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1843 - Of
Mars, our precise knowledge is little. It has an atmosphere not
unlike that of the earth- certainly not more extensive,and
probably clearer. Its day and night are almost of the duration of
ours, and its surface is divided into continents and seas, whose
complete outline we have not been able to trace. PLATE XII- for
which Astronomy is indebted to the accurate and graphic pencil of
Sir John Herschel- shows one side of Mars. The darker parts are
seas, and the land is characterized by a reddish color, undoubtedly
springing from its chief geological formation. The bright spot at
the top, is at the pole of Mars; it
disappears as the Sun shines on it more directly, and there can be
no doubt that it is a reflection from snow. Rain and sunshine are
therefore there, mornings and gorgeous sunsets, with their tongue of
flame shooting across the waters; also in Mars there is the eternal
flow of the ocean! Its tides, however, must be gentle, such as wash
the isles of Egean. The division of this planet into land and sea
shows that its profile is irregular- in other words that there are
elevations in it.
Nichol, J.P., The
Phenomena and Order of the Solar System, 1843, Dayton & Newman, New
York.
1843 - When viewed with a powerful telescope,
the surface of Mars appears diversified with numerous varieties of
light and shade. The region around the poles is marked by white
spots, which vary their appearance with the changes of seasons in
the planet. Hence Dr. Herschel conjectured that they were owing to
ice and snow, which alternately accumulates and melts, according to
the position of each pole with respect to the sun. It has been
common to ascribe the ruddy light of this planet to an extensive and
dense atmosphere, which was said to be distinctly indicated, by the
gradual diminution of light observed in a star as it approached very
near to the planet in undergoing an occultation; but more recent
observations afford no such evidence of an atmosphere.
Olmstead, Dennison,
An Introduction to Astronomy, 1843,
Collins, Keese and Co., New York. -
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1859 - The
extraordinary height and density of the atmosphere of Mars, are
supposed to be the cause of the remarkable redness of its light. It
has been found, by experiment, that when a beam of white light
passes through any colorless transparent medium, its color inclines
to red, in proportion to the density of the medium, and the space
through which it has traveled. Thus the Sun, Moon, and stars appear
of a reddish color when near the horizon, and every luminous object,
seen through a mist, is of a ruddy hue.
Burritt, Elijah H.,
The Geography of the Heavens, 1859, Mason
Brothers, New York. -
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1869 - To
the naked eye Mars is the reddest star of the sky, shining with a
steady brightness, which varies with its distance from the earth. In
the telescope its color is less intense, and is relieved by spots of
bluish-green or white. The red portions are thought to be land,
showing the general color of rocks and soil; the green tints are
believed to come from water. Definite outlines of lands and seas are
discernible. Mr. Dawes has mapped them, and they have received the
names of distinguished astronomers who have given special study to
this planet. The long bottle-shaped seas,
and the vast length of coastline contrast strongly with the broad
oceans and compact continents on the earth.
Peabody, Selim H.,
The Elements of Astronomy, 1869, Wilson, Hinkle & Co., New
York. - back to
top
1870 - Then,
lastly, there must be rivers on Mars. The clouds which often hide
from our view the larger part of a Martian continent indicate a
rainfall at least as considerable (in proportion) as that which we
have on the earth. The water thus precipitated on the Martian
continents can find its way no otherwise to the ocean than along
river courses.
As to the nature
of these rivers, again, we may form conjectures founded on
trustworthy analogies. The mere existence of continents and oceans
on Mars proves the action of forces of upheaval and of depression.
There must be volcanic eruptions and earthquakes modelling and
remodelling the crust of Mars. Thus there must be mountains and
hills, valleys and ravines, water-sheds and water-courses. All the
various kinds of scenery which make our earth so beautiful have
their representatives in the ruddy planet.
Proctor, Richard A., Other Worlds
Than Ours, 1870, Thomas Y. Crowell & Co.,
New York. - back
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1879 - The first thing that strikes the
observer is a dazzling spot of white near the pole which happens to
be toward him, or at both poles when the planet is so situated that
they can be seen. When the north pole is
turned toward the sun the size of the spot sensibly diminishes, and
the spot at the south pole enlarges, and vice versa. Clearly they
are ice fields. Hence Mars has water, and air to carry it, and heat
to melt ice.
