CHAPTER I

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TO MARS _via_ THE MOON

[Illustration: _Drawn by M. Wicks_

VIEW FROM THE AIR-SHIP, OVER THE CANALS AND THE CITY OF SIRAPION

"What a splendid view we then had over the country all around us!...

Across the country, in line after line, were the canals which we had

been so anxious to see, extending as far as the eye could reach!"]

To Mars _via_ The Moon

_AN ASTRONOMICAL STORY_

BY

MARK WICKS

"_It is astronomy which will eventually be the chief educator and

emancipator of the human race._"--SIR EDWIN ARNOLD.

WITH ILLUSTRATIONS

LONDON

SEELEY AND CO. LIMITED

38 GREAT RUSSELL STREET

1911

Printed by BALLANTYNE, HANSON & CO.

At the Ballantyne Press, Edinburgh

TO

PROFESSOR PERCIVAL LOWELL

A.B., LL.D.

_Director of the Observatory at Flagstaff, Arizona_

TO WHOSE CAREFUL AND PAINSTAKING RESEARCHES,

EXTENDING OVER MANY YEARS, THE WORLD OWES

SO MUCH OF ITS KNOWLEDGE OF

THE PLANET MARS,

THIS LITTLE BOOK IS RESPECTFULLY INSCRIBED BY

ONE WHO HAS DERIVED INFINITE PLEASURE FROM

THE PERUSAL OF HIS WORKS ON

THE SUBJECT

PREFACE

In the course of my experience as an occasional lecturer during the past

twelve years, I have been much impressed by the keen interest evinced,

even by the most unlettered persons, when astronomical subjects are

dealt with in plain untechnical language which they can really grasp and

understand.

The pertinent questions which have been addressed to me privately by

members of my audiences have clearly indicated that there is ample scope

for writers in satisfying a widespread desire for fuller and clearer

information upon such subjects. I have observed that particular interest

is taken in the planet Mars and also in the moon, but ordinary persons

usually find astronomical text-books too technical and too difficult to

master; whilst, as regards Mars, the information they contain is

generally meagre and sometimes not up-to-date.

Scientific readers are already provided for: and it occurred to me that

it would be much more useful and appeal to a more numerous class if,

instead of writing a book on the usual lines, I wrote a narrative of

events which might be supposed to occur in the course of an actual

voyage to Mars; and describing what might be seen on the planet during a

short visit.

This is the genesis of the story; and, in carrying out my programme, I

have endeavoured to convey by means of natural incidents and

conversations between the characters portrayed, the most recent and

reliable scientific information respecting the moon and Mars; together

with other astronomical information: stating it in an interesting form,

and in concise, clear, and understandable language.

Every endeavour has been made to ensure that this scientific information

shall be thoroughly accurate, so that in this respect the book may be

referred to with as much confidence as any ordinary textbook.

Apart from my own studies and work, all these facts have been carefully

verified by reference, as regards the moon, to the works of such

well-known authorities as Neison, Elger, Proctor, Sir Robert Ball, &c.,

whilst, with respect to Mars, the works of Professor Lowell, Flammarion,

Professor Langley, and other writers, as well as practical papers by

other actual observers of the planet, have been studied.

The personal opinions expressed are entirely my own, and the technical

writers above mentioned are in no way responsible for them. I do not,

however, expect my readers to accept all my views, as they relate to

matters in which there is ample room for differences of opinion.

The reader will, of course, understand that whilst the astronomical

information is, in all cases, scientific fact according to our present

knowledge, the story itself--as well as the attempt to describe the

physical and social conditions on Mars--is purely imaginative. It is

not, however, merely random imagining. In a narrative such as this some

matters--as, for instance, the "air-ship," and the possibility of a

voyage through space--must be taken for granted; but the other ideas

are mainly logical deductions from known facts and scientific data, or

legitimate inferences.

