The eventful night came. It was August, 1890. Mars was then in opposition. The evening had been extremely beautiful. Nature united in her mood the most transporting contradictions of temperament. It was August and the day had been marked by changes of almost tropical severity, although, as we were south of the equator (the latitude of Christ Church is S. 44 degrees) August was, with us, mid-winter. A thunderstorm had broken upon us in the morning, itself an unusual meteorological phenomenon, and the downpour of black rain, shutting off the views and enclosing us in a torrential embrace of floods, had lasted an hour when it passed away, and the Sun re-illumined the wide glistening scene. The line of foam from the breakers along the remote shore, yet lashing with curbing crests the inlets, promontories, and islands, was readily seen; the northern Alps shone in their ermine robes, greatly lengthened and deepened by the season's snows, the washed country side below us was a patch work of rocks and fields and denuded forestland. Christ Church like a vision of whiteness sprang out to the west upon our vision, and immediately about us the mingling rivulets poured their musical streams through and over the icy banks of half consolidated snow.
As night came up, the stars seemed almost to pop out in their appropriate places, like those stellar illusions that appear so appropriately upon the theatrical stage, and the low lying moon sent its flickering radiance over the yet unsubdued waters. It was the time of the opposition of Mars which brings that planet nearest to us. As is well known to astronomers, the perihelion of Mars is in the same longitude in which the earth is on August 27; and when an opposition occurs near that date, the planet is only 35 millions of miles from the earth, and this is the closest approach which their bodies can ever make.
Our magnetic receiver had been placed in position, the Morse register was attached; the whole apparatus was in one of the upper rooms of the observatory, in proximity with the telescope through whose glass for days we had watched the approach of our sister planet. As the night settled down upon us we had taken our seats for a few instants at a table in a lower room engaged in one of those innumerable desultory talks upon our project and their, even to us, somewhat problematic character. Everything connected with that evening, apart from its having been carefully recorded in my diary and notebooks, is very distinctly remembered by me. I recall my father reading from a letter to Nature, May 15, 1884, by Mr. W.F. Denning, discussing "The Rotation Period of Mars." From my note-book I find the passage literally transcribed:
It read—"Notwithstanding his comparatively small diameter and its slow axial motion, the planet Mars affords especial facilities for the exact determination of the rotation period. Indeed, no other planet appears to be so favorably circumstanced in this respect, for the chief markings on Mars have been perceptible with the same definiteness of outline and characteristics of form through many succeeding generations, whereas the features, such as we discern on the other planets, are either temporary, atmospheric phenomena, or rendered so indistinct by unfavorable conditions as to defy measurement and observation. Moreover, it may be taken for granted that the features of Mars are permanent objects on the actual surface of the planet, whereas the markings displayed by our telescopes on some of the other planetary members of our system are mere effects of atmospheric changes, which, though visible for several years and showing well defined periods of rotation cannot be accepted as affording the true periods. The behavior of the red spot on Jupiter may closely intimate the actual motion of the sphere of that planet, but markings of such variable, unstable character can hardly exhibit an exact conformity of motion with the surface upon which they are seen to be projected. With respect to Mars' case, it is entirely different. No substantial changes in the most conspicuous features have been detected since they were first confronted with telescopic power and we do not anticipate that there will be any material difference in their general configurations.
"The same markings which were indistinctly revealed to the eyes of Fontana and Huyghens in 1636 and 1659 will continue to be displayed to the astronomers of succeeding generations, though with greater fullness and perspicuity owing to improved means. True, there may possibly be variations in progress as regards some of the minor features, for it has been suggested that the visibility of certain spots has varied in a manner which cannot be satisfactorily accounted for on ordinary grounds. These may possibly be due to atmospheric effects on the planet itself, but in many cases the alleged variations have doubtless been more imaginary than real. The changes in our own climate are so rapid and striking, and occasion such abnormal appearances in celestial objects that we are frequently led to infer actual changes where none have taken place; in fact, observers cannot be too careful to consider the origin of such differences and to look nearer home for some of the discordances which may have become apparent in their results."
It was just as he finished reading this extract that the shrill fluttering call of the maxy bird was heard from the bare branches of a poplar near the station, and in the next instant, in that intense quiet that succeeds sometimes a sudden unexpected and acute accent, the Morse register was audible above us, clicking with a continuity and evident intention that, weighted as we were with vague sensational hopes, drew the blood from our faces, and seemed almost like a voice from the red orb then glowing in the southeastern sky. We sprang together up the stairs to the operating-room and saw with our eyes the moving lever of the little Morse machine. We had made ourselves familiar with the ordinary telegraphic codes, the international Telegraphic Code and that in use in Canada and the United States. They were useless. The succession of short or long intervals was entirely different and the message, if message it was, defied our persistent efforts at translation. The disturbance of the register continued some three hours, and though we were unmistakably in communication with some external regulated and intentional source of magnetic impulses we were hopelessly confused as to their meaning.
I can never forget our excitement. We were certainly the recipient of exact careful conscious messages. Their terrestrial origin, strange and incredible as it might appear, did not seem likely, for the two codes so generally in use were not represented in it. Could it be—the thought seemed to stop the beating of our hearts—could it be that we had indeed received an extra-terrestrial communication? The register of the dots and dashes cannot be all reproduced here, though a very long record of them, indeed almost complete, was made by myself. During the whole time that the register moved hardly a word of conversation escaped our lips. We were fixed in mute amazement. We were full of unexpressed imaginings, which were told, however in my father's face, so flushed with eagerness, as with half-parted lips he bent over the instrument or interrupted his attention by walking to the window and gazing far out into the heavens.
The record we obtained is here reproduced, in part, as the whole would occupy altogether too much space. I am interested in giving it as it may effectually remain a proof of my sincerity in this matter, and will, I have the firm conviction, be repeated in the future, not exactly or at all, as I have written it, but some message similarly received will corroborate the statement here made, and the still further marvellous facts I am yet to relate.
The record I will select for reproduction is as follows:
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