have virtually given their decision in favour of Hansen,
by crowning him with their highest award of the gold medal. They have
recognised his lunar tables as the complete solution of the grand
nautical problem of finding the longitude at sea. The problem consisted
in merely assigning, with absolute accuracy, the place of the moon in
the heavens at any given time. Hitherto this was not done, as the
perplexing and complicated irregularities of the moon's motion baffled
all attempts to calculate her position with the requisite accuracy.
There are even still some outstanding errors which are yet to be
accounted for, but they are so small, that any further approximation
would practically be of no service to the mariner.
Every time the sailor takes a lunar with his sextant,
he has a practical illustration of the triumphs of astronomy in
assigning at any moment the exact place of the moon in the heavens.
Still every mind must feel the more startling effect produced, when, in
an eclipse of the sun, the first impact of the moon coincides with the
very beat of the clock assigned by the astronomer; and assigned, too,
not as an empirical deduction from previously observed regularity, but
as the result of the all-pervading power of gravitation, which not only
produces the most bewildering inequalities, but furnishes, by its simple
law, a key by which they may be all reduced to the most wonderful
symmetry and order.
We have, however, on the present occasion, taken up
the subject of eclipses, not so much with the view of illustrating the
accuracy of astronomical calculations, as of turning the attention of
our readers to the physical aspects of the total eclipse on the 18th of
July next. No total eclipse has been witnessed in these islands for
several generations. The last observed at Greenwich, was in 1715; and
there was an interval of 375 years between this and the previous one.
The chance of a person ever witnessing in his lifetime a total eclipse
in any given spot of the earth's surface, is exceedingly small. The
shadow forms only a narrow band on the earth's surface, and, though that
strip of darkness will cross Europe six times during the remainder of
the present century, yet comparatively few places will enjoy the
spectacle. It is certain that none of the inhabitants of the British
Isles, will ever see a total eclipse if they do not move beyond their
own shores. But if the shadow does not come to us, we have the
alternative of going to the shadow, And it so happens that the eclipse
of July next, in regard to time and place, presents no ordinary
temptation to the tourist, to plan his summer's trip so as to cross the
path of the shadow.
It may, however, be asked, is it worth while to go
much out of one's way to enjoy the spectacle? "We have seen eclipses
very nearly total, and we can readily conceive one that is absolutely
so. "Would it, then, really reward one to travel far to behold a sight
which may differ so little from what we have already seen? We can give a
very decided answer to this question. No approach to totality can give
the slightest conception of, the effect produced the instant that the
last thread of light is extinguished. The light of the sun is so
intense, that while the slightest part of the disk is visible, the
darkness is by no means alarming. The eclipse of 1857, which was nearly
total, gave great disappointment to many who were led to expect
something very appalling. Accounts of total eclipses were previously
given, and it was a natural and popular expectation, that one so nearly
total would produce effects very similar. But such was not the case. The
darkness was no greater than that often produced by a passing cloud,
and, in the case of many, the eclipse occurred without being in the
least noticed. Partial and annular eclipses are now regarded as matters
of mere curiosity, and a momentary glance upwards is regarded as ail
that is demanded in the way of attention. It is far otherwise with the
total eclipse. The gradual creeping of the moon over the disk of the
sun, gives no preparation for the grand final effect when the last ray
is quenched. It is felt not to be a matter of gradations so frightfully
sudden is the darkness. There is no comparison between a man nearly
drowned and drowned altogether, or between a man half over a precipice
and over altogether; so there is no comparison between a nearly total
eclipse and one absolutely total. As it is the last straw that breaks
the back of the camel, so it is the extinction of the last line of light
that produces the darkness that may be felt; and the " feeling of the
darkness " is hardly a metaphor, as the borders of the terrible pall
thrown over the earth can be actually seen swiftly floating past in the
air .
In these days, when the passion for travel is so
strongly developed, people are ready to go any distance to experience a
new and strong sensation. They do not scruple to traverse the Atlantic,
that they may gaze on the Falls of Niagara, or shoot the rapids of the
St Lawrence; but such sights are not to be compared to a total eclipse,
if measured by the power of stirring strong emotion. In an eclipse all
things combine to deepen the effect; there is nothing out of keeping
with the grandeur and awfulness of the spectacle. In viewing the Falls
of Niagara, there is much to tone down the feelings of awe and wonder.