Many years' careful study of the various theories which have been

evolved has convinced me that the weight of evidence is in favour of

Professor Lowell's conceptions, as being not only the most reasonable

but the most scientific; and that they fit the observed facts with a

completeness attaching to no other theory. These conceptions I have

endeavoured to present fully and clearly; together with my own views as

an entirely independent writer.

In dealing with the conditions on a distant and inaccessible world the

farthest flight of imagination might fall short of the reality, but I

have preferred to treat these matters somewhat restrainedly. Whilst no

one can say positively that the intelligent inhabitants of Mars do not

possess bodies resembling our own, it is very probable that they differ

from us entirely; and may possess forms which would appear to us strange

and weird. I have, however, thought it desirable to endow the Martians

with bodies resembling ours, but glorified in form and features. The

powers ascribed to the Martians are really only extensions of powers

which some amongst us claim to possess, and they fall short of what more

than one modern scientific writer has predicated as being within the

possibilities of science at a not very distant future.

During the past few years I have been greatly indebted to Professor

Lowell for his kindness and ready courtesy in furnishing me with

information on obscure matters connected with Mars; and my thanks are

also due to the Rev. Theodore E.R. Phillips, of Ashstead, who was good

enough to read the manuscript of this book, and whose great

observational experience enabled him to make valuable suggestions in

regard to the scientific matters dealt with therein.

Truly "a labour of love," this little book--which Professor Lowell has

most kindly permitted me to dedicate to him--is now submitted to the

public, in the sincere hope that its perusal may serve not only to while

away a leisure hour, but tend to nurture a love of the sublime science

of astronomy, and at the same time provide some food for thought.

A few maps, plates, and charts have been added to give completeness to

the work, and it is hoped that they will aid the reader in understanding

the several matters dealt with.

M.W.

1910.

CONTENTS

PAGE

LIST OF PLATES AND MAPS xvii

NOTES ON THE MAPS AND CHARTS xix

THE SUN, MOON, AND PLANETS xxiii

(_Narrative by Wilfrid Poynders, Esq._)

CHAP.

