with no more seeming hesitation than we would feel in beginning a walk of a like distance upon the land. Once he was seen to turn upon his back and float for a moment leisurely upon the surface, but soon resumed his swimming position again, heading steadily for the land.
At that moment the cry came from forward, "There she blows!" the usual signal at sea for a whale in sight, and all eyes were turned to watch the gambols of a large whale and her calf, half a mile to windward. It will be remembered that these were once famous whaling latitudes, but this adventurous industry has now become almost a thing of the past in these regions. In the mean time the Leviathan and its giant baby were lashing the sea and sending up small mountains of spray, the calf occasionally leaping quite out of the water in its redundant sportiveness. When we finally turned toward the swimming native again, in the opposite direction, his shock of yellow hair was quite lost to view amid the vivid sunlight which blazed over the quivering sea.
After the Samoan group, we passed through or near the Society Islands, encircled by coral reefs, but kept steadily on our course south-southwest, making thirteen knots an hour, and hastening out of the heat of the tropics into a cooler and more comfortable region.
In no other part of the world has the author seen a clearer atmosphere or a grander display of the heavens at night than was enjoyed in the regions through which we were now sailing. Hours were passed in watching the luminous sky, where new and brilliant constellations were serenely gazing down upon us. Venus, the evening star, shone so clear and bright as to cast a long wake upon the wrinkled surface of the sea. There are but about fifteen hundred stars which can be counted from a ship's deck by the naked eye, – a fact which but few persons realize. With an opera-glass or telescope, however, the number can be much increased. We are told that astronomers, by means of their greatly improved facilities, have counted twenty millions of stars. This may be true, and yet it seems almost incredible. We have seen an observer, not familiar with the location of the Southern Cross, examine the heavens long and patiently before being able to find this famous cluster of the Southern Hemisphere, – a visual obtuseness not uncommon among persons who seldom watch the heavens by night. Few give much thought to the stars. Some hastily glance at them and pronounce them beautiful; others regard them with more patient admiration; but not one in a thousand seriously and carefully studies them. A good way of readily finding the Cross is to remember that there are two prominent stars in Centaurus that point directly to it. The one farthest from the Cross is regarded as the fixed star nearest to the earth, but its distance from us is twenty thousand times that of the sun. Stellar distances especially can be realized only by comparison. For instance: were it possible for a person to journey to the sun in a single day of twenty-four hours, basing the time upon a corresponding calculation of speed, it would require fifty-five years to reach this nearest star!
Probably not one half of those who have sailed beneath its tranquil and impressive beauty are aware, that in the middle of the Southern Cross there is a brilliant cluster of stars, which though not visible to the naked eye, are brought out with a strong telescope, – shining like new gems in a beautiful necklace of pearls. In these far-southern waters we saw for the first time what are called the Magellan Clouds. They lie between Canopus, Acherner, and the South Pole. These two light clouds – or what seem to be such, seen in a perfectly clear sky – are nothing more nor less than visible nebulæ, or star-clusters, at such vast distances from the earth as to have by combination this effect upon the human vision.
At sea the stars assume perhaps a greater importance in our estimation than on land, because from them is obtained latitude and longitude, on the principles of terrestrial measurement; and thus by their aid the mariner determines his bearing in the great waste of ocean. Forty or fifty centuries ago the Chaldean shepherds were accustomed to gaze upon these shining orbs in worshipful admiration, but with no idea of their vast system. They were to them "the words of God, the Scriptures of the skies." It has been left to our later days to formulate the methods of their constant and endless procession. All the principal stars are now well known and their limits clearly defined upon charts, so that we can easily acquire a knowledge of them. The inhabitants of North America have the constellation of Ursa Major as also the North Star always with them; they never wholly disappear below the horizon. When the mariner sailing north of the equator has determined the position of this group of seven stars, two of which are known as "the pointers" indicating the North Star, he can designate all points of the compass unerringly. But in the South Sea, where we are writing these lines, a little north of New Zealand, they are not visible. Other constellations however, whose relative positions are as fixed in the Southern Hemisphere, become equally sure guides to the watchful navigator.
How suggestive are these "altar-fires of heaven," particularly when seen from the deck of a ship, alone and at midnight, surrounded by infinite space, thousands of miles from land and home! Generations of men succeed one another in rapid succession, nations rise and fade away, whole races are obliterated from existence, pyramids moulder into dust with thousands of years upon their heads; but the stars fade not; they are the same, unchanged, unchanging, through all the centuries, uninfluenced by the fall of empires or the wreck of human hopes and beliefs.
On the night of the 20th of June the hundred and eightieth meridian was crossed, and the 21st of June was dropped into the sea, so to speak. We had no Tuesday that week; Wednesday followed Monday, – a natural experience in going round the world, which has often been explained. We had been losing time daily in sailing south and west, until this change of date became necessary to regulate the ship's time in accordance with that of Greenwich. An ungeographical Englishman whom we had on board our steamer refused to alter the time of his watch from the first, saying that he only knew that it would come right of itself when he got back to London, which was true enough, though he could not explain why.
Twenty-one days from San Francisco the light at Tiri-tiri Point, on the coast of New Zealand, was sighted, twenty miles distant from Auckland. We entered the harbor early in the morning, and were soon moored at the Union Company's wharf, at the foot of Queen Street. Here the ship not only had freight to discharge, but two or three hundred tons of coal to take on board; so we enjoyed a whole day wherein to stroll about the city, and in the evening we witnessed the "Pirates of Penzance" at Abbott's Opera House. The play was admirably performed by an itinerant company, which regularly makes the rounds of the colonial cities of both Australia and New Zealand.
The outer and inner harbors of Auckland are very beautiful, having picturesque headlands, dominated by volcanic mountains and extinct craters, – indeed the city stands upon the lava vomited from the bowels of Mount Eden. The first land made on coming from the Samoan group was great Barrier Island, which separates the ocean eastward from the Hauraki Gulf, upon which Auckland is situated.
As we shall return in future chapters to this interesting country, no more need be said of its northern metropolis in this connection.
Early on the morning after our arrival the "Zealandia" was again under way, steering north-northeast, until the most northerly point of New Zealand was doubled, then an exact due-west course sped the good ship on her way to Sydney, Australia, twelve hundred and eighty miles distant. It is a stormy ocean that lies between these two countries, and it is useless to disguise the fact that the voyager who crosses it must make up his mind to great and unavoidable discomfort. Any one pursuing the course indicated in these pages, however, will have become pretty well seasoned before entering upon this stage of the long journey. The famous English man-of-war "Challenger" essayed this voyage between Sydney and Auckland twice before she accomplished it, finally fighting her way through the boisterous waves and adverse currents with the united power of sails and steam.
We approached the coast of Australia in tempestuous weather and at night, the "Zealandia" stoutly ploughing her way through a heavy head-sea, while half a gale of wind blew in our faces, and hailstones nearly as large as marbles cumbered the deck. The ship seemed to evince almost human instinct, pausing for an instant now and again, and trembling in every seam as huge waves blocked the way; then, bending down determinedly to the work of forcing a path through the opposing billows, she forged ahead, with the bows at one moment lifted high in air, and the next half