Familiarity has destroyed man's reverence; merry, laughing, picnic-ing
parties dispel the charm. Blondin exhibits his tight-rope antics in
their very presence. The very birds despise their terrors, and dash
heedlessly into the spray, to catch the stupified fish as they come
tumbling down the liquid arch. The descent of the rapids of the St
Lawrence, however daring the exploit may at first seem, fails, from the
requisite accessaries, to produce a very powerful sensation. Even when
shooting the Long Sault, there is no overpowering feeling. The Indian at
the wheel, with his imperturbable matter-of-fact every-day expression;
the old traveller, not caring to rise from the breakfast-table to look
out on the tumultuous rush of waters; the air of security around, all
combine to break the spell of that wonderful feat. It is quite different
in the case of the total eclipse. All nature sympathises with and
enhances your feelings of awe and mysterious apprehension. The earth,
seas, sky assume a lurid, unnatural hue. An unearthly silence is felt-at
the moment of totality. Every living thing catches the influence, and
cowers under the great blank in the heavens. Beasts of burden lie down
with their loads on the road, and refuse to move on. Swallows in their
bewilderment dash against the walls of houses, and fall down dead. The
dog drops its bone from its mouth, and does not venture to seize it
again till the light returns. Chickens seek the shelter of the parent
wing; and even ants halt in their tracks with their loads, and remain
immovable till the shadow is past.
With such accessaries as the above, it cannot be
wondered at that, in the case of man, however impassive his nature may
be, a total eclipse never fails to produce feelings of mysterious awe.
The most learned savant, as well as the most unsophisticated peasant,
confess to such feelings. Even Mr Airy, the astronomer-royal, the
impersonation of the calm and the abstract, confessed to very curious
and indescribable feelings. It is, however, when men are massed together
that the finest opportunity is afforded for watching the psychical
effects of an eclipse. Such an opportunity was enjoyed by the French
astronomers when observing the total eclipse of 1842 at Perpignan. The
observers were stationed on the ramparts with their instruments; the
soldiers were drawn up in a square on one hand, and on the other the
inhabitants were grouped on the glacis, so that the station commanded
the full view of twenty thousand upturned faces. The astronomers did not
fail to watch the phases of feeling in the crowd, as well as the phases
of the eclipse. The moment that the people, with smoked glasses to their
eyes, marked the first indentiture in the sun's disk, they raised a
deafening shout of applause, much in the way in which they would salute
a military hero, or a popular actor. The moon gradually crept over the
sun, and for a considerable time there was nothing observable but the
ordinary loquacity of a French crowd. As the eclipse drew towards
totality, the murmur of twenty thousand voices rapidly increased, each
one telling his neighbour of the strange feelings coming over him.
Suddenly the last filament of the sun's disk was covered, and at that
moment a deep, prolonged moan, as from one man, arose from that vast
crowd. It was like the stifled groan of the multitude witnessing a
public execution, at the moment that the axe or the drop falls. The
moan, however, did not mark the climax of high-strained feeling. The
dead silence that ensued was the culminating point. Not a whisper was
heard, not an attitude was changed, as with the rigidity of a statue
each man stood and gazed upwards. So unearthly was the silence, that the
beat of the chronometers was heard with painful distinctness. The heart
of the universe seemed to cease its throbbings. Nature had fallen into a
state of syncope. For two and a half minutes this dreadful pause
continued. At the end of this period a thread of light burst forth; the
tension was at once relieved, and one loud burst of joy rent the
heavens. They could not restrain their transports of happiness, now that
the dread, undefinable woe had passed over. They did not care now to
look at the final phase of the eclipse, as the darkness wore off; they
had beheld the crowning spectacle; they would not weaken the impression
by looking at the partial obscuration, and soon the whole crowd melted
away, leaving the astronomers to continue their observations alone.
"We have seen how the eclipse told upon a French
crowd, noted for its impressible and demonstrative character. But there
were also numer-ous illustrations of its power over individuals. Take
one as a specimen:—A young boy, on the same occasion, was herding a few
sheep in a lonely heath, under a cloudless sky; he felt a strange
darkness coming over the face of nature, and at the moment of totality,
he fled towards home, sobbing piteously. Before he reached the door, the
sun burst forth, and in the transport of his joy, he clapped his hands,
exclaiming, ''Beautiful sun! beautiful sun!"
We have viewed the total eclipse merely as a
spectacle of surpassing grandeur; but it is one, too, of the greatest
scientific interest, as throwing unexpected light on the physical
constitution of the sun—
"Who could have thought such darkness lay conceal'd
Within thy beams, O sun! or who could find,
Whilst fly, and leaf, and insect stood reveal'd,
That to such countless orbs thou mad'st us blind!
Why should we then shun death with anxious strife?
If light can thus deceive, wherefore not life?"
If night can give us a surprise by revealing
countless worlds, the eclipse can also surprise by revealing a new glory
of the sun. When the totality is complete, a corona bursts out around
the black circle, like the glory that surrounds the heads of saints in
the pictures of the old masters. This corona has usually been observed
to consist of two zones or concentric strata. The innermost is the
brighter of the two, and the light is nearly uniform. The outer and
fainter zone is diversified with radiating beams. In consequence of the
light of the corona, the darkness is by no means so great as the
darkness of night. The degree of darkness is best measured by the number
of stars visible. In all the authentic accounts we have of total
eclipses, none but the brighter stars have been visible.
The most remarkable and baffling phenomenon is the
rose-coloured prominences seen in the innermost and brighter zone. They
affect curious shapes; one, seen in the eclipse of 1851, has been
designated the boomerang, another, the balloon. Some have been compared
to the teeth of circular saws, others to the flames issuing from the top
of a burning house, and driven aside by the wind.