I. WE START ON A VERY LONG VOYAGE 25

II. PERSONAL REMINISCENCES--WHY WE DECIDED ON

THE VOYAGE 35

III. WE APPROACH THE MOON--A MAGNIFICENT SPECTACLE 44

IV. CLOSE TO THE MOON--I GIVE SOME INFORMATION

ABOUT IT 52

V. WE VIEW THE LUNAR SCENERY IN THE NORTHERN

HEMISPHERE 63

VI. THE SCENERY OF THE MOON'S SOUTHERN HEMISPHERE 78

VII. WE RESUME OUR VOYAGE--THE SUN AND THE

SKY AS SEEN FROM SPACE 92

VIII. JOHN INSISTS ON GOING BACK AGAIN--A STRANGE,

BUT AMUSING INCIDENT OCCURS 101

IX. A NARROW ESCAPE FROM DESTRUCTION--I GIVE

SOME PARTICULARS ABOUT MARS AND MARTIAN

DISCOVERY 113

X. THE DISCOVERY OF LINES UPON MARS--THE

GREAT MARTIAN CONTROVERSY 128

XI. THE GREAT MARTIAN CONTROVERSY (_continued_) 139

XII. WE ARE MYSTERIOUSLY PREVENTED FROM APPROACHING

MARS 155

XIII. WE ARRIVE ON MARS AND MEET WITH A STARTLING

SURPRISE 162

XIV. I MAKE A MOST AMAZING DISCOVERY 166

XV. WHAT IS IN A NAME!--THE STORY OF MERNA 169

XVI. WE LEARN SOMETHING ABOUT THE POWERS OF

THE MARTIANS 184

XVII. WE VISIT THE CANALS AND DISCOVER THEIR

SECRET--MARTIAN VIEWS OF LIFE AND DEATH 194

XVIII. WE ATTEND A MARTIAN BANQUET 207

XIX. THE CHIEF OF THE MARTIAN COUNCIL DISCUSSES

THE SOCIAL CONDITIONS OF OUR

WORLD AND MARS 212

XX. THE SECRET OF THE "CARETS"--THE SUN AS

SEEN FROM MARS 224

XXI. OUR FIRST VIEW OF THE EARTH FROM MARS--A

MARTIAN COURTSHIP 236

XXII. CELESTIAL PHENOMENA SEEN FROM MARS--M'ALLISTER

RECEIVES A PRACTICAL LESSON

IN GRAVITATION 242

XXIII. I HAVE A SERIOUS TALK WITH JOHN 253

XXIV. THE MARTIAN SEASONS 256

XXV. MANY THINGS SEEN UPON MARS--I RECEIVE

SOME NEWS 264

XXVI. WE WITNESS SOME WONDERFUL AERIAL EVOLUTIONS

AND LISTEN TO MARVELLOUS MUSIC 282

XXVII. A FAREWELL BANQUET AND A PAINFUL PARTING 293

XXVIII. LAST WORDS TO MY READERS 298

(_Addendum by John Yiewsley Claxton_)

XXIX. WHAT HAPPENED UPON OUR RETURN HOME--RESULTS

OF THE MOST RECENT OBSERVATIONS OF MARS--PROFESSOR

LOWELL'S IMPORTANT DISCOVERY 302

LIST OF PLATES AND MAPS

PLATE PAGE

I. "WHAT A SPLENDID VIEW WE THEN HAD!" _frontispiece_

II. IDEAL VIEW OF LUNAR SCENERY 54

III. CHART OF THE MOON, SHOWING THE PRINCIPAL }

FORMATIONS SEEN ON ITS SURFACE } 80

}

IV. INDEX MAP TO CHART OF THE MOON }

V. DIAGRAM SHOWING THE RELATIVE POSITIONS

AND MOVEMENTS OF THE PLANETS DURING

THE VOYAGE OF THE _AREONAL_ 100

VI. DIAGRAM SHOWING THE RELATIVE POSITIONS

OF THE EARTH AND MARS AT THE TIME OF

VARIOUS OPPOSITIONS OF MARS 110

VII. CHART SHOWING THE RELATIVE POSITIONS OF

THE EARTH AND MARS DURING THE YEARS

1909-1910 118

VIII. MARS. MAP 1 128

IX. MARS. MAP 2 138

X. MARS. MAP 3 154

XI. MARS. MAP 4 206

XII. MARS. MAP 5 224

XIII. MARS. MAP 6 256

XIV. MARS. MAP 7, SHOWING THE PLANET'S SOUTHERN

SNOW-CAP AT ITS MAXIMUM 266

XV. MARS AS SEEN ON AUGUST 16, 1909 }

} 314

XVI. MARS AS SEEN ON OCTOBER 29, 1909 }

NOTES ON THE MAPS AND CHARTS

The maps included in this work have been photographed from a globe of

Mars specially made for the purpose from various charts. In all the maps

the south is at the top and the north at the bottom; and the series

shows the general surface configuration all round the planet, together

with the principal canal lines which have been observed; but many other

canal lines exist, especially on the dark areas near the south pole.

These lines are usually straight and uniform in width throughout their

whole length: indeed it is difficult to mark them upon a globe so that

they shall appear as regular and uniform as they are actually seen on

the planet.

The names on the maps are those now generally accepted and used by

astronomers.

The "Greenwich" of Mars, _i.e._ the point on the Meridian from which

astronomers reckon the Martian longitudes, is indicated by the apex of

the small triangular light area just above the equator in Map I. It is

marked on the map as "Fastigium Aryn," and is chosen as longitude "0,"

because from its general outline it cannot be mistaken by observers.

"Sirapion," the supposed landing-place of the travellers mentioned in

the story, is shown on Map III., just above the central and lowest point

of the dark area at the top of the map. This name will not be found upon

any other map of Mars.

The chart showing the relative positions of the Earth and Mars during

the years 1909-10 is reduced and modified from one prepared accurately

to scale by the author for his own use in connection with the book. From

it the reader will gain a clear idea of the shape of the two orbits and

how they are placed with regard to each other.