This carrying of
water from pole to pole, and melting of ice over such large areas,
might give rise to uncomfortable currents in ocean and air; but very
likely an inhabitant of earth might be transported to the surface of
Mars, and be no more surprised at what he observed there than if he
went to some point of the earth to him unknown. It may be
conjectured that Mars might be a comfortable place of residence to
beings like men.
Warren, Henry
White, Recreations in Astronomy, 1879, Harper & Brothers, New York.
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1890 - On the question as to the possibility
of life on Mars, a few words may be added. If we could be certain of
the existence of water on Mars, then one of the most fundamental
conditions would be fulfilled, and even though the atmosphere on
Mars had but few points of resemblance in composition or in density
to the atmosphere of the earth, life might still be possible. Yet
even if we could suppose that a man would find suitable nutriment
for his body and suitable air for his respiration, it yet seems very
doubtful whether he would be able to live. Owing to the small size
of Mars and the smallness of its mass in comparison with the earth,
the intensity of the gravitation on the surface of Mars would be
very different to the gravitation on the surface of the earth. The
effect of such changes on man would be indeed remarkable. He would
experience a buoyancy quite unfamiliar to
his terrestrial experience. It may well be doubted whether our
organism would be adapted to a change so radical and so complete. We
should imagine that the circulation of the blood and the various
movements which constitute life would be deranged by such changes.
Ball, Robert Stawell,
The Story of the Heavens, 1890, Cassell &
Co., London. -
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1906 - That Mars is inhabited by beings of
some sort or other we may consider as certain as it is uncertain
what those beings may be.
Just as we have
now found organic existence in abyssal depths of sea and in
excessive degrees of both heat and cold, so do we find from
exploration of our island mountains, which more than any other
locality on earth facsimile the Martian surface, its possession
there as well.
Another point,
too, is worth consideration. In an aging world where the conditions
of life have grown more difficult, mentality must characterize more
and more its beings in order for them to survive, and would in
consequence tend to be evolved. To find, therefore, upon Mars highly
intelligent life is what the planet's state would lead one to
expect.
By studying
others we learn about ourselves, and though from the remote we learn
less easily, we eventually learn the more.
Lowell, Percival,
Mars and Its Canals, 1906, The Macmillan
Co., New York. -
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1906 - It
is the design of physical science not only to record but to explain
appearances; and the canals, whether double or single, have, to many
astronomers who have seen them, a look of artificiality rather than
naturalness. If we accept the former, the explanation of the canals
themselves, advanced by W. H. Pickering and reinforced by the
argument of Lowell, seems very plausible: water is scarce on the
planet; with melting of the polar caps, it is gradually conducted
along narrow channels through the middle of the canals, thereby
irrigating areas of great breadth which, with the advance of the
season, become clothed with vegetation.
Of course,
acceptance of this theory implies that Mars in ages past, has been,
and may be still, peopled by intelligent beings; and that
continuation of their existence upon that planet,
during secular dissipation of natural water supply, has rendered
extensive irrigation a prime requisite. But only by long continued
observation of the behavior of canal and oasis in both hemispheres
of Mars can we hope for a rational solution of the question of life
in another world than ours.
Todd, David,
A New Astronomy, 1906, American Book
Company, New York. -
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1926 - The explanation for the scanty
atmosphere of this planet is that its mass is so small and its
surface gravity so feeble that it has not power to control one. If
Mars does control an atmosphere, probably it is made up largely of
the heavier gases. When Mars passes between us and a star the light
of the star is suddenly extinquished as the edge of Mars reaches it.
If Mars had an extensive atmosphere the light of the star would
gradually diminish as it shone through more and more of the gaseous
envelope surrounding the planet. Probably atmospheric pressure on
Mars does not exceed that on the top of our highest mountains.
The most serious
question in the interpretation of the polar caps is that apparently
the climate of Mars ought to be considerably colder than that of the
earth. Mars is so much farther from the sun than the earth is, that
it receives less than half as much light and heat from the sun as
the earth. Using this fact to compute the theoretical temperature
which it would have if its atmospheric conditions were the same as
those of the earth, and assuming that the mean temperature of the
whole earth is 60 degrees F., it turns out that the average
temperature on Mars should be 38 degrees below zero F.
Moulton, Forest
Ray, Astronomy, 1926, American School Publishers, London.
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1926 -
Finally, after all these conditions are satisfied, will life come or
will it not. We must probably discard the at one time widely
accepted view that once life had come into the universe in any way
whatsoever, it would rapidly spread from planet to planet and from
one planetary system to another until the whole universe teemed with
life; space now seems too cold, and
planetary systems too far apart. Our terrestrial life must in all
probability have originated on the earth itself. What we would like
to know is whether it originated as the result of still another
amazing accident or succession of coincidences or whether it is the
normal event for inanimate matter to produce life in due course,
when the physical environment is suitable. We look to the biologist
for the answer.