The most important inquiry that suggests itself is,
"Does this corona belong to the sun or the moon?" This point has been
keenly disputed; but the general belief is that it is an appendage of
the sun. Father Secchi, to whose discoveries in regard to the nature of
the moon's surface we in a former article alluded, is disposed still to
refer the phenomenon to the moon, and to explain it by means of his
discoveries. According to his hypothesis, the corona is produced by the
edges of the moon affecting, in a peculiar manner, the rays of light
which pass across them. The much more probable supposition is that the
corona is the atmosphere of the sun extending beyond its luminous disk,
and that the red flames are substances floating in that atmosphere. In
ordinary circumstances, the photosphere of the sun, or luminous
envelope, is so overpowering, that the atmosphere, with the flames, is
invisible. When, however, the eye is protected by the moon covering the
luminous disk, the atmosphere at once is made visible. No plausible
theory has yet been given to explain the nature of the red flames. A
coincidence has been traced in the position of the flames and that of
the dark spots of the sun ; and it has been conjectured from this that
these dark spots are funnels in the luminous envelope, through which
inflammable gases rise and are burned in the region of the corona or
atmosphere, where they appear as red flames. The truth is, that we have
almost no ground whatever, as yet, on which to base a theory. It was
thought that during the last eclipse of 1851 several points would be set
at rest; but the evidence was very conflicting, arising very much from
the flurried state of feeling caused by the startling character of the
phenomena, and their very brief duration. European astronomers are
looking forward to the approaching eclipse with eagerness, as it is
confidently expected that it will be conclusively settled whether the
corona really belongs to the sun or the moon ; and, for this purpose,
the attention will be directed to two points in the phenomena —first,
whether the corona retains its symmetry, or continues concentric with
the black circle of the moon during the totality ; and, secondly,
whether, during the same period, the red flames change their position on
the circumference of the moon. If there be a want of symmetry, and if
the flames change their place, the evidence is conclusive that the
appendage belongs to the sun.
Another point of interest will be the search for the
newly-discovered planet Vulcan. It is expected that it will be readily
found, from our knowledge of its approximate place.
To make amends for the imperfection of the testimony
of the human eye in such unusual circumstances, it is intended to employ
an artificial substitute, which will record the impression with due
calmness and fidelity. This is to be done by applying a sensitive
photographic surface to the telescope, instead of the human retina. In
other words, photographic pictures of the eclipse are to be taken, and
under Mr Be La Rue's superintendence, we may expect all that skill and
experience can effect.
We are persuaded that many besides professed
astronomers will seize this opportunity of beholding the grandest
spectacle in nature. And why should they not ? It is not a matter
specially belonging to the astronomer. It involves no profound
calculations, nor demands any delicate astronomical methods. It is
simply a physical phenomenon, which any intelligent observer can
appreciate as much as the astronomer. Indeed, the astronomer with all
his imposing instruments, has, as yet, contributed little more than any
one might have done with the use of his naked eye. Any one who goes
merely for the enjoyment of the spectacle, should discard all scientific
pretensions, and abjure the use of instruments. The time of observation
is so brief, that the attention would be distracted and the enjoyment
destroyed by attempting to employ instruments.
The most accessible part of the eclipse's track is in
the north-west of Spain. The centre of the shadow first touches the
coast about Santander, and crosses the peninsula nearly along the valley
of the Ebro. The French astronomers have selected the lofty mountain of
Moncayo, as being in the very centre of the shadow, and enjoying a
climate that precludes all fear of disappointment. There is, however, no
need to climb a mountain to enjoy the spectacle to advantage. The mere
amateur will have much more scope for observation in the neighbourhood
of a populous town. Perhaps the best for this purpose is Vitoria. The
traveller reaches Bayonne from Paris by railway the whole distance, and
the distance from Bayonne to Vitoria across the Cantabrian Pyrenees is
only about twenty-five miles, the journey being performed by diligence.
The eclipse is also total at Pamplona, Burgos, Santander, Bilbao,
Reynosa, all in the same region. To travellers who consult their
comfort, Vitoria presents by far the strongest attraction. The hotels,
according to Ford, are '' some of the best in the peninsula, being more
European than Spanish, and possessing carpets, papered rooms, and even
bells." The Spanish Government have promised every facility to
travellers, and, notwithstanding the Carlist insurrection in the
district, there is little fear of political discomfort. Mr Brassey with
his army of navvies is busy as the pioneers of civilisation, in the
valley of the Ebro. He and Mr Vignoles, the engineer of the railway in
progress, have generously offered any aid in their power to travellers.
It is understood that the Admiralty are ready to put a steamship at the
disposal of such observers as wish to go by sea, and to land at
Santander. Happy is the man who can so arrange his summer holidays as to
combine a visit to one of the most interesting regions of the earth's
surface with the sight of the grandest spectacle the heavens can
present.