It also shows the course supposed to be taken by the air-ship on its

outward and homeward journeys, and the point reached when one of the

travellers desired to turn back; together with the alternative routes

which were then discussed.

This chart, and the other one showing the positions of the two planets

at different oppositions of Mars, will enable the reader to understand

how it is that Mars approaches so much nearer to the earth at some

oppositions than it does at others. The positions of the oppositions

from 1916 to 1922 are only approximations, as no exact data are yet

available. The earth is closest to the orbit of Mars about the 27th of

August each year, and if Mars comes into opposition about that date it

is then only about thirty-five million miles away. If, however, the

opposition occurs near the 22nd February, the earth is then at its

greatest possible distance from the orbit of Mars, and that planet will

then be over sixty million miles away: appearing very much smaller than

when at its most favourable point of approach.

On the 18th of September, 1909, Mars was only slightly over thirty-six

million miles from the earth, and it will be fifteen years before such a

favourable situation again occurs.

The nearest point of approach does not necessarily occur on the actual

date of the opposition. In 1907 Mars was in perigee, as it is termed,

seven days after the opposition; while in 1909, perigee was before

opposition.

The diagram showing the positions and movements of the planets during

the period covered by the outward voyage of the _Areonal_ is

sufficiently explained by the notes printed thereon. It may, however, be

pointed out that though the orbits of the planets are all elliptical,

especially those of Mercury and Mars, they are so nearly true circles

that, when reduced to the scale of these diagrams, they practically

become circles. The exaggerated ellipses so often found in astronomical

books are very misleading. The orbits of Mercury and Mars have an

appearance of ellipticity because the sun does not occupy the central

point in the diagram.

The view of the moon is photographed from a large coloured drawing by

the author, which occupied many months in preparation and execution. It

shows all the principal formations seen through the telescope as the

moon passes through its various phases, but it must be understood that

the formations can never all be seen at one view as shown in this

picture. As the sun rises on any particular formation the details are

gradually revealed by the long shadows cast by the more elevated

portions when the sun is low down in the lunar sky. As the sun rises

higher and higher the shadows grow shorter and shorter, and when the sun

is vertically over the formation the shadows entirely disappear; all

details are thus rendered invisible.

When the moon is full the sun is practically vertical over the whole

lunar surface, so the only details then seen are those which are vaguely

brought out by differences in tint.

The bright ray-streaks are only suggested in the picture, because, if

shown complete, they would have the same effect as upon the moon, viz.

they would entirely obliterate all the formations over which they

passed.

The Key Map indicates the principal lunar formations, and includes the

names of those mentioned in the book.

The last two plates in the book are from drawings made at the telescope

(a 12-inch Calver reflector) by the Rev. T. E. R. Phillips. The

opposition of 1909 was not favourable for the observation of Martian

details from England; for although the planet was near to us, it was too

low down in the sky; and many of the nights were either cloudy or

misty.

THE SUN, MOON, AND PLANETS

Diameter. Period of Rotation. Mean Distance

from the Earth.

---------------------------------------------------------------------------

SUN 865,000 miles 25 to 26 days 92,800,000 miles

MOON 2,160 miles 27-1/3 days 238,000 miles

(It revolves round the

earth in the same time.)

---------------------------------------------------------------------------

PLANETS. Diameter in Number of Period of Period of Mean Distance

Miles.[1] Satellites Rotation. Revolution from the Sun in

Known.[2] Round the Sun. Millions

of Miles.

---------------------------------------------------------------------------

Hrs. Mins. Days.

Mercury 2,992 None [3]? 88 36

Venus 7,660 None ? 225 67

Earth 7,918 One 23 56 365-1/4 92-3/4

Mars 4,220 Two 24 37 687 141-1/2

Asteroids Very tiny planets, hundreds in number; and more are

frequently being discovered.

Jupiter 86,000 Eight 9 55 4,332-1/2 482

Saturn 74,000 Ten 10 14 10,759 886

Uranus 31,700 Four Not known 30,687 1,780

Neptune 34,500 One " " 60,127 2,780

---------------------------------------------------------------------------

TO MARS _via_ THE MOON

(_Narrative written by Wilfrid Poynders, Esquire, late of Norbury, in

the County Borough of Croydon, Surrey_)

CHAPTER I

WE START ON A VERY LONG VOYAGE

"Well, I suppose it is about time to get ready for starting?"

The speaker was a smart, well-set-up man about forty-three years of age,

whose keen and alert expression, clear eyes and well-cut features were a

true index to the intellectuality and integrity of his character; whilst

his closely compressed lips and the deep vertical line down the centre

of his forehead betokened a dogged perseverance in carrying into effect

anything he might undertake.

John Yiewsley Claxton, for that was his name, was my very intimate

friend of at least twenty-five years' standing; and during the greater

portion of that time he had been my constant companion. We had passed

through many trials and troubles together, but a better friend and

companion no man could have desired.

We were just finishing a last quiet smoke and chat in my snuggery at

Norbury, near Croydon, preparatory to starting off on a very long

journey for which all arrangements had been completed, and we had risen

early that morning in order to have everything in readiness.

John took his pipe from his lips as he spoke, then, rising, stretched

out his arms and braced himself up like one ready and eager for any

emergency; the next minute he was smoking in his usual calm and

thoughtful manner. I rose when he did, then giving a few final

instructions to Mrs. Challen, my housekeeper, we bade her "good-bye" and

stepped out on to the lawn, thence crossing over to a gate at the far

end of the garden, we passed into an extensive field and walked toward a

large shed that stood near its centre.

It was a most beautiful evening near the beginning of August 1909, clear

and calm. The sun had only just passed below the horizon, the sky

immediately above it being a rippled glory of gold, merging higher up

into gold flecked with crimson, then into a placid sea of pale

apple-green. Above this were fleecy clouds of delicate rose-pink, which

reflected their splendours upon the higher parts of the surrounding

hills, the latter standing out clear and sharp, and glowing with roseate

hues, whilst their bases were seen dimly as through a thin veiling of

purple mist.

Surely nothing could be better for the commencement of our long-planned

trip. The moon would not rise until about a quarter-past nine, and

darkness would have descended by the time we were ready to start. This

was exactly what we required, because we did not wish either our

preparations or our departure to be observed.

Just as we arrived within hail of the shed the door opened, and a

rugged-featured man with sandy hair stepped out. This was Kenneth

M'Allister, our engineer and general factotum in all mechanical

matters--a typical specimen of a Scotch engineer. He had followed his

profession in its different phases on tramp-steamers, on ocean liners,

naval gunboats, and even on battle-ships, besides having served for

several years in the workshops of a great firm of electrical engineers.

Whether repairing a broken propeller-shaft two or three scores of tons

in weight, the most intricate machinery, or the most delicate electric

mechanism, he was equally at home and sure in his work; in fact nothing

seemed to come amiss to him. His machinery was always the object of his

most anxious care, and, providing that all worked satisfactorily,

nothing else troubled him much.

"Well, M'Allister," I called to him, "is everything ready for our trip

to-night?"

"Heh, mon," he replied, "everything is all ready; will you look in and

take a turn round the ship?"

"Certainly we will," I answered; so we all went into the shed, where we

gazed with equal pride and satisfaction upon the splendid shining object

which was housed therein. Here, in perfect readiness for its destined

service, was our air-ship--if it could be so called--upon which we three

had expended years of thought, experiment, and work.

Outwardly it was shaped somewhat like a fish, being constructed of a

special metal--our joint invention--which we had named "martalium." The

metal was composed of aluminium and two other rarer metals which, when

combined together, produced a substance almost as light as aluminium,

yet many times harder and tougher than case-hardened steel; whilst its

surface shone like burnished silver and could never in any circumstances

become tarnished or affected by rust.

