like Potter, but managed to do a prodigious amount of work, showing cattle and figures in landscape with much technical ability and good feeling. He was particularly good in composition and the subtle gradation of neutral tints. A little of the Italian influence appeared in his work, and with the men who came with him and after him the Italian imitation became very pronounced. Aelbert Cuyp (1620-1691) was a many-sided painter, adopting at various times different styles, but was enough of a genius to be himself always. He is best known to us, perhaps, by his yellow sunlight effects along rivers, with cattle in the foreground, though he painted still-life, and even portraits and marines. In composing a group he was knowing, recording natural effects with power; in light and atmosphere he was one of the best of his time, and in texture and color refined, and frequently brilliant. Both (1610-1650?), Berchem (1620-1683), Du Jardin (1622?-1678), followed the Italian tradition of Claude Lorrain, producing semi-classic landscapes, never very convincing in their originality. Van der Heyden (1637-1712), should be mentioned as an excellent, if minute, painter of architecture with remarkable atmospheric effects.

The minimum temperature during the night was 69 deg. F. We slept in the boat, and were simply devoured by mosquitoes. The chief of the Indians who had been lent me by the Fiscal Agent became seriously ill during the night with a severe attack of fever. All my men, with no exception, also became ill, and were shivering with cold, owing to fever. The chief of the police, Luiz Perreira da Silva, who had been placed by Mr. Barretto in charge of the Indians who were to accompany me, in jumping from the boat that night on to the shore hurt his foot, the pain caused by that slight injury giving him also a severe attack of fever. So that of the entire crew there remained only two men in good health--viz. Mr. Julio Nery and myself.

Our system, in fact, is shaped something like a lens, and our sun is situated near the centre of this lens. In the remoter part of this lens, near its edge, or possibly outside it altogether, lies the great series of star clouds which make up the Milky Way. All the stars are in motion within this system, but the very remarkable discovery has been made that these motions are not entirely random. The great majority of the stars whose motions can be measured fall into two groups drifting past one another in opposite directions. The velocity of one stream relative to the other is about twenty-five miles per second. The stars forming these two groups are thoroughly well mixed; it is not a case of an inner stream going one way and an outer stream the other. But there are not quite as many stars going one way as the other. For every two stars in one stream there are three in the other. Now, as we have said, some eminent astronomers hold that the spiral nebulae are universes like our own, and if we look at the two photographs (Figs. 25 and 26) we see that these spirals present features which, in the light of what we have just said about our system, are very remarkable. The nebula in Coma Berenices is a spiral edge-on to us, and we see that it has precisely the lens-shaped middle and the general flattened shape that we have found in our own system. The nebula in Canes Venatici is a spiral facing towards us, and its shape irresistibly suggests motions along the spiral arms.

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