The astronomer
might be able to give a partial answer if he could find evidence of
life on Mars or some other planet, for we should then at least know
that life had occurred more than once in the history of the
universe, but so far no convincing evidence has been forthcoming.
The supposed canals on Mars disappear when looked at through a
really large telescope, and have not survived the test of being
photographed. Seasonal changes necessarily occur on Mars as on the
earth, and cerain phenomena accompany these which many astronomers
are inclined to ascribe to the growth and decline of vegetation,
although they may represent nothing more than rains watering the
desert. There is no definite evidence of life, and certainly no
evidence of conscious life, on Mars or indeed anywhere else in the
universe.
Jeans, James, The
Universe Around Us, 1929, The Macmillan Co., New York. -
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1932 - There
is no longer any doubt as to the existence of the canals of Mars.
They have been observed by many astronomers, and have been
photographed successfully. In all probability they are somewhat
broader, and less regular and artificial in appearance, than they
seemed to some of the earlier observers. We accept the canals as
natural features of the Martian landscape.
There appears to
be life on the planet Mars. A few years ago this statement was
commonly regarded as fantastic. Now it is commonly accepted. We
refer, however, to forms resembling our vegetable life and not to
intelligent human life, for there is no evidence to prove the
existence of such life on Mars. The planet possesses air and
water, although in very small quantities compared with the earth, to
be sure; and in the tropics the surface is above freezing at noon,
although far below freezing most of the time even there and of
course all the time on the rest of the planet.
Baker, Robert H.,
Simon Newcomb's Astronomy for Everybody, 1932, Garden City
Publishing Co., Garden City, N.Y. -
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1935 - Astronomers at Mount Wilson inform us,
as the result of their spectroscopic examinations of the planet,
that the amount of oxygen above the reflecting level of Mars cannot
exceed a thousandth part of the amount above an equal area of the
earth at sea level, while the amount of water vapor is as low as
five percent. These restrictions on life appear to be serious. The
blue-green areas are not bodies of water. Mars is a desert, in
general.
The dark markings
in a Martian hemisphere grow greener and more prominent in the late
spring and early summer of that hemisphere. They fade to a chocolate
brown as the fall season approaches. These changes in the surface
markings are such as would be expected, if they are produced by the
growth and decline of vegetation. If this be the correct
explanation, then there is life on Mars- vegetable life, at least.
But some other explanation of the seasonal changes may come forth.
It seems wisest to leave the whole question of life on Mars open for
the present.
Baker, Robert H.,
An Introduction to Astronomy, 1935, D. Van Nostrand Co., New
York. - back to
top
1935 - Some people are of the
opinion that the markings on Mars are canals which have been
constructed by intelligent human beings. There seems to be no good
reason why human beings could not live on Mars. This planet is
probably at a rather advanced period in its evolution and much of
its surface is desert waste. We would probably find on Mars a higher
state of civilization than on the earth, but the inhabitants, like
the planet, have probably passed their zenith and are on the
decline.
The question is
frequently raised as to whether it will ever be possible to send
signals to Mars. How much power will be required? Can the millions
of horsepower of energy which is exhibited in lightning be seen on
Mars? Is radio communication possible? Who is going to pay the cost
of this gigantic power plant? What language are we going to speak?
What are we going to talk about? Do the inhabitants of Mars know
anything that we know, that is, can we find a topic of conversation?
How are we going to determine whether or not they get our message?
Harding, Arthur M., Astronomy, 1935,
Garden City Publishing Co., Garden City, N.Y. -
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1944 - Many observers of Mars deny the
existence of this network of fine straight lines, claiming that the
markings are not only much broader individually but that there are
considerable variations in width and direction. There are on the
surface of Mars many details which cannot be seen individually but
which the eye unconsciously integrates into lines and spots. If this
is the case we would expect small telescopes to bring out the fine
network while large telescopes, having a greater resolving power,
would be able to bring out more detail and thus destroy the
appearance of the network.
There seems to be
no question about the existence of some sort of vegetation on Mars.
Change in the color of the dark regions with the change in seasons
appears well established, but we have no way of determining whether
this vegetation consists of the simple forms, such as might
correspond to lichens and mosses on the earth, or of higher forms,
such as trees. If plant life exists it does not seem impossible that
at least low forms of animal life also may be there, but no
observations have been brought forward to establish this.
Fath, Edward Arthur,
The Elements of Astronomy, 1944,
McGraw-Hill Book Co., New York. -
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1949 - It
has often been suggested that the bright regions of Mars may
resemble the "Painted Desert" and that its surface is covered with
reddish iron oxides, in particular FE2O3; that, in fact, the oxygen
of the Mars atmosphere was depleted in the process of oxidation. The
reflections of red soil and red rock, collected by the writer in
Oklahoma, Texas, and Arizona, were found to be quite different
from those of Mars. However, a brownish, fine-grained felsite was
found that closely matches the Mars curve in the full range
considered. We may tentatively assume that the bright desert regions
of Mars are composed of igneous rock, similar to felsite.
The Mars
atmosphere contains, therefore, slightly more than 2.2 as much CO2
as the atmosphere above McDonald Observatory. Mars polar caps are
not composed of CO2 and are almost certainly composed of H2O frost
at low temperature.
It is too early
to conclude that the green areas on Mars are covered with lichens or
mosses; different forms of plant life may well have developed under
very different conditions on Mars.
Kuiper, Gerard P.,
The Atmospheres of the Earth and Planets, 1949, University of
Chicago Press, Chicago, Ill. -
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1949 - Then the pendulum swung
back. It was all a mistake. The canals were optical illusions,
caused by eyestrain and by the effort to see details below the
limits of visibility. Those color changes, and especially those
reported by Percival Lowell from his Flagstaff Observatory built
especially for the purpose of establishing the Martians were mere
wishful thinking. The dark areas were not seas but something like
the Asiatic salt steppes, only much saltier, too salty for anything
to grow. And even the white polar caps which were to have furnished
the irrigation water were not water at all but frozen carbon
dioxide- not ice, but dry ice.
Suppose all these
dismal statements were correct (which they are not), Mars would have
remained a highly interesting planet. But after all the imaginative
tracing of Martian superengineering, the disappointment, especially
to the layman, was enormous.
The present
concepts of Mars: There are no real mountains on Mars. The polar
caps are water, or rather, ice. We are justified in believing in
life on Mars- hardy plant life. And as of 1949, the canals of Mars
do exist.
Ley, Willy, The
Conquest of Space, 1949, The Viking Press, New York. -
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1950 - As we
look in on another world and try to understand what
is occuring there we see in the generally
reddish surface a desert where nothing flourishes. The white polar
caps are rather thin snow fields. The seas and fine dark markings
may well be depressions which catch enough water to promote the
growth of some hardy types of vegetation.
The times of the
Martian year when the dark markings change in intensity and color
are such as would be expected if the changes are caused by the
growth and decline of vegetation. This seems to be true of the
canals as well. Kuiper's studies of sunlight reflected from the
green areas seem to rule out familiar seed plants and ferns. They
suggest but do not definitely establish the presence of lichens and
certain hardy mosses.
The hazy
atmosphere of Mars itself affects the view of the planet's surface.
Kuiper's observations at McDonald Observatory lead him to suppose
that the haze is caused by ice crystals in the atmosphere of the
planet, similar to the light cirrus clouds in our own atmosphere. At
times the haze clears rapidly over a large area of the planet.
Baker, Robert H., Astronomy, 1950, D.
Van Nostrand Co., New York. -
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1953 -
Carbon dioxide has not been detected in the Martian atmosphere. This
is not surprising because carbon dioxide must be present in large
quantity before it will produce absorptions of sufficient strength
to be detected.
As we have
mentioned, the color of the surface of Mars provides sure evidence
of the presence of free oxygen, at any rate in the past. The
presence of free oxygen almost certainly demands the existence of
vegetation. Combining this argument with the evidence from the
changes that occur on the surface, we may conclude that it is almost
certain that there is some form of vegetation on Mars. If this
conclusion is accepted, it follows that life does not occur as the
result of a special act of creation or because of some unique
accident, but that it is the result of the occurrence of definite
processes; given suitable conditions, these processes will
inevitably lead to the development of life.
Jones, H. Spencer, Life on Other
Worlds, 1953, The New American Library,
New York. - back
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1955 -
Kuiper considers the rocks are composed of igneous rock, similar to
felsite; but H. Spencer Jones suggests that the distinctly ruddy
tint is due to the "oxidation of iron-bearing ores by atmospheric
oxygen". So we probably do not greatly err in believing that the
reddish-ochre stretches which give the planet its distinctive color
consist of sandy desert alternating with rusty rocks. The low
reflective capacity of the planet, which sends back only 15 percent
of the light which it receives confirms
this supposition. The desert regions appear to be about two thousand
feet above the level of the lower areas and to consist of plateaux,
diversified by valleys and crevices but comparatively flat. There
are no ranges of mountians on the planet nor
even high hills.
Macpherson, Hector, Guide to the
Stars, 1955, Philosophical Library, New York. -
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1964 - The
conspicuous red color apparently comes from regions not too
different from various deserts of the earth, such as the Painted
Desert of Arizona. White "buttons" on the two polar caps, which vary
in size with Martian seasons, are undoubtedly formed from ice-
presumably a thin layer of hoarfrost- which completely vanishes
during the Martian summer. Water is a scarce commodity; the planet
possesses no discernible oceans or lakes. The grayish areas, once
thought to be water, show seasonal changes suggestive of vegetation,
but their precise nature has not yet been determined. They may be a
form of moss or lichen.
Menzel, Donald H.
, A Field Guide to the Stars and Planets, 1964, Houghton
Mifflin Co., Boston. -
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1976 - (Tom Mutch, speaking about the Mariner
spacecraft discoveries that there were no oceans, no canals, no
vegetation on Mars)
To a geologist,
each day's pictures were like a new traverse across unfamiliar
terrain. Progressively revealed as a new planet,
detail emerging from obscurity with overwhelming rapidity.
Immense fracture systems spread across the planet as a new geologic
map was constructed. Near the telescopic feature, Argyre, a basin
the size of the lunar Imbrium Basin was identified. Hellas, whose
western margin was seen in pictures taken by the Mariner '69
mission was revealed in its entirety.
Strange tributaries and fluvial-like forms were seen scattered
across the equatorial region. Sinuous ridges resembling lunar mare
ridges were seen. Lobate flow fronts suggesting basaltic outpouring
were observed. The new pictures quickly erased from memory the "old"
Mars as though the countless hours of previous speculation had been
little more than science fiction.
Mutch, Thomas A. et al, The Geology of
Mars, 1976, Princeton University Press, Princeton, N.J. -
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1980 - As telescopes improved and the
equipment used with them grew more sophisticated, the image of Mars
began to change. The first challenges came from a series of
temperature measurements. Mars is cold. The average temperature on
Mars falls far below the freezing point of water. Under these
conditions, any channels of liquid water, natural or Martian made,
appear highly unlikely.
By the early
1960's, astronomers knew that Martian "air" consists mostly of
carbon dioxide, with only a trace of water vapor.
The total amount of gas in the Martian
atmosphere, and the pressure that the atmosphere exerts at the
Martian surface, must be less than one percent of the values for our
atmosphere. The surface pressure plays an important role in
the speculation about the possible existence of life on Mars,
because if the Martian atmosphere does not exert at least 0.6
percent of our atmosphere's pressure, then water cannot exist as a
liquid, no matter what the surface temperature may be. Without
liquid water, life as we know it cannot exist.
Goldsmith, Donald and Owen, Tobias,
The Search for Life in the Universe,
1980, Benjamin Cummings Publishing Co., Menlo Park, Ca. -
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1996 -The Mariner 4 results spurred
astronomers to completely revise their ideas about Mars; it was now
obvious that earlier views had been very wide of the mark indeed.
The vegetation theory was dead- the Martian environment seemed to be
too hostile to support vegetation, and even the existence of the
wave of darkening, which "took second place only to the Martian
canals in historical development of the life on Mars hypothesis" was
doubtful. Though there could be no question that there were
considerable changes in the form and intensity of the dark areas,
the existence of an actual "wave" extending from the south pole to
the equator each spring seemed at best only weakly supported by the
observations. A study by Charles Capen of the Lowell Observatory
showed systematic latitudinal changes in the intensity of features
with the seasons, at least, did not seem to occur, and any changes
that did take place were evidently due to windblown dust rather than
vegetation. Carl Sagan describes this as "the alternate deposition
and deflation of windblown dust having detectable contrast with
respect to basement material".
Sheehan, William,
The Planet Mars, 1996, The University of
Arizona Press, Tucson. -
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CONCLUSION: IT'S DUST, BLOWIN IN THE
WIND, MESSIN WITH OUR MINDS |