The ship was ninety-five feet in length, and its diameter twenty feet in

the broadest part, tapering off to a point at either end.

With the exception of the steering and balancing fans, there was no

machinery whatever visible on the exterior of the vessel. Several

windows along each side, together with a few at the top and bottom of

the vessel, gave light to the interior, and would allow for observations

being made in any direction. These windows were all constructed of a

special toughened glass obtained from Vienna, very thick and warranted

to withstand the hardest blows. Along each side of the vessel there was

an observation platform or gallery on to which the exterior doors

opened, and each gallery was provided with a protecting railing.

The interior of the ship was divided into five separate compartments,

the rear one being the general living and sleeping room, having

observation windows so arranged as to command an outlook in all

directions. The next compartment was mainly a store-room, but, like all

the others, could be used for observation purposes; next to that was a

small compartment intended for a special purpose which will hereafter be

apparent; then another containing water storage, apparatus for

compressing or rarefying air, as well as machinery for producing the

latter chemically.

Lastly, right in the forepart of the vessel was M'Allister's special

sanctum, containing the driving, lighting, warming, and steering

machinery, but electric buttons and switches were also provided for

controlling these in every compartment, so that whichever one we

happened to be in we were prepared for all emergencies. Periscopes

capable of being turned in all directions also communicated with every

compartment, thus we could always see what might be around us.

All the machinery was either electric or magnetic, some of it being very

simple; other portions were extremely intricate, but nearly all was the

outcome of our joint inventions. Such parts as could not profitably be

made by ourselves had been carefully distributed between several firms

of founders and engineers, in order that none could have any means of

discovering the use to which they were intended to be put. The whole of

the shell of the vessel was double, with a packed space between the two

skins; and each door opened into a small lobby, having another door on

the farther side, to ensure that every part might be kept perfectly

air-tight when required.

By the time we had completed a thorough inspection of the vessel and its

machinery, and overhauled the stores to make sure that everything

requisite was on board, it had become nearly dark, so, moving a switch,

M'Allister swung open the great doors at the end of the shed. The vessel

was standing upon a low trolley having many wheels running on rails,

with a small electric motor beneath it, and, upon M'Allister moving the

trolley switch, the whole affair glided smoothly out into the open

field. I may as well confess that we owed this trolley and the mode of

its working to ideas gained during an inspection of the construction and

working of the conduit trams belonging to the London County Council.

When the vessel was out in the open we congratulated ourselves upon its

splendid proportions and business-like appearance.

I asked M'Allister whether "he was satisfied with the result of our

labours?"

"Mon," he replied, "she's grand, and it's fine to have the handling of

such machinery; everything works as slick as grease!" It was a pleasure

to hear him talk about his machines, for he was always so enthusiastic

where they were concerned.

"Now," I suggested, "before we start we'll give our good ship her name."

"Bravo!" said John Claxton, "and we'll drink to her success, a good

voyage and a safe return"; and he was so struck by the brilliancy of his

idea that he actually took his pipe from his lips, and, holding it in

his hand, regarded it with thoughtful contemplation for quite three

minutes.

I accordingly went to the store-room and brought out two bottles of

champagne. Directly M'Allister saw them he entered a vigorous and

emphatic protest, saying, "Heh, Professor! you're surely not going to

celebrate this most auspicious event with such poor fizzy stuff as

champagne? Let's have a wee drop of good old Scotch whisky, and do the

thing properly!"

John Claxton here interposed: "Let M'Allister have his whisky if he

prefers it, and we'll have the 'fizz'!" So I went laughing to the store

again and returned with a bottle of special Scotch, whereat

M'Allister's eye gleamed as he smiled approval.

Then, taking up a bottle of the champagne, I broke it over the prow of

the vessel, and we solemnly christened her the _Areonal_ in honour of

the planet for which we were bound.

Raising high our glasses we gave the toast of "_The Areonal_; may she

and her passengers have a good voyage and a safe return home!"

M'Allister peered over the rim of his glass, and, with upturned eyes,

remarked that "his old wife in Glasgow would be looking for his safe

return in a few months' time"; then his glass slowly tipped up, and the

old Scotch whisky disappeared.

Claxton and I at once stepped on board the vessel, and having just set

the machinery slowly moving so as to raise the vessel a few feet, I put

on the neutral power so that the ship remained poised in the air.

M'Allister ran the trolley back into the shed, closed the doors, and

switched off the electric current; then climbed the extending ladder,

and came on board, John steadying the vessel by an anchor rope in the

meantime.

M'Allister took over the command of the machinery, and, setting it in

motion, the _Areonal_ at once rose slowly and gracefully straight up

into the air.

John and I were standing outside on the platform, from whence, looking

toward the house, we could plainly see Mrs. Challen at the open door of

our sitting-room waving farewell to us--her figure silhouetted against

the bright light of the room. We waved back to her in response, but I am

very doubtful if she could see our signal, as she was looking into the

darkness.

We now rose rapidly as M'Allister switched on more power, and far away

to the northward we could see over the whole extent of the vast

metropolis, with its countless miles of lighted streets. On turning

towards the east the Crystal Palace, which was lighted up, was a very

conspicuous object against the skyline over the Sydenham hills.

John, when he saw it, remarked that "it would have been an appropriate

tribute to our enterprise if the Palace Company had provided one of

their grand firework displays as a send-off for us"; "but," he added,

"these companies will never do what is expected of them!" On the

westward side the lights all along the hill where Sutton lies were

clearly visible; farther off was Epsom, and, with the aid of a glass, we

could even faintly see the lights of Guildford in the far distance.

Nearly south of us Croydon seemed from our altitude to lie almost

beneath our vessel. We directed our course towards the south-east,

passing over the railway-station at Thornton Heath, with Croydon to the

right of us, just as the clock of the Croydon Town Hall was striking

nine. The long lines of lighted streets made a fine panorama, and we

could trace the lights of the moving tram-cars out to Anerley, South

Norwood, Purley, Wallington, and Mitcham.

Although we were fully 5000 feet, or nearly a mile, above the earth it

was surprising how clearly we could hear the sounds from below--the

rumble of the electric tram-cars, the clang of their gongs, the

toot-toot of the motor-horns, and, louder still, the whistles of the

locomotives on the London and Brighton Railway were borne to us with

almost startling distinctness through the still night air.

Our electric lights were now switched on at their full power, their

bright beams shining out through the windows all around the vessel.

Whilst we were on the ground we only used just sufficient light to see

by, as we did not wish to draw attention to our proceedings; but now we

were well up and on our way it mattered not who saw us.

With increased speed we passed over South Norwood and the village of

Shirley, rising higher and higher as we proceeded on our way. The moon,

which was just past the full, had not risen above the horizon of those

upon the earth below us; but we had now attained such an altitude that

it became visible to us, low down on the horizon and far ahead on our

left hand. Owing to our height above the earth it soon became impossible

for us to see the places over which we passed, and as we were moving

over an open part of Kent there were very few lights which we could have

seen in any case. As there was nothing of particular interest to attract

our attention which we had not already seen on our trial trips, we

entered our general room and sat down to supper.

The machinery had been set to maintain a speed of 150 miles an hour

until we passed beyond the limits of the earth's atmosphere; for though,

no doubt, we might safely have travelled faster, we did not intend

taking any risk of overheating our vessel by the friction of the

atmosphere.

Notwithstanding the speed at which we were travelling we were quite

unconscious of any movement in our vessel. The impression we received

was not that we were rushing away from the earth, but that the earth was

rapidly falling away from our position in space.

It may, perhaps, be desirable that I should now give a little

information respecting myself and my friends, together with some

explanation of our reasons for embarking upon such a very long voyage.

To Mars via the Moon: An Astronomical Story · 第 1 / 